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Open Issues In Core Collapse Supernova Theory.
Efforts 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 event...
| Clasificación: | Libro Electrónico |
|---|---|
| Autor principal: | |
| Otros Autores: | |
| Formato: | Electrónico eBook |
| Idioma: | Inglés |
| Publicado: |
Singapore :
World Scientific,
2005.
|
| Colección: | Proceedings from the Institute for Nuclear Theory ;
v. 14. |
| Temas: | |
| Acceso en línea: | Texto completo |
MARC
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| 100 | 1 | |a Mezzacappa, Anthony. | |
| 245 | 1 | 0 | |a Open Issues In Core Collapse Supernova Theory. |
| 260 | |a Singapore : |b World Scientific, |c 2005. | ||
| 300 | |a 1 online resource (475 pages) | ||
| 336 | |a text |b txt |2 rdacontent | ||
| 337 | |a computer |b c |2 rdamedia | ||
| 338 | |a online resource |b cr |2 rdacarrier | ||
| 490 | 1 | |a Proceedings from the Institute for Nuclear Theory ; |v v. 14 | |
| 520 | |a Efforts 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. | ||
| 588 | 0 | |a Print version record. | |
| 505 | 0 | |a 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 Curves. | |
| 504 | |a Includes bibliographical references. | ||
| 590 | |a ProQuest Ebook Central |b Ebook Central Academic Complete | ||
| 650 | 0 | |a Cataclysmic variable stars. | |
| 650 | 0 | |a Supernovae |x Mathematical models |v Congresses. | |
| 650 | 6 | |a Étoiles variables cataclysmiques. | |
| 650 | 6 | |a Supernovae |x Modèles mathématiques |v Congrès. | |
| 650 | 7 | |a Cataclysmic variable stars |2 fast | |
| 650 | 7 | |a Supernovae |x Mathematical models |2 fast | |
| 655 | 7 | |a Conference papers and proceedings |2 fast | |
| 700 | 1 | |a Fuller, George M. | |
| 758 | |i has work: |a Open issues in core collapse supernova theory (Text) |1 https://id.oclc.org/worldcat/entity/E39PCFydmvGmXHMVcTHkQxRjhb |4 https://id.oclc.org/worldcat/ontology/hasWork | ||
| 776 | 1 | |z 9789812563149 | |
| 830 | 0 | |a Proceedings from the Institute for Nuclear Theory ; |v v. 14. | |
| 856 | 4 | 0 | |u https://ebookcentral.uam.elogim.com/lib/uam-ebooks/detail.action?docID=296196 |z Texto completo |
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