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Nucleosynthesis in Non-Spherical Supernova Explosion and Observations

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Supernovae

Abstract

During the last two decades many investigators had taken attempts to construct Supernova models, that will be able to describe observed physical pattern of this phenomena. Most of them considered models of collapsing iron core of massive star, that were supposed to be a mechanism for Type II Supernova (see HILLEBRANDT [11 and references there). But despite the fact that some of them were very sophisticated one (includes rotation, relativity effects, neutrino transport and some other physical processes), models of this class have failed to explain some aspects of Type II Supernova and Type I Supernova. That was the reason why thermonuclear model of Supernova explosion was suggested by FOWLER and HOYLE [2], ARNETT [3] and others for Type I Supernova.

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© 1991 Springer-Verlag New York, Inc.

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Chechetkin, V.M., Denissov, A.A., Popov, Y.P. (1991). Nucleosynthesis in Non-Spherical Supernova Explosion and Observations. In: Woosley, S.E. (eds) Supernovae. Santa Cruz Summer Workshops in Astronomy and Astrophysics. Springer, New York, NY. https://doi.org/10.1007/978-1-4612-2988-9_55

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  • DOI: https://doi.org/10.1007/978-1-4612-2988-9_55

  • Publisher Name: Springer, New York, NY

  • Print ISBN: 978-1-4612-7748-4

  • Online ISBN: 978-1-4612-2988-9

  • eBook Packages: Springer Book Archive

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