02930nam 2200625Ia 450 991078392350332120230617010302.01-281-90581-X9786611905811981-270-344-6(CKB)1000000000334298(EBL)296196(OCoLC)476064092(SSID)ssj0000215232(PQKBManifestationID)11204395(PQKBTitleCode)TC0000215232(PQKBWorkID)10184824(PQKB)11120814(MiAaPQ)EBC296196(WSP)00001598 (Au-PeEL)EBL296196(CaPaEBR)ebr10174116(CaONFJC)MIL190581(EXLCZ)99100000000033429820060228d2005 uy 0engur|n|---|||||txtccrOpen issues in core collapse supernova theory[electronic resource] /editors, Anthony Mezzacappa, George M. FullerHackensack, N.J. World Scientificc20051 online resource (475 p.)Proceedings from the Institute for Nuclear Theory ;v. 14"National Institute for Nuclear Theory, University of Washington, Seattle, 22-24 June 2004."981-256-314-8 Includes bibliographical references.PREFACE; 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 CurvesEfforts 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 turbulProceedings from the Institute for Nuclear Theory ;v. 14.SupernovaeMathematical modelsCongressesCataclysmic variable starsSupernovaeMathematical modelsCataclysmic variable stars.523.8/4465Mezzacappa Anthony1501768Fuller George Michael1501769Institute for Nuclear Theory (U.S.)MiAaPQMiAaPQMiAaPQBOOK9910783923503321Open issues in core collapse supernova theory3729067UNINA