Open Issues in Core Collapse Supernova Theory

Anthony Mezzacappa

ISBN 10: 9812563148 / ISBN 13: 9789812563149

Published by World Scientific Publishing Company Dez 2005, 2005

About this Item

Neuware - 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 turbulent stellar core fluid flow, its magnetic fields, the neutrinos produced in and emanating from the proto-neutron star, the stellar core rotation, and the strong gravitational fields have yet to be performed. Only subsets of these fundamental ingredients have been included in the models thus far, often with approximation. The purpose of this volume is to identify the outstanding issues that remain.

Seller Inventory # 9789812563149

Bibliographic Details

• Title: Open Issues in Core Collapse Supernova Theory
• Publisher: World Scientific Publishing Company Dez 2005
• Publication Date: 2005
• Language: English
• ISBN 10: 9812563148
• ISBN 13: 9789812563149
• Binding: Buch
• Condition: Neu
• Dimensions: 228W x 157H x 31D millimeters 228 millimeters width by 157 millimeters height by 31 millimeters depth
• Weight: 780 grams

About this title

Synopsis

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 turbulent stellar core fluid flow, its magnetic fields, the neutrinos produced in and emanating from the proto-neutron star, the stellar core rotation, and the strong gravitational fields have yet to be performed. Only subsets of these fundamental ingredients have been included in the models thus far, often with approximation.The purpose of this volume is to identify the outstanding issues that remain in order to come to a complete understanding of these important astrophysical events. As the book focuses on open issues rather than the current state of the art in the field -- although the latter will certainly be discussed -- it will remain relevant for some time.