<?xml version='1.0' encoding='UTF-8'?><?xml-stylesheet href="http://www.blogger.com/styles/atom.css" type="text/css"?><feed xmlns='http://www.w3.org/2005/Atom' xmlns:openSearch='http://a9.com/-/spec/opensearchrss/1.0/' xmlns:georss='http://www.georss.org/georss' xmlns:gd='http://schemas.google.com/g/2005' xmlns:thr='http://purl.org/syndication/thread/1.0'><id>tag:blogger.com,1999:blog-28009426</id><updated>2011-06-07T23:21:58.513-07:00</updated><title type='text'>Neutrino Astrophysics literature</title><subtitle type='html'>A collection of recent references on neutrino astrophysics, as they appear online (see link to the arXiv)</subtitle><link rel='http://schemas.google.com/g/2005#feed' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/posts/default'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default?max-results=100'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/'/><link rel='hub' href='http://pubsubhubbub.appspot.com/'/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><generator version='7.00' uri='http://www.blogger.com'>Blogger</generator><openSearch:totalResults>33</openSearch:totalResults><openSearch:startIndex>1</openSearch:startIndex><openSearch:itemsPerPage>100</openSearch:itemsPerPage><entry><id>tag:blogger.com,1999:blog-28009426.post-116473379987091496</id><published>2006-11-28T09:02:00.000-08:00</published><updated>2006-11-28T09:10:00.016-08:00</updated><title type='text'></title><content type='html'>New Hubble Space Telescope Discoveries of Type Ia Supernovae at z&gt;=1: Narrowing Constraints on the Early Behavior of Dark Energy.&lt;br /&gt;&lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/hep/wwwauthors?key=6982530"&gt;Adam G. Riess et al.&lt;/a&gt; 46455850950, Nov 2006. 82pp.&lt;br /&gt;&lt;a href="http://hubblesite.org/newscenter/archive/releases/2006/52/"&gt;Press Release&lt;/a&gt;. Submitted to Astrophys.J. e-Print Archive: astro-ph/0611572&lt;br /&gt;&lt;a href="http://arxiv.org/abs/astro-ph/0611572"&gt;Abstract &lt;/a&gt;and &lt;a href="http://arxiv.org/ps/astro-ph/0611572"&gt;Postscript&lt;/a&gt; and &lt;a href="http://arxiv.org/pdf/astro-ph/0611572"&gt;PDF&lt;/a&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-116473379987091496?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/116473379987091496/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=116473379987091496' title='2 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116473379987091496'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116473379987091496'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/11/new-hubble-space-telescope-discoveries.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>2</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-116473249891571340</id><published>2006-11-28T08:39:00.000-08:00</published><updated>2006-11-28T08:48:18.926-08:00</updated><title type='text'></title><content type='html'>Dark matter sterile neutrinos in stellar collapse: Alteration of energy/lepton number transport and a mechanism for supernova explosion enhancement.&lt;br /&gt;&lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Hidaka,"&gt;Jun Hidaka&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Fuller,"&gt;George M. Fuller&lt;/a&gt;. Sep 2006. 13pp. e-Print Archive: astro-ph/0609425&lt;br /&gt;&lt;a href="http://arxiv.org/abs/astro-ph/0609425"&gt;Abstract &lt;/a&gt;and &lt;a href="http://arxiv.org/ps/astro-ph/0609425"&gt;Postscript&lt;/a&gt; and &lt;a href="http://arxiv.org/pdf/astro-ph/0609425"&gt;PDF&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;Limits on the Radiative Decay of Sterile Neutrino Dark Matter from the Unresolved Cosmic and Soft X-ray Backgrounds.&lt;br /&gt;&lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Abazajian,"&gt;Kevork N. Abazajian&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Markevitch,Maxim%22"&gt;Maxim Markevitch&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Koushiappas,Savvas"&gt;Savvas M. Koushiappas&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Hickox,"&gt;Ryan C. Hickox&lt;/a&gt;. UMD-PP-06-057, LA-UR-06-3820, Nov 2006. 8pp. Submitted to Phys.Rev.D e-Print Archive: astro-ph/0611144&lt;br /&gt;&lt;a href="http://arxiv.org/abs/astro-ph/0611144"&gt;Abstract &lt;/a&gt;and &lt;a href="http://arxiv.org/ps/astro-ph/0611144"&gt;Postscript&lt;/a&gt; and &lt;a href="http://arxiv.org/pdf/astro-ph/0611144"&gt;PDF&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;Neutrino Oscillations Induced by Chiral Phase Transition in a Compact Star.&lt;br /&gt;&lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Mu,"&gt;Cheng-Fu Mu&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Sun,Gao-Feng%22"&gt;Gao-Feng Sun&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Zhuang,"&gt;Peng-Fei Zhuang&lt;/a&gt;. Nov 2006. 11pp. e-Print Archive: astro-ph/0611146&lt;br /&gt;&lt;a href="http://arxiv.org/abs/astro-ph/0611146"&gt;Abstract &lt;/a&gt;and &lt;a href="http://arxiv.org/ps/astro-ph/0611146"&gt;Postscript&lt;/a&gt; and &lt;a href="http://arxiv.org/pdf/astro-ph/0611146"&gt;PDF&lt;/a&gt;&lt;br /&gt;&lt;br /&gt;TeV gamma-rays and neutrinos from photo-disintegration of nuclei in Cygnus OB2.&lt;br /&gt;&lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Anchordoqui,"&gt;Luis A. Anchordoqui&lt;/a&gt; , &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Beacom,"&gt;John F. Beacom&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Goldberg,Haim%22"&gt;Haim Goldberg&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Palomares-Ruiz,Sergio%22"&gt;Sergio Palomares-Ruiz&lt;/a&gt;, &lt;a style="TEXT-DECORATION: none" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Weiler,"&gt;Thomas J. Weiler&lt;/a&gt;. Nov 2006. 19pp. e-Print Archive: astro-ph/0611581&lt;br /&gt;&lt;a href="http://arxiv.org/abs/astro-ph/0611581"&gt;Abstract &lt;/a&gt;and &lt;a href="http://arxiv.org/ps/astro-ph/0611581"&gt;Postscript&lt;/a&gt; and &lt;a href="http://arxiv.org/pdf/astro-ph/0611581"&gt;PDF&lt;/a&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-116473249891571340?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/116473249891571340/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=116473249891571340' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116473249891571340'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116473249891571340'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/11/dark-matter-sterile-neutrinos-in.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-116058494168593764</id><published>2006-10-11T09:40:00.000-07:00</published><updated>2006-10-11T09:42:21.700-07:00</updated><title type='text'>General Upper Bound on the Dark Matter Total Annihilation Cross Section</title><content type='html'>&lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608090&lt;/b&gt; [&lt;a href="http://www.arxiv.org/abs/astro-ph/0608090"&gt;abs&lt;/a&gt;, &lt;a href="http://www.arxiv.org/ps/astro-ph/0608090"&gt;ps&lt;/a&gt;, &lt;a href="http://www.arxiv.org/pdf/astro-ph/0608090"&gt;pdf&lt;/a&gt;, &lt;a href="http://www.arxiv.org/format/astro-ph/0608090"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;General Upper Bound on the Dark Matter Total Annihilation Cross Section&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://www.arxiv.org/find/astro-ph/1/au:+Beacom_J/0/1/0/all/0/1"&gt;John F. Beacom&lt;/a&gt; (Ohio State),  &lt;a href="http://www.arxiv.org/find/astro-ph/1/au:+Bell_N/0/1/0/all/0/1"&gt;Nicole F. Bell&lt;/a&gt; (Caltech),  &lt;a href="http://www.arxiv.org/find/astro-ph/1/au:+Mack_G/0/1/0/all/0/1"&gt;Gregory D. Mack&lt;/a&gt; (Ohio State)&lt;/b&gt;&lt;br /&gt;Comments: 4 pages, 3 figures&lt;/dd&gt; &lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-116058494168593764?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/116058494168593764/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=116058494168593764' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116058494168593764'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/116058494168593764'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/10/general-upper-bound-on-dark-matter.html' title='General Upper Bound on the Dark Matter Total Annihilation Cross Section'/><author><name>Orlando L. G. Peres</name><uri>http://www.blogger.com/profile/09954161437897021206</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115940280567855113</id><published>2006-09-27T17:15:00.000-07:00</published><updated>2006-09-27T17:20:05.683-07:00</updated><title type='text'></title><content type='html'>&lt;p&gt; 3) &lt;b&gt; Solar Model Parameters and Direct Measurements of Solar &lt;/b&gt;Neutrino&lt;b&gt; Fluxes.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Bandyopadhyay,%20Abhijit%22"&gt;Abhijit Bandyopadhyay&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Choubey,%20Sandhya%22"&gt;Sandhya Choubey&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Goswami,Srubabati%22"&gt;Srubabati Goswami&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Petcov,%20S.T.%22"&gt;S.T. Petcov&lt;/a&gt; . Aug 2006. 25pp. **&lt;br /&gt;e-Print Archive: &lt;b&gt;hep-ph/0608323&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/hep-ph/0608323"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/hep-ph/0608323"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/hep-ph/0608323"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 4) &lt;b&gt; Oscillations of solar atmosphere &lt;/b&gt;neutrino&lt;b&gt;s.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Fogli,%20G.L.%22"&gt;G.L. Fogli&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Lisi,%20E.%22"&gt;E. Lisi&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Mirizzi,A.%22"&gt;A. Mirizzi&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Montanino,%20D.%22"&gt;D. Montanino&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Serpico,P.D.%22"&gt;P.D. Serpico&lt;/a&gt; . MPP-2006-92, Aug 2006. 10pp. **&lt;br /&gt;e-Print Archive: &lt;b&gt;hep-ph/0608321&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/hep-ph/0608321"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/hep-ph/0608321"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/hep-ph/0608321"&gt;PDF&lt;/a&gt; from arXiv.org&lt;br /&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;br /&gt;&lt;p&gt; 11) &lt;b&gt; &lt;/b&gt;Neutrino&lt;b&gt; oscillation physics at an upgraded CNGS with large next generation liquid Argon TPC detectors.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Meregaglia,%20A.%22"&gt;A. Meregaglia&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Rubbia,%20A.%22"&gt;A. Rubbia&lt;/a&gt; . Sep 2006. 37pp. ** &lt;a href="http://www.slac.stanford.edu/spires/hep/te.html"&gt;Temporary entry&lt;/a&gt; **&lt;br /&gt;e-Print Archive: &lt;b&gt;hep-ph/0609106&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/hep-ph/0609106"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/hep-ph/0609106"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/hep-ph/0609106"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 12) &lt;b&gt; Probing long-range leptonic forces with solar and reactor &lt;/b&gt;neutrino&lt;b&gt;s.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Gonzalez-Garcia,%20M%20C%22"&gt;M C Gonzalez-Garcia&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22de%20Holanda,%20PC%22"&gt;P C de Holanda&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Masso,%20E%22"&gt;E Masso&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Zukanovich%20Funchal,R.%22"&gt;R. Zukanovich Funchal&lt;/a&gt; . Sep 2006. 20pp. **&lt;br /&gt;e-Print Archive: &lt;b&gt;hep-ph/0609094&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/hep-ph/0609094"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/hep-ph/0609094"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/hep-ph/0609094"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115940280567855113?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115940280567855113/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115940280567855113' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940280567855113'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940280567855113'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/09/3-solar-model-parameters-and-direct.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115940196458787149</id><published>2006-09-27T17:05:00.000-07:00</published><updated>2006-09-27T17:12:19.796-07:00</updated><title type='text'></title><content type='html'>&lt;p&gt; 7) &lt;b&gt; &lt;/b&gt;Neutrino&lt;b&gt; signals from the formation of black hole: A probe of equation of state of dense matter.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Sumiyoshi,%20Kohsuke%22"&gt;Kohsuke Sumiyoshi&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Numazu+Coll.+Tech."&gt;Numazu Coll. Tech.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Tokyo,+Astron.+Observ."&gt;Tokyo, Astron. Observ.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Yamada,S.%22"&gt;S. Yamada&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Waseda+U.,+RISE"&gt;Waseda U., RISE&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Suzuki,H.%22"&gt;H. Suzuki&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Sci.+U.,+Tokyo+-+Noda+Campus"&gt;Sci. U., Tokyo - Noda Campus&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Chiba,S.%22"&gt;S. Chiba&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=JAERI,+Tokai"&gt;JAERI, Tokai&lt;/a&gt;) . Aug 2006. 4pp.&lt;br /&gt;Published in &lt;b&gt;Phys.Rev.Lett.97:091101,2006&lt;/b&gt;&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608509&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608509"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608509"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608509"&gt;PDF&lt;/a&gt; from arXiv.org&lt;br /&gt;&lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 8) &lt;b&gt; Thermal &lt;/b&gt;neutrino&lt;b&gt;s from pre-supernova.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Odrzywolek,%20Andrzej%22"&gt;Andrzej Odrzywolek&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Misiaszek,%20M.%22"&gt;M. Misiaszek&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Jagiellonian+U."&gt;Jagiellonian U.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Kutschera,M.%22"&gt;M. Kutschera&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Jagiellonian+U."&gt;Jagiellonian U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Cracow,+INP"&gt;Cracow, INP&lt;/a&gt;) . Aug 2006.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608492&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608492"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608492"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608492"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt;&lt;p&gt; 10) &lt;b&gt; Astrophysical tau &lt;/b&gt;neutrino&lt;b&gt; detection in kilometer-scale Cherenkov detectors via muonic tau decay.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22DeYoung,%20Tyce%22"&gt;Tyce DeYoung&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Penn+State+U."&gt;Penn State U.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Razzaque,S.%22"&gt;S. Razzaque&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Cowen,%20D.F.%22"&gt;D.F. Cowen&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Penn+State+U.,+Astron.+Astrophys."&gt;Penn State U., Astron. Astrophys.&lt;/a&gt;) . Aug 2006. 6pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608486&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608486"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608486"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608486"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 11) &lt;b&gt; Is there a problem with low energy SN1987A &lt;/b&gt;neutrino&lt;b&gt;s?&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Costantini,%20MariaLaura%22"&gt;Maria Laura Costantini&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Ianni,%20Aldo%22"&gt;Aldo Ianni&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Pagliaroli,Giulia%22"&gt;Giulia Pagliaroli&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Vissani,%20Francesco%22"&gt;Francesco Vissani&lt;/a&gt; . Aug 2006. 8pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608399&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608399"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608399"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608399"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 12) &lt;b&gt; Light Element Signatures of Sterile &lt;/b&gt;Neutrino&lt;b&gt;s and Cosmological Lepton Numbers.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Smith,%20Christel%20J.%22"&gt;Christel J. Smith&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Fuller,%20GeorgeM.%22"&gt;George M. Fuller&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Kishimoto,%20Chad%20T.%22"&gt;Chad T. Kishimoto&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=UC,+San+Diego"&gt;UC, San Diego&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Abazajian,Kevork%20N.%22"&gt;Kevork N. Abazajian&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Los+Alamos"&gt;Los Alamos&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Maryland+U."&gt;Maryland U.&lt;/a&gt;) . LA-UR-06-2383, Aug 2006. 12pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608377&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608377"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608377"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608377"&gt;PDF&lt;/a&gt; from arXiv.org &lt;/dd&gt;&lt;/dl&gt;&lt;p&gt; 13) &lt;b&gt; The impact of &lt;/b&gt;neutrino&lt;b&gt; masses on the determination of dark energy properties.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22De%20La%20Macorra,%20Axel%22"&gt;Axel De La Macorra&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=UNAM,+Mexico"&gt;UNAM, Mexico&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Melchiorri,Alessandro%22"&gt;Alessandro Melchiorri&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Serra,%20Paolo%22"&gt;Paolo Serra&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Rome+U."&gt;Rome U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=INFN,+Rome"&gt;INFN, Rome&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Bean,Rachel%22"&gt;Rachel Bean&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Cornell+U.,+Astron.+Dept."&gt;Cornell U., Astron. Dept.&lt;/a&gt;) . Aug 2006. 4pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608351&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608351"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608351"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608351"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt;&lt;p&gt; 15) &lt;b&gt; Anisotropy of the Cosmic &lt;/b&gt;Neutrino&lt;b&gt; Background.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Michney,%20R.J.%22"&gt;R.J. Michney&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Caldwell,%20RobertR.%22"&gt;Robert R. Caldwell&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Dartmouth+Coll."&gt;Dartmouth Coll.&lt;/a&gt;) . Aug 2006. 5pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608303&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608303"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608303"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608303"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115940196458787149?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115940196458787149/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115940196458787149' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940196458787149'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940196458787149'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/09/7-neutrino-signals-from-formation-of.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115940190756574233</id><published>2006-09-27T17:02:00.000-07:00</published><updated>2006-09-27T17:13:03.126-07:00</updated><title type='text'></title><content type='html'>&lt;p&gt; 1) &lt;b&gt; Assessing The Starburst Contribution to the Gamma-Ray and &lt;/b&gt;Neutrino&lt;b&gt; Backgrounds.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Thompson,%20Todd%20A.%22"&gt;Todd A. Thompson&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Princeton+U."&gt;Princeton U.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Quataert,Eliot%22"&gt;Eliot Quataert&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=UC,+Berkeley,+Astron.+Dept."&gt;UC, Berkeley, Astron. Dept.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Waxman,Eli%22"&gt;Eli Waxman&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Weizmann+Inst."&gt;Weizmann Inst.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Loeb,Abraham%22"&gt;Abraham Loeb&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Harvard+U."&gt;Harvard U.&lt;/a&gt;) . Aug 2006. 3pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608699&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608699"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608699"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608699"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 2) &lt;b&gt; Self-induced conversion in dense &lt;/b&gt;neutrino&lt;b&gt; gases: Pendulum in flavour space.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Hannestad,%20Steen%22"&gt;Steen Hannestad&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Aarhus+U."&gt;Aarhus U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Munich,+Max+Planck+Inst."&gt;Munich, Max Planck Inst.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Raffelt,%20GeorgG.%22"&gt;Georg G. Raffelt&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Munich,+Max+Planck+Inst."&gt;Munich, Max Planck Inst.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Sigl,Gunter%22"&gt;Gunter Sigl&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=APC,+Paris"&gt;APC, Paris&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Paris,+Inst.+Astrophys."&gt;Paris, Inst. Astrophys.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Wong,%20YvonneY.Y.%22"&gt;Yvonne Y.Y. Wong&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Munich,+Max+Planck+Inst."&gt;Munich, Max Planck Inst.&lt;/a&gt;) . MPP-2006-102, Aug 2006. 20pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608695&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608695"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608695"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608695"&gt;PDF&lt;/a&gt; from arXiv.org &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 3) &lt;b&gt; &lt;/b&gt;Neutrino&lt;b&gt; pair annihilation near accreting, stellar-mass black holes.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Birkl,%20R.%22"&gt;R. Birkl&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Aloy,%20M.-A.%22"&gt;M.-A. Aloy&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Janka,H.-Th.%22"&gt;H.-Th. Janka&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Mueller,%20E.%22"&gt;E. Mueller&lt;/a&gt; . Aug 2006. 19pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608543&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608543"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608543"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608543"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt; &lt;p&gt; 4) &lt;b&gt; The r-Process in the Proto-Neutron-Star Winds with Anisotropic &lt;/b&gt;Neutrino&lt;b&gt; Emission.&lt;/b&gt;&lt;br /&gt;&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Wanajo,%20Shinya%22"&gt;Shinya Wanajo&lt;/a&gt; . Aug 2006. 8pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608539&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608539"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608539"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608539"&gt;PDF&lt;/a&gt; from arXiv.org  &lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115940190756574233?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115940190756574233/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115940190756574233' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940190756574233'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940190756574233'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/09/1-assessing-starburst-contribution-to.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115940162857035000</id><published>2006-09-27T16:56:00.000-07:00</published><updated>2006-09-27T17:00:28.576-07:00</updated><title type='text'></title><content type='html'>&lt;p&gt;&lt;b&gt; On the Law of Gravity, the Mass of &lt;/b&gt;Neutrino&lt;b&gt;s and the Proof of Dark Matter.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Angus,%20Garry%20W.%22"&gt;Garry W. Angus&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=St.+Andrews+U."&gt;St. Andrews U.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Shan,HuanYuan%22"&gt;HuanYuan Shan&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Zhao,%20HongSheng%22"&gt;HongSheng Zhao&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=St.+Andrews+U."&gt;St. Andrews U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Beijing+Observ."&gt;Beijing Observ.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Famaey,Benoit%22"&gt;Benoit Famaey&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Brussels+U.,+IAA"&gt;Brussels U., IAA&lt;/a&gt;) . Sep 2006. 5pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0609125&lt;/b&gt;&lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0609125"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0609125"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0609125"&gt;PDF&lt;/a&gt; from arXiv.org&lt;/dd&gt;&lt;/dl&gt;&lt;p&gt; &lt;b&gt; Ultrahigh Energy &lt;/b&gt;Neutrino&lt;b&gt;s in the Mediterranean: Detecting v(tau) and v(mu) with a km**3 Telescope.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Cuoco,%20Alessandro%22"&gt;Alessandro Cuoco&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Mangano,%20G.%22"&gt;G. Mangano&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Miele,%20G.%22"&gt;G. Miele&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Naples+U."&gt;Naples U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=INFN,+Naples"&gt;INFN, Naples&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Pastor,S.%22"&gt;S. Pastor&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Valencia+U."&gt;Valencia U.&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Perrone,L.%22"&gt;L. Perrone&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Lecce+U."&gt;Lecce U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=INFN,+Lecce"&gt;INFN, Lecce&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Pisanti,O.%22"&gt;O. Pisanti&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Naples+U."&gt;Naples U.&lt;/a&gt; &amp; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=INFN,+Naples"&gt;INFN, Naples&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Serpico,P.D.%22"&gt;P.D. Serpico&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Munich,+Max+Planck+Inst."&gt;Munich, Max Planck Inst.&lt;/a&gt;) .&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0609241&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0609241"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0609241"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0609241"&gt;PDF&lt;/a&gt; from arXiv.org&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115940162857035000?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115940162857035000/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115940162857035000' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940162857035000'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940162857035000'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/09/on-law-of-gravity-mass-of-neutrinos.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115940112295805157</id><published>2006-09-27T16:49:00.000-07:00</published><updated>2006-09-27T16:52:02.980-07:00</updated><title type='text'></title><content type='html'>&lt;p&gt;&lt;b&gt; Dark matter sterile &lt;/b&gt;neutrino&lt;b&gt;s in stellar collapse: Alteration of energy/lepton number transport and a mechanism for &lt;/b&gt;supernova&lt;b&gt; explosion enhancement.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Hidaka,%20Jun%22"&gt;Jun Hidaka&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Fuller,%20GeorgeM.%22"&gt;George M. Fuller&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=UC,+San+Diego"&gt;UC, San Diego&lt;/a&gt;) . Sep 2006. 13pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0609425&lt;/b&gt; &lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://www.slac.stanford.edu/spires/find/hep/wwwrefs?key=6904394"&gt; References &lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6904394&amp;FORMAT=WWWBRIEFLATEX"&gt;LaTeX(US)&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6904394&amp;amp;FORMAT=WWWBRIEFLATEX2"&gt;LaTeX(EU)&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6904394&amp;FORMAT=WWWBRIEFHARVMAC"&gt;Harvmac&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6904394&amp;amp;FORMAT=WWWBRIEFBIBTEX"&gt;BibTeX&lt;/a&gt; &lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0609425"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0609425"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0609425"&gt;PDF&lt;/a&gt; from arXiv.org&lt;/dd&gt;&lt;/dl&gt;&lt;p&gt;&lt;b&gt; Coherent Development of &lt;/b&gt;Neutrino&lt;b&gt; Flavor in the &lt;/b&gt;Supernova&lt;b&gt; Environment.&lt;/b&gt;&lt;br /&gt; &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Duan,%20Huaiyu%22"&gt;Huaiyu Duan&lt;/a&gt;, &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Fuller,%20GeorgeM.%22"&gt;George M. Fuller&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=UC,+San+Diego"&gt;UC, San Diego&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Carlson,J.%22"&gt;J. Carlson&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Los+Alamos"&gt;Los Alamos&lt;/a&gt;) ,  &lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/wwwhepau/wwwscan?rawcmd=fin+%22Qian,Yong-Zhong%22"&gt;Yong-Zhong Qian&lt;/a&gt; (&lt;a style="text-decoration: none;" href="http://www.slac.stanford.edu/spires/find/inst/www?icncp=Minnesota+U."&gt;Minnesota U.&lt;/a&gt;) . LA-UR-06-4692, Aug 2006. 4pp.&lt;br /&gt;e-Print Archive: &lt;b&gt;astro-ph/0608050&lt;/b&gt;&lt;a href="http://www.slac.stanford.edu/spires/find/hep/wwwrefs?key=6862527"&gt;&lt;br /&gt;&lt;/a&gt;&lt;/p&gt;&lt;p&gt;&lt;a href="http://www.slac.stanford.edu/spires/find/hep/wwwrefs?key=6862527"&gt;References &lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6862527&amp;FORMAT=WWWBRIEFLATEX"&gt;LaTeX(US)&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6862527&amp;amp;FORMAT=WWWBRIEFLATEX2"&gt;LaTeX(EU)&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6862527&amp;FORMAT=WWWBRIEFHARVMAC"&gt;Harvmac&lt;/a&gt;  | &lt;a href="http://www.slac.stanford.edu/spires/find/hep/www?key=6862527&amp;amp;FORMAT=WWWBRIEFBIBTEX"&gt;BibTeX&lt;/a&gt; | Cited &lt;a href="http://www.slac.stanford.edu/spires/find/hep?c=ASTRO-PH+0608050"&gt; 2 times &lt;/a&gt;&lt;/p&gt;&lt;dl&gt;&lt;dd&gt; &lt;a href="http://arxiv.org/abs/astro-ph/0608050"&gt; Abstract &lt;/a&gt; and &lt;a href="http://arxiv.org/ps/astro-ph/0608050"&gt;Postscript&lt;/a&gt;  and &lt;a href="http://arxiv.org/pdf/astro-ph/0608050"&gt;PDF&lt;/a&gt; from arXiv.org&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115940112295805157?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115940112295805157/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115940112295805157' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940112295805157'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115940112295805157'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/09/dark-matter-sterile-neutrinos-in.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115584854538038648</id><published>2006-08-17T13:49:00.000-07:00</published><updated>2006-08-17T14:02:25.403-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0608138&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/hep-ph/0608138"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/hep-ph/0608138"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/hep-ph/0608138"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/hep-ph/0608138"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;A-term inflation and the smallness of neutrino masses&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Allahverdi_R/0/1/0/all/0/1"&gt;Rouzbeh Allahverdi&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Kusenko_A/0/1/0/all/0/1"&gt;Alexander Kusenko&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/hep-ph/1/au:+Mazumdar_A/0/1/0/all/0/1"&gt;Anupam Mazumdar&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608017&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0608017"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0608017"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0608017"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0608017"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Revised WMAP constraints on neutrino masses and other extensions of the   minimal $\Lambda$CDM model&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kristiansen_J/0/1/0/all/0/1"&gt;Jostein R. Kristiansen&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Eriksen_H/0/1/0/all/0/1"&gt;Hans Kristian Eriksen&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Elgaroy_O/0/1/0/all/0/1"&gt;Oystein Elgaroy&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608313&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0608313"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0608313"&gt;pdf&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;A new type of massive stellar death: no supernovae from two nearby long   gamma ray bursts&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt; Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fynbo_J/0/1/0/all/0/1"&gt;Johan P. U. Fynbo&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Watson_D/0/1/0/all/0/1"&gt;Darach Watson&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Thoene_C/0/1/0/all/0/1"&gt;Christina C. Thoene&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Sollerman_J/0/1/0/all/0/1"&gt;Jesper Sollerman&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Bloom_J/0/1/0/all/0/1"&gt;Joshua S. Bloom&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Davis_T/0/1/0/all/0/1"&gt;Tamara M. Davis&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hjorth_J/0/1/0/all/0/1"&gt;Jens Hjorth&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jakobsson_P/0/1/0/all/0/1"&gt;Pall Jakobsson&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Joergensen_U/0/1/0/all/0/1"&gt;Uffe G. Joergensen&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cassan_A/0/1/0/all/0/1"&gt;Arnaud Cassan&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ceron_J/0/1/0/all/0/1"&gt;José María Castro Cerón&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Gorosabel_J/0/1/0/all/0/1"&gt;Javier Gorosabel&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Hinse_T/0/1/0/all/0/1"&gt;Tobias C. Hinse&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Jensen_B/0/1/0/all/0/1"&gt;Brian L. Jensen&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Klose_S/0/1/0/all/0/1"&gt;Sylvio Klose&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kocevski_D/0/1/0/all/0/1"&gt;Daniel Kocevski&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perley_D/0/1/0/all/0/1"&gt;Daniel Perley&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ramirez_Ruiz_E/0/1/0/all/0/1"&gt;Enrico Ramirez-Ruiz&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Stritzinger_M/0/1/0/all/0/1"&gt;Maximilian D. Stritzinger&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Vreeswijk_P/0/1/0/all/0/1"&gt;Paul Vreeswijk&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wijers_R/0/1/0/all/0/1"&gt;Ralph A. M. Wijers&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Woller_K/0/1/0/all/0/1"&gt;Kristian G. Woller&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Zub_M/0/1/0/all/0/1"&gt;Marta Zub&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Xu_D/0/1/0/all/0/1"&gt;Dong Xu&lt;/a&gt;&lt;/b&gt;&lt;/dt&gt;&lt;dd&gt;&lt;br /&gt;&lt;/dd&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608341&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0608341"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0608341"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0608341"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0608341"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a   25 Solar Mass Supernova Model&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Rapp_W/0/1/0/all/0/1"&gt;W. Rapp&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Goerres_J/0/1/0/all/0/1"&gt;J. Goerres&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Wiescher_M/0/1/0/all/0/1"&gt;M. Wiescher&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schatz_H/0/1/0/all/0/1"&gt;H. Schatz&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Kaeppeler_F/0/1/0/all/0/1"&gt;F. Kaeppeler&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115584854538038648?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115584854538038648/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115584854538038648' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115584854538038648'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115584854538038648'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/08/hep-ph0608138-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115525007591461066</id><published>2006-08-10T15:46:00.000-07:00</published><updated>2006-08-10T15:47:55.930-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608206&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0608206"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0608206"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0608206"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0608206"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Sterile neutrinos, lepton asymmetries, primordial elements: how much of   each?&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Chu_Y/0/1/0/all/0/1"&gt;Yi-Zen Chu&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Cirelli_M/0/1/0/all/0/1"&gt;Marco Cirelli&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115525007591461066?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115525007591461066/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115525007591461066' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115525007591461066'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115525007591461066'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/08/astro-ph0608206-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115501232725298309</id><published>2006-08-07T21:41:00.000-07:00</published><updated>2006-08-07T21:45:27.270-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0608060&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0608060"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0608060"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0608060"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0608060"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Observables sensitive to absolute neutrino masses: A reappraisal after   WMAP-3y and first MINOS results&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Fogli_G/0/1/0/all/0/1"&gt;G.L. Fogli&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Lisi_E/0/1/0/all/0/1"&gt;E. Lisi&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Marrone_A/0/1/0/all/0/1"&gt;A. Marrone&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Melchiorri_A/0/1/0/all/0/1"&gt;A. Melchiorri&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Palazzo_A/0/1/0/all/0/1"&gt;A. Palazzo&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Serra_P/0/1/0/all/0/1"&gt;P. Serra&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Silk_J/0/1/0/all/0/1"&gt;J. Silk&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Slosar_A/0/1/0/all/0/1"&gt;A. Slosar&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608103&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0608103"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0608103"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0608103"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0608103"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Relaxed constraints on neutrino oscillation parameters&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kirilova_D/0/1/0/all/0/1"&gt;Daniela P. Kirilova&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Panayotova_M/0/1/0/all/0/1"&gt;Mariana P. Panayotova&lt;/a&gt;&lt;/b&gt;&lt;br /&gt; &lt;br /&gt;&lt;/dd&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0608130&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0608130"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0608130"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0608130"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0608130"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Star formation rate in the solar neighborhood&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Cignoni_M/0/1/0/all/0/1"&gt;Michele Cignoni&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115501232725298309?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115501232725298309/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115501232725298309' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115501232725298309'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115501232725298309'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/08/hep-ph0608060-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115446606932451835</id><published>2006-08-01T13:56:00.000-07:00</published><updated>2006-08-01T14:01:09.340-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607341&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607341"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607341"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607341"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607341"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Neutrino emission from compact stars and inhomogeneous color   superconductivity&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Anglani_R/0/1/0/all/0/1"&gt;R. Anglani&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Mannarelli_M/0/1/0/all/0/1"&gt;M. Mannarelli&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Nardulli_G/0/1/0/all/0/1"&gt;G. Nardulli&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Ruggieri_M/0/1/0/all/0/1"&gt;M. Ruggieri&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;    &lt;/dt&gt;   &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607324&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607324"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607324"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607324"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607324"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Determination of the Atmospheric Neutrino Fluxes from Atmospheric   Neutrino Data&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Gonzalez_Garcia_M/0/1/0/all/0/1"&gt;M.C. Gonzalez-Garcia&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Maltoni_M/0/1/0/all/0/1"&gt;M. Maltoni&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Rojo_J/0/1/0/all/0/1"&gt;J. Rojo&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt; &lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607674&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607674"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607674"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607674"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607674"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Cosmic Supernova Rates and the Hubble Sequence&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Calura_F/0/1/0/all/0/1"&gt;F. Calura&lt;/a&gt; (1),  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Matteucci_F/0/1/0/all/0/1"&gt;F. Matteucci&lt;/a&gt;&lt;/b&gt;&lt;b&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115446606932451835?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115446606932451835/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115446606932451835' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115446606932451835'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115446606932451835'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/08/hep-ph0607341-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115402163060553971</id><published>2006-07-27T10:33:00.000-07:00</published><updated>2006-07-27T10:33:50.630-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607281&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607281"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607281"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607281"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607281"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Probing Late Neutrino Mass Properties with Supernova Neutrinos&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Baker_J/0/1/0/all/0/1"&gt;J. Baker&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Goldberg_H/0/1/0/all/0/1"&gt;H. Goldberg&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Perez_G/0/1/0/all/0/1"&gt;G. Perez&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Sarcevic_I/0/1/0/all/0/1"&gt;I. Sarcevic&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115402163060553971?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115402163060553971/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115402163060553971' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115402163060553971'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115402163060553971'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/hep-ph0607281-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115392976698772577</id><published>2006-07-26T08:57:00.000-07:00</published><updated>2006-07-26T09:02:47.010-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607564&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607564"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607564"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607564"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607564"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Neutrino Scattering in Heterogeneous Supernova Plasmas&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Caballero_O/0/1/0/all/0/1"&gt;O.L Caballero&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Horowitz_C/0/1/0/all/0/1"&gt;C. J. Horowitz&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Berry_D/0/1/0/all/0/1"&gt;D. K. Berry&lt;/a&gt; (Indiana U.)&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607267&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607267"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607267"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607267"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607267"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Effects of non-standard neutrino-electron interactions on relic neutrino   decoupling&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Mangano_G/0/1/0/all/0/1"&gt;Gianpiero Mangano&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Miele_G/0/1/0/all/0/1"&gt;Gennaro Miele&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Pastor_S/0/1/0/all/0/1"&gt;Sergio Pastor&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Pinto_T/0/1/0/all/0/1"&gt;Teguayco Pinto&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Pisanti_O/0/1/0/all/0/1"&gt;Ofelia Pisanti&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Serpico_P/0/1/0/all/0/1"&gt;Pasquale D. Serpico&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115392976698772577?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115392976698772577/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115392976698772577' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115392976698772577'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115392976698772577'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607564-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115385394210232816</id><published>2006-07-25T11:51:00.000-07:00</published><updated>2006-07-25T11:59:02.120-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607527&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607527"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607527"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607527"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607527"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Neutrino-Neutrino Interactions and Flavor Mixing in Dense Matter&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Balantekin_A/0/1/0/all/0/1"&gt;A.B. Balantekin&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Pehlivan_Y/0/1/0/all/0/1"&gt;Y. Pehlivan&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607521&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607521"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607521"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607521"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607521"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Inverse Compton scattering on solar photons, heliospheric modulation,   and neutrino astrophysics&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Moskalenko_I/0/1/0/all/0/1"&gt;Igor V. Moskalenko&lt;/a&gt; (Stanford),  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Porter_T/0/1/0/all/0/1"&gt;Troy A. Porter&lt;/a&gt; (UCSC),  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Digel_S/0/1/0/all/0/1"&gt;Seth W. Digel&lt;/a&gt; (SLAC)&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115385394210232816?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115385394210232816/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115385394210232816' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115385394210232816'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115385394210232816'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607527-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115343296723606212</id><published>2006-07-20T14:57:00.000-07:00</published><updated>2006-07-20T15:02:47.250-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607427&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607427"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607427"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607427"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607427"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Astrophysical implications of high energy neutrino limits I. Overall   diffuse limits&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Becker_J/0/1/0/all/0/1"&gt;Julia K. Becker&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Rhode_W/0/1/0/all/0/1"&gt;Wolfgang Rhode&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Biermann_P/0/1/0/all/0/1"&gt;Peter L. Biermann&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Muenich_K/0/1/0/all/0/1"&gt;Kirsten Muenich&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115343296723606212?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115343296723606212/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115343296723606212' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115343296723606212'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115343296723606212'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607427-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115334572006094869</id><published>2006-07-19T14:44:00.000-07:00</published><updated>2006-07-19T14:48:40.076-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607176&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607176"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607176"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607176"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607176"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Spectral Distortions at Super-Kamiokande&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Dev_S/0/1/0/all/0/1"&gt;S. Dev&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Kumar_S/0/1/0/all/0/1"&gt;Sanjeev Kumar&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt; &lt;/dt&gt;&lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607368&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607368"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607368"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607368"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607368"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;LS I +61 303 as a potential neutrino source on the light of MAGIC   results&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Torres_D/0/1/0/all/0/1"&gt;Diego F. Torres&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Halzen_F/0/1/0/all/0/1"&gt;Francis Halzen&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt; &lt;/dt&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607403&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607403"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607403"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607403"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607403"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Coherent Active-Sterile Neutrino Flavor Transformation in the Early   Universe&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kishimoto_C/0/1/0/all/0/1"&gt;Chad T. Kishimoto&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Fuller_G/0/1/0/all/0/1"&gt;George M. Fuller&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Smith_C/0/1/0/all/0/1"&gt;Christel J. Smith&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115334572006094869?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115334572006094869/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115334572006094869' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115334572006094869'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115334572006094869'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/hep-ph0607176-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115316219553678383</id><published>2006-07-17T11:44:00.000-07:00</published><updated>2006-07-17T11:49:55.546-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607315&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607315"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607315"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607315"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607315"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Cosmological Information from Lensed CMB Power Spectra&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Smith_K/0/1/0/all/0/1"&gt;Kendrick M. Smith&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Hu_W/0/1/0/all/0/1"&gt;Wayne Hu&lt;/a&gt; (KICP, UChicago),  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kaplinghat_M/0/1/0/all/0/1"&gt;Manoj Kaplinghat&lt;/a&gt; (UC Irvine)&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607316&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607316"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607316"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607316"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607316"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Supernovae, Lensed CMB and Dark Energy&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Hu_W/0/1/0/all/0/1"&gt;Wayne Hu&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Huterer_D/0/1/0/all/0/1"&gt;Dragan Huterer&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Smith_K/0/1/0/all/0/1"&gt;Kendrick M. Smith&lt;/a&gt; (KICP, UChicago)&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt; &lt;/dt&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115316219553678383?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115316219553678383/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115316219553678383' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115316219553678383'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115316219553678383'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607315-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115291963864744355</id><published>2006-07-14T16:22:00.000-07:00</published><updated>2006-07-14T16:27:18.660-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607281&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607281"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607281"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607281"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607281"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;A Numerical Algorithm for Modeling Multigroup Neutrino-Radiation   Hydrodynamics in Two Spatial Dimensions&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Swesty_F/0/1/0/all/0/1"&gt;F. Douglas Swesty&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Myra_E/0/1/0/all/0/1"&gt;Eric S. Myra&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607286&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607286"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607286"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607286"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607286"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Potential Neutrino Signals from Galactic Gamma-Ray Sources&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kappes_A/0/1/0/all/0/1"&gt;Alexander Kappes&lt;/a&gt; ,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Hinton_J/0/1/0/all/0/1"&gt;Jim Hinton&lt;/a&gt; ,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Stegmann_C/0/1/0/all/0/1"&gt;Christian Stegmann&lt;/a&gt; ,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Aharonian_F/0/1/0/all/0/1"&gt;Felix A. Aharonian&lt;/a&gt;&lt;br /&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dt&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115291963864744355?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115291963864744355/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115291963864744355' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115291963864744355'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115291963864744355'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607281-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115281808072953349</id><published>2006-07-13T12:10:00.000-07:00</published><updated>2006-07-13T12:14:40.743-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607244&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607244"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607244"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607244"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607244"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Neutrino signatures of supernova turbulence&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Friedland_A/0/1/0/all/0/1"&gt;Alexander Friedland&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Gruzinov_A/0/1/0/all/0/1"&gt;Andrei Gruzinov&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607249&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607249"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607249"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607249"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607249"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Neutrinos from galactic sources of cosmic rays with known gamma-ray   spectra&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Vissani_F/0/1/0/all/0/1"&gt;Francesco Vissani&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dt&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115281808072953349?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115281808072953349/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115281808072953349' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115281808072953349'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115281808072953349'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607244-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115272112065175993</id><published>2006-07-12T09:08:00.000-07:00</published><updated>2006-07-12T09:18:40.666-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607224&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607224"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607224"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607224"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607224"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Gravitational Radiation from Standing Accretion Shock Instability in   Core-Collapse Supernovae&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kotake_K/0/1/0/all/0/1"&gt;Kei Kotake&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Ohnishi_N/0/1/0/all/0/1"&gt;Naofumi Ohnishi&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Yamada_S/0/1/0/all/0/1"&gt;Shoichi Yamada&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607233&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607233"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607233"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607233"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607233"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Limits on the high-energy gamma and neutrino fluxes from the SGR 1806-20   giant flare of December 27th, 2004 with the AMANDA-II detector&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; The &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Collaboration_IceCube/0/1/0/all/0/1"&gt;IceCube Collaboration&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0607109&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607109"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607109"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607109"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607109"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Probing Dark Energy via Neutrino &amp; Supernova Observatories&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Hall_L/0/1/0/all/0/1"&gt;Lawrence J. Hall&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Murayama_H/0/1/0/all/0/1"&gt;Hitoshi Murayama&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Papucci_M/0/1/0/all/0/1"&gt;Michele Papucci&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Perez_G/0/1/0/all/0/1"&gt;Gilad Perez&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ex/0607010&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ex/0607010"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ex/0607010"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ex/0607010"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ex/0607010"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;A Search for Neutrinos from the Solar hep Reaction and the Diffuse   Supernova Neutrino Background with the Sudbury Neutrino Observatory&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; The &lt;a href="http://xxx.lanl.gov/find/hep-ex/1/au:+Collaboration_SNO/0/1/0/all/0/1"&gt;SNO Collaboration&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115272112065175993?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115272112065175993/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115272112065175993' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115272112065175993'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115272112065175993'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607224-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115263452138307883</id><published>2006-07-11T09:15:00.000-07:00</published><updated>2006-07-11T09:15:22.323-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0607197&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607197"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607197"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607197"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607197"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Are Diffuse High Energy Neutrinos from Starburst Galaxies Observable?&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Stecker_F/0/1/0/all/0/1"&gt;F.W. Stecker&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;hep-ph/0607086&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607086"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607086"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607086"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607086"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Determining Supersymmetric Parameters With Dark Matter Experiments&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Hooper_D/0/1/0/all/0/1"&gt;Dan Hooper&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Taylor_A/0/1/0/all/0/1"&gt;Andrew M. Taylor&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;hep-ph/0607095&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0607095"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0607095"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0607095"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0607095"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Far Field Monitoring of Rogue Nuclear Activity with an Array of Large   anti-neutrino Detectors&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Guillian_E/0/1/0/all/0/1"&gt;Eugene Guillian&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115263452138307883?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115263452138307883/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115263452138307883' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115263452138307883'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115263452138307883'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607197-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115256529347446575</id><published>2006-07-10T14:01:00.000-07:00</published><updated>2006-07-10T14:01:33.756-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0607145&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607145"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607145"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607145"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607145"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Neutrino-Cooled Accretion Disks around Spinning Black Hole&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Chen_W/0/1/0/all/0/1"&gt;Wen-Xin Chen&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Beloborodov_A/0/1/0/all/0/1"&gt;Andrei M. Beloborodov&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt; &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0607143&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607143"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607143"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607143"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607143"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;   &lt;dd&gt; Title: &lt;b&gt;The beginning of the star formation epoch&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Mannucci_F/0/1/0/all/0/1"&gt;F. Mannucci&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Buttery_H/0/1/0/all/0/1"&gt;H. Buttery&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Maiolino_R/0/1/0/all/0/1"&gt;R. Maiolino&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Marconi_A/0/1/0/all/0/1"&gt;A. Marconi&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Pozzetti_L/0/1/0/all/0/1"&gt;L. Pozzetti&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt; &lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115256529347446575?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115256529347446575/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115256529347446575' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115256529347446575'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115256529347446575'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607145-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115230935982494929</id><published>2006-07-07T14:50:00.000-07:00</published><updated>2006-07-07T14:56:00.046-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;dt&gt;&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0606311&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0606311"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0606311"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0606311"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0606311"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Ultra high energy neutrino-nucleon cross section from cosmic ray   experiments and neutrino telescopes&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Barger_V/0/1/0/all/0/1"&gt;V. Barger&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Huber_P/0/1/0/all/0/1"&gt;Patrick Huber&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Marfatia_D/0/1/0/all/0/1"&gt;Danny Marfatia&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;    &lt;/dt&gt;   &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607104&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607104"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607104"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607104"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607104"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;High Energy Neutrinos and Cosmic-Rays from Low-Luminosity Gamma-Ray   Bursts?&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Murase_K/0/1/0/all/0/1"&gt;Kohta Murase&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Ioka_K/0/1/0/all/0/1"&gt;Kunihito Ioka&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Nagataki_S/0/1/0/all/0/1"&gt;Shigehiro Nagataki&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Nakamura_T/0/1/0/all/0/1"&gt;Takashi Nakamura&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dt&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607101&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607101"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607101"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607101"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607101"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Neutrino masses and cosmic radiation density: Combined analysis&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Hannestad_S/0/1/0/all/0/1"&gt;Steen Hannestad&lt;/a&gt; ,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Raffelt_G/0/1/0/all/0/1"&gt;Georg G.Raffelt&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607086&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607086"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607086"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607086"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607086"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Cosmology of neutrinos and extra light particles after WMAP3&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Cirelli_M/0/1/0/all/0/1"&gt;Marco Cirelli&lt;/a&gt;&lt;/b&gt;&lt;b&gt;  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Strumia_A/0/1/0/all/0/1"&gt;Alessandro Strumia&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115230935982494929?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115230935982494929/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115230935982494929' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115230935982494929'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115230935982494929'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/hep-ph0606311-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115222433932310028</id><published>2006-07-06T15:16:00.000-07:00</published><updated>2006-07-06T15:18:59.586-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607082&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607082"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607082"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607082"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607082"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Guaranteed and Prospective Galactic TeV Neutrino Sources&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kistler_M/0/1/0/all/0/1"&gt;Matthew D. Kistler&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Beacom_J/0/1/0/all/0/1"&gt;John F. Beacom&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115222433932310028?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115222433932310028/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115222433932310028' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115222433932310028'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115222433932310028'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607082-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115212645600931750</id><published>2006-07-05T12:00:00.000-07:00</published><updated>2006-07-05T12:07:36.270-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0607030&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0607030"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0607030"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0607030"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0607030"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Snapping Supernovae at z&gt;1.7&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Aldering_G/0/1/0/all/0/1"&gt;Greg Aldering&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kim_A/0/1/0/all/0/1"&gt;Alex G. Kim&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kowalski_M/0/1/0/all/0/1"&gt;Marek Kowalski&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Linder_E/0/1/0/all/0/1"&gt;Eric V. Linder&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Perlmutter_S/0/1/0/all/0/1"&gt;Saul Perlmutter&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115212645600931750?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115212645600931750/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115212645600931750' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115212645600931750'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115212645600931750'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/07/astro-ph0607030-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115159173494520381</id><published>2006-06-29T07:35:00.000-07:00</published><updated>2006-06-29T07:35:36.903-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;&lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606653&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0606653"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0606653"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0606653"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0606653"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Neutrino emission due to Cooper pairing in neutron stars&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leinson_L/0/1/0/all/0/1"&gt;L.B. Leinson&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perez_A/0/1/0/all/0/1"&gt;A. Perez&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606651&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0606651"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0606651"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0606651"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0606651"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;dl&gt;&lt;dd&gt; Title: &lt;b&gt;Vector current conservation and neutrino emission from singlet-paired   baryons in neutron stars&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Leinson_L/0/1/0/all/0/1"&gt;L.B. Leinson&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Perez_A/0/1/0/all/0/1"&gt;A. Perez&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606616&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0606616"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0606616"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0606616"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0606616"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;dl&gt;&lt;dd&gt; Title: &lt;b&gt;Simulation of Coherent Non-Linear Neutrino Flavor Transformation in the   Supernova Environment I: Correlated Neutrino Trajectories&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Duan_H/0/1/0/all/0/1"&gt;Huaiyu Duan&lt;/a&gt; (UCSD),  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fuller_G/0/1/0/all/0/1"&gt;George M. Fuller&lt;/a&gt; (UCSD),  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Carlson_J/0/1/0/all/0/1"&gt;J Carlson&lt;/a&gt; (LANL),  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Qian_Y/0/1/0/all/0/1"&gt;Yong-Zhong Qian&lt;/a&gt; (UMN)&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606607&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0606607"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0606607"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0606607"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0606607"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;dl&gt;&lt;dd&gt; Title: &lt;b&gt;Stellar Collapse Dynamics With Neutrino Flavor Changing Neutral Currents&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Amanik_P/0/1/0/all/0/1"&gt;Philip S. Amanik&lt;/a&gt;,  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Fuller_G/0/1/0/all/0/1"&gt;George M. Fuller&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt;&lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606316&lt;/b&gt; [&lt;a href="http://arxiv.org/abs/astro-ph/0606316"&gt;abs&lt;/a&gt;, &lt;a href="http://arxiv.org/ps/astro-ph/0606316"&gt;ps&lt;/a&gt;, &lt;a href="http://arxiv.org/pdf/astro-ph/0606316"&gt;pdf&lt;/a&gt;, &lt;a href="http://arxiv.org/format/astro-ph/0606316"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Probing Neutrino Dark Energy with Extremely High-Energy Cosmic Neutrinos&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Ringwald_A/0/1/0/all/0/1"&gt;Andreas Ringwald&lt;/a&gt; (DESY),  &lt;a href="http://arxiv.org/find/astro-ph/1/au:+Schrempp_L/0/1/0/all/0/1"&gt;Lily Schrempp&lt;/a&gt; (DESY)&lt;/b&gt;&lt;/dd&gt;&lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115159173494520381?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115159173494520381/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115159173494520381' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115159173494520381'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115159173494520381'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/06/astro-ph0606653-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-115136456790282151</id><published>2006-06-26T16:23:00.000-07:00</published><updated>2006-06-26T16:32:13.470-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606575&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0606575"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0606575"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0606575"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0606575"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Neutrino-Accelerated Hot Hydrogen Burning&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kishimoto_C/0/1/0/all/0/1"&gt;Chad T. Kishimoto&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Fuller_G/0/1/0/all/0/1"&gt;George M. Fuller&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt; &lt;/dl&gt; &lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606413&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0606413"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0606413"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0606413"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0606413"&gt;other&lt;/a&gt;] :&lt;/span&gt; &lt;dl&gt; &lt;dd&gt; Title: &lt;b&gt;High energy neutrino astronomy using upward-going muons in   Super-Kamiokande-I&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+al._K/0/1/0/all/0/1"&gt;K. Abe et al.&lt;/a&gt; (The Super-Kamiokande Collaboration)&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt; &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606504&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0606504"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0606504"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0606504"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0606504"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;   &lt;dd&gt; Title: &lt;b&gt;Standing Accretion Shocks in the Supernova Core: Effects of Convection   and Realistic EOS&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Yamasaki_T/0/1/0/all/0/1"&gt;Tatsuya Yamasaki&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Yamada_S/0/1/0/all/0/1"&gt;Shoichi Yamada&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;   &lt;dt&gt;&lt;br /&gt; &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0606450&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0606450"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0606450"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0606450"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0606450"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;   &lt;dd&gt; Title: &lt;b&gt;Supernova Fallback: A Possible Site for the r-Process&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Fryer_C/0/1/0/all/0/1"&gt;Chris L. Fryer&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Herwig_F/0/1/0/all/0/1"&gt;Falk Herwig&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Hungerford_A/0/1/0/all/0/1"&gt;Aimee Hungerford&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Timmes_F/0/1/0/all/0/1"&gt;Frank Timmes&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0606248&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0606248"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0606248"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0606248"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0606248"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;   &lt;dd&gt; Title: &lt;b&gt;Model Independent Bounds on Magnetic Moments of Majorana Neutrinos&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Bell_N/0/1/0/all/0/1"&gt;Nicole F. Bell&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Gorchtein_M/0/1/0/all/0/1"&gt;Mikhail Gorchtein&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Ramsey_Musolf_M/0/1/0/all/0/1"&gt;Michael J. Ramsey-Musolf&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Vogel_P/0/1/0/all/0/1"&gt;Petr Vogel&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Wang_P/0/1/0/all/0/1"&gt;Peng Wang&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;  &lt;/dl&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0606406&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0606406"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0606406"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0606406"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0606406"&gt;other&lt;/a&gt;] :&lt;/span&gt; &lt;dl&gt; &lt;dd&gt; Title: &lt;b&gt;High energy neutrino yields from astrophysical sources I: Weakly   magnetized sources&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kachelriess_M/0/1/0/all/0/1"&gt;M. Kachelriess&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Tomas_R/0/1/0/all/0/1"&gt;R. Tomas&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt; &lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-115136456790282151?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/115136456790282151/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=115136456790282151' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115136456790282151'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/115136456790282151'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/06/astro-ph0606575-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-114979259835980539</id><published>2006-06-08T11:46:00.000-07:00</published><updated>2006-06-08T11:49:58.373-07:00</updated><title type='text'></title><content type='html'>astro-ph/0606126 [abs, ps, pdf, other] :&lt;br /&gt;    Title: Search for Diffuse Astrophysical Neutrino Flux Using Ultra-High Energy Upward-Going Muons in Super-Kamiokande I&lt;br /&gt;    Authors: The Super-Kamiokande Collaboration&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-114979259835980539?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/114979259835980539/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=114979259835980539' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114979259835980539'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114979259835980539'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/06/astro-ph0606126-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-114843225559762361</id><published>2006-05-23T17:28:00.000-07:00</published><updated>2006-05-23T18:14:46.433-07:00</updated><title type='text'></title><content type='html'>astro-ph/0605327 [abs, ps, pdf, other] :&lt;br /&gt;Title: Cosmogenic Neutrinos from the propagation of Ultra High Energy Nuclei&lt;br /&gt;Authors: D. Allard, M. Ave, N. Busca, M. A. Malkan, A. V. Olinto, E. Parizot, F. W. Stecker, T. Yamamoto&lt;br /&gt;&lt;br /&gt;hep-ph/0605219 [abs, ps, pdf, other] :&lt;br /&gt;Title: Neutrino Telescopes as a Probe of Broken $\mu$-$\tau$ Symmetry&lt;br /&gt;Authors: Zhi-zhong Xing&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-114843225559762361?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/114843225559762361/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=114843225559762361' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114843225559762361'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114843225559762361'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/05/astro-ph0605327-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-114833476649965344</id><published>2006-05-22T14:47:00.000-07:00</published><updated>2006-05-22T14:52:46.510-07:00</updated><title type='text'></title><content type='html'>astro-ph/0605480 [abs, ps, pdf, other] :&lt;br /&gt;Title: Limits on the Transient Ultra-High Energy Neutrino Flux from Gamma-Ray Bursts (GRB) Derived from RICE Data&lt;br /&gt;Authors: S. Hussain, S. Razzaque, et al&lt;br /&gt;&lt;br /&gt;astro-ph/0605493 [abs, ps, pdf, other] :&lt;br /&gt;Title: A New Mechanism for Gravitational Wave Emission in Core-Collapse Supernovae&lt;br /&gt;Authors: Christian D. Ott (1), Adam Burrows (2), Luc Dessart (2), Eli Livne (3)&lt;br /&gt;&lt;br /&gt;hep-ph/0605209 [abs, ps, pdf, other] :&lt;br /&gt;Title: On the hadronic contribution to sterile neutrino production&lt;br /&gt;Authors: Takehiko Asaka, Mikko Laine, Mikhail Shaposhnikov&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-114833476649965344?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/114833476649965344/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=114833476649965344' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114833476649965344'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114833476649965344'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/05/astro-ph0605480-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-114798804899623303</id><published>2006-05-18T14:31:00.000-07:00</published><updated>2006-05-18T14:34:09.003-07:00</updated><title type='text'></title><content type='html'>&lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0605362&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0605362"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0605362"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0605362"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0605362"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Limit on the Neutrino Mass from the WMAP Three Year Data&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Fukugita_M/0/1/0/all/0/1"&gt;Masataka Fukugita&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Ichikawa_K/0/1/0/all/0/1"&gt;Kazuhide Ichikawa&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Kawasaki_M/0/1/0/all/0/1"&gt;Masahiro Kawasaki&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Lahav_O/0/1/0/all/0/1"&gt;Ofer Lahav&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;&lt;/dt&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/060&lt;/b&gt;&lt;/span&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;5424&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0605424"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0605424"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0605424"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0605424"&gt;other&lt;/a&gt;] :&lt;/span&gt; &lt;dt&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Direct X-ray Constraints on Sterile Neutrino Warm Dark Matter&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Watson_C/0/1/0/all/0/1"&gt;Casey R. Watson&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Beacom_J/0/1/0/all/0/1"&gt;John F. Beacom&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Yuksel_H/0/1/0/all/0/1"&gt;Hasan Yuksel&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Walker_T/0/1/0/all/0/1"&gt;Terry P. Walker&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;&lt;dt&gt;&lt;br /&gt;  &lt;/dt&gt;   &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;astro-ph/0605354&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0605354"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0605354"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0605354"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0605354"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;  &lt;dd&gt; Title: &lt;b&gt;Cosmological Neutrino Entanglement and Quantum Pressure&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Pfenniger_D/0/1/0/all/0/1"&gt;Daniel Pfenniger&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Observatory_V/0/1/0/all/0/1"&gt;Veruska Muccione&lt;/a&gt;&lt;/b&gt;     &lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;hep-ph/0605180&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0605180"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0605180"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0605180"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0605180"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Common Origin of Neutrino Mass, Dark Matter, and Baryogenesis&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Ma_E/0/1/0/all/0/1"&gt;Ernest Ma&lt;/a&gt; &lt;/b&gt;&lt;/dd&gt;     &lt;/dl&gt; &lt;/dd&gt;&lt;span style="font-size:+1;"&gt;&lt;b&gt;&lt;br /&gt;  &lt;/b&gt;&lt;/span&gt;&lt;/dt&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-114798804899623303?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/114798804899623303/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=114798804899623303' title='0 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114798804899623303'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114798804899623303'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/05/astro-ph0605362-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>0</thr:total></entry><entry><id>tag:blogger.com,1999:blog-28009426.post-114747024532886762</id><published>2006-05-12T14:42:00.000-07:00</published><updated>2006-05-18T14:34:38.346-07:00</updated><title type='text'></title><content type='html'>&lt;dl&gt;   &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0605281&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0605281"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0605281"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0605281"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0605281"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt; &lt;dd&gt; Title: &lt;b&gt;Supernova Neutrinos: The Accretion Disk Scenario&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+McLaughlin_G/0/1/0/all/0/1"&gt;G. C. McLaughlin&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Surman_R/0/1/0/all/0/1"&gt;R. Surman&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt;  &lt;/dl&gt;  &lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;astro-ph/0605271&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/astro-ph/0605271"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/astro-ph/0605271"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/astro-ph/0605271"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/astro-ph/0605271"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Constraints on Sterile Neutrino Dark Matter&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Abazajian_K/0/1/0/all/0/1"&gt;Kevork Abazajian&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/astro-ph/1/au:+Koushiappas_S/0/1/0/all/0/1"&gt;Savvas M. Koushiappas&lt;/a&gt;&lt;br /&gt;&lt;/b&gt;&lt;/dd&gt; &lt;/dl&gt; &lt;dl&gt; &lt;dt&gt;&lt;span style="font-size:78%;"&gt;&lt;b&gt;hep-ph/0605086&lt;/b&gt; [&lt;a href="http://xxx.lanl.gov/abs/hep-ph/0605086"&gt;abs&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/ps/hep-ph/0605086"&gt;ps&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/pdf/hep-ph/0605086"&gt;pdf&lt;/a&gt;, &lt;a href="http://xxx.lanl.gov/format/hep-ph/0605086"&gt;other&lt;/a&gt;] :&lt;/span&gt;&lt;/dt&gt;&lt;dd&gt; Title: &lt;b&gt;Probing low-x QCD with ultra-high energy cosmic neutrinos at Auger&lt;/b&gt;&lt;br /&gt;Authors: &lt;b&gt; &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Anchordoqui_L/0/1/0/all/0/1"&gt;Luis A. Anchordoqui&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Cooper_Sarkar_A/0/1/0/all/0/1"&gt;Amanda M. Cooper-Sarkar&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Hooper_D/0/1/0/all/0/1"&gt;Dan Hooper&lt;/a&gt;,  &lt;a href="http://xxx.lanl.gov/find/hep-ph/1/au:+Sarkar_S/0/1/0/all/0/1"&gt;Subir Sarkar&lt;/a&gt;&lt;/b&gt;&lt;/dd&gt; &lt;/dl&gt;&lt;div class="blogger-post-footer"&gt;&lt;img width='1' height='1' src='https://blogger.googleusercontent.com/tracker/28009426-114747024532886762?l=neutrinoastro.blogspot.com' alt='' /&gt;&lt;/div&gt;</content><link rel='replies' type='application/atom+xml' href='http://neutrinoastro.blogspot.com/feeds/114747024532886762/comments/default' title='Post Comments'/><link rel='replies' type='text/html' href='http://www.blogger.com/comment.g?blogID=28009426&amp;postID=114747024532886762' title='1 Comments'/><link rel='edit' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114747024532886762'/><link rel='self' type='application/atom+xml' href='http://www.blogger.com/feeds/28009426/posts/default/114747024532886762'/><link rel='alternate' type='text/html' href='http://neutrinoastro.blogspot.com/2006/05/astro-ph0605281-abs-ps-pdf-other-title.html' title=''/><author><name>Cecilia Lunardini</name><uri>http://www.blogger.com/profile/11591794816595828452</uri><email>noreply@blogger.com</email><gd:image rel='http://schemas.google.com/g/2005#thumbnail' width='16' height='16' src='http://img2.blogblog.com/img/b16-rounded.gif'/></author><thr:total>1</thr:total></entry></feed>
