LEADER 02962nam 2200637Ia 450 001 9910450680103321 005 20200520144314.0 010 $a1-281-90581-X 010 $a9786611905811 010 $a981-270-344-6 035 $a(CKB)1000000000334298 035 $a(EBL)296196 035 $a(OCoLC)476064092 035 $a(SSID)ssj0000215232 035 $a(PQKBManifestationID)11204395 035 $a(PQKBTitleCode)TC0000215232 035 $a(PQKBWorkID)10184824 035 $a(PQKB)11120814 035 $a(MiAaPQ)EBC296196 035 $a(WSP)00001598 035 $a(Au-PeEL)EBL296196 035 $a(CaPaEBR)ebr10174116 035 $a(CaONFJC)MIL190581 035 $a(EXLCZ)991000000000334298 100 $a20060228d2005 uy 0 101 0 $aeng 135 $aur|n|---||||| 181 $ctxt 182 $cc 183 $acr 200 00$aOpen issues in core collapse supernova theory$b[electronic resource] /$feditors, Anthony Mezzacappa, George M. Fuller 210 $aHackensack, N.J. $cWorld Scientific$dc2005 215 $a1 online resource (475 p.) 225 1 $aProceedings from the Institute for Nuclear Theory ;$vv. 14 300 $a"National Institute for Nuclear Theory, University of Washington, Seattle, 22-24 June 2004." 311 $a981-256-314-8 320 $aIncludes bibliographical references. 327 $aPREFACE; CONTENTS; Section 1 Overview; Section 2 Fundamental Issues in Radiation Magnet ohydrodynamics; Section 3 The Core Collapse Supernova Mechanism; Section 4 Neutrino Mixing; Section 5 Neutrino Interactions; Section 6 The Equation of State; Section 7 Nucleosynthesis and Light Curves 330 $aEfforts to uncover the explosion mechanism of core collapse supernovae and to understand all of their associated phenomena have been ongoing for nearly four decades. Despite this, our theoretical understanding of these cosmic events remains limited; two- and three-dimensional modeling of these events is in its infancy. Most of the modeling efforts over the past four decades have, by necessity, been constrained to spherical symmetry, with the first two-dimensional, albeit simplified, models appearing only during the last decade. Simulations to understand the complex interplay between the turbul 410 0$aProceedings from the Institute for Nuclear Theory ;$vv. 14. 606 $aSupernovae$xMathematical models$vCongresses 606 $aCataclysmic variable stars 608 $aElectronic books. 615 0$aSupernovae$xMathematical models 615 0$aCataclysmic variable stars. 676 $a523.8/4465 701 $aMezzacappa$b Anthony$0949889 701 $aFuller$b George Michael$0949890 712 02$aInstitute for Nuclear Theory (U.S.) 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910450680103321 996 $aOpen issues in core collapse supernova theory$92147190 997 $aUNINA