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  • © 2004

Stellar Collapse

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Part of the book series: Astrophysics and Space Science Library (ASSL, volume 302)

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Table of contents (13 chapters)

  1. Front Matter

    Pages i-xxxi
  2. Core-Collapse Supernovae

    1. Front Matter

      Pages 1-4
    2. Massive Star Evolution

      • Patrick A. Young, David Arnett
      Pages 5-38
    3. Explosion Mechanisms of Massive Stars

      • H.-Thomas Janka, Robert Buras, Konstantinos Kifonidis, Markus Rampp, Tomek Plewa
      Pages 65-97
    4. Neutrino Transport in Core Collapse Supernovae

      • Anthony Mezzacappa, Matthias Liebendörfer, Christian Y. Cardall, O. E. Bronson Messer, Stephen W. Bruenn
      Pages 99-131
    5. Neutrino-Matter Interaction Rates in Supernovae

      • Adam Burrows, Todd A. Thompson
      Pages 133-174
    6. Protoneutron Star Winds

      • Todd A. Thompson
      Pages 175-202
  3. Asymmetries in Collapse, Beyond the Basic Supernova Mechanism

    1. Front Matter

      Pages 203-205
    2. Radioactive Decay in Core-Collapse Supernovae

      • Aimee L. Hungerford
      Pages 207-236
    3. Asymmetric Supernova Explosions

      • P. Höflich, L. Wang, A. Khokhlov
      Pages 237-258
    4. Magnetic Fields in Supernovae

      • Shizuka Akiyama, J. Craig Wheeler
      Pages 259-275
    5. Hypernovae and Other Black-Hole-Forming Supernovae

      • Ken’ichi Nomoto, Keiichi Maeda, Paolo A. Mazzali, Hideyuki Umeda, Jinsong Deng, Koichi Iwamoto
      Pages 277-325
    6. The Collapsar Engine for GRBS and Hypernovae

      • Weiqun Zhang, Chris L. Fryer
      Pages 327-355
    7. Gamma-Ray Bursts from Supernovae

      • Christopher D. Matzner
      Pages 357-372
    8. Stellar Collapse and Gravitational Waves

      • Chris L. Fryer, Daniel E. Holz, Scott A. Hughes, Michael S. Warren
      Pages 373-402
  4. Back Matter

    Pages 403-411

About this book

Supernovae, hypernovae and gamma-ray bursts are among the most energetic explosions in the universe. The light from these outbursts is, for a brief time, comparable to billions of stars and can outshine the host galaxy within which the explosions reside. Most of the heavy elements in the universe are formed within these energetic explosions. Surprisingly enough, the collapse of massive stars is the primary source of not just one, but all three of these explosions.
As all of these explosions arise from stellar collapse, to understand one requires an understanding of the others. Stellar Collapse marks the first book to combine discussions of all three phenomena, focusing on the similarities and differences between them. Designed for graduate students and scientists newly entering this field, this book provides a review not only of these explosions, but the detailed physical models used to explain them from the numerical techniques used to model neutrino transport and gamma-ray transport to the detailed nuclear physics behind the evolution of the collapse to the observations that have led to these three classes of explosions.

Editors and Affiliations

  • Los Alamos National Laboratory, Los Alamos, USA

    Chris L. Fryer

  • University of Arizona, Tucson, USA

    Chris L. Fryer

Bibliographic Information

Buy it now

Buying options

eBook USD 129.00
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 169.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info
Hardcover Book USD 169.99
Price excludes VAT (USA)
  • Durable hardcover edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access