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Magnetorotational supernovae with different equations of state

Published online by Cambridge University Press:  05 September 2012

Sergey G. Moiseenko  and
Gennady S. Bisnovatyi-Kogan
Sergey G. Moiseenko
Affiliation:
Space Research Institute, Profsouznaya str. 84/32 117997 Moscow, Russia email: [email protected]
Gennady S. Bisnovatyi-Kogan
Affiliation:
Space Research Institute, Profsouznaya str. 84/32 117997 Moscow, Russia email: [email protected]
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Abstract

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We present results of the simulation of a magneto-rotational supernova explosion. We show that, due to the differential rotation of the collapsing iron core, the magnetic field increases with time. The magnetic field transfers angular momentum and a MHD shock wave forms. This shock wave produces the supernova explosion. The explosion energy computed in our simulations is 0.5-2.5 ċ 1051erg. We used two different equations of state for the simulations. The results are rather similar.

Keywords

supernovae: generalmethods: numerical
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 7 , Symposium S279: Death of Massive Stars: Supernovae and Gamma-Ray Bursts , April 2011 , pp. 357 - 358
Copyright
Copyright © International Astronomical Union 2012

References

Ardeljan, N. V., Bisnovatyi-Kogan, G. S., Kosmachevskii, K. V., & Moiseenko, S. G., 1996, A&AS, 115, 573Google Scholar
Ardelyan, N. V., Bisnovatyi-Kogan, G. S., Popov, Yu. P., & Chernigovsky, S. V., 1987, Astron. Zh. 64, 761 (Soviet Astronomy, 1987, 31, 398)Google Scholar
Ardeljan, N. V., Bisnovatyi-Kogan, G. S., & Moiseenko, S. G., Monthly Not. Roy. Astron. Soc. 359 333 (2005).CrossRefGoogle Scholar
Bisnovatyi-Kogan, G. S., 1970, Astron. Zh. 47, 813 (Soviet Astronomy 1971 14, 652)Google Scholar
Bisnovatyi-Kogan, G. S., Moiseenko, S. G., & Ardelyan, N. V., 2008, Astronomy Reports, 52, 997CrossRefGoogle Scholar
Ivanova, L. N., Imschennik, V. S., & Nadyozhin, D. K., 1969 Nauch. inf. Astron. Soveta, 13, 3Google Scholar
Kotake, K., Yamada, S., & Sato, K. 2003, ApJ, 595, 304CrossRefGoogle Scholar
Moiseenko, S. G., Bisnovatyi-Kogan, G. S., & Ardeljan, N. V., 2006, Monthly Not. Roy. Astron. Soc., 370, 501CrossRefGoogle Scholar
Shen, H., Toki, H., Oyamatsu, K., & Sumiyoshi, K. 1998, Nucl. Phys. A, 637, 435CrossRefGoogle Scholar