3D Core-Collapse Supernova Calculations

  • Tobias Bollenbach
  • Terrance Strother
  • Wolfgang Bauer
Conference paper

DOI: 10.1007/978-1-4020-2705-5_21

Part of the NATO Science Series book series (NAII, volume 166)
Cite this paper as:
Bollenbach T., Strother T., Bauer W. (2004) 3D Core-Collapse Supernova Calculations. In: Greiner W., Itkis M.G., Reinhardt J., Güçlü M.C. (eds) Structure and Dynamics of Elementary Matter. NATO Science Series (Series II: Mathematics, Physics and Chemistry), vol 166. Springer, Dordrecht

Abstract

Recent observations of the polarization of the light emitted by supernova explo-sions indicate that there are large deviations from spherical symmetry in the very heart of these explosions. Asymmetries may well play a key role in the explosion mechanism. So far there is no convincing theoretical explanation for these observations. In this work the impact of angular momentum on the core collapse which is possibly the origin of large asymmetries is studied. We introduce a new approach to the supernova problem: a three dimensional test particle based simulation. The infall phase of the collapse of a typical iron core is investigated using numerical calculations. Our main focus is the impact of angular momentum. Significant deviations from spherical symmetry are found for rapidly rotating supernova cores.

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Copyright information

© Springer Science+Business Media Dordrecht 2004

Authors and Affiliations

  • Tobias Bollenbach
    • 1
  • Terrance Strother
    • 2
  • Wolfgang Bauer
    • 2
  1. 1.Max-Planck-Institut für Physik komplexer SystemeDresdenGermany
  2. 2.National Superconducting Cyclotron Laboratory and Department of Physics and AstronomyMichigan State UniversityEast LansingUSA

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