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This article is cited in 21 scientific papers (total in 21 papers)
ASTROPHYSICS AND COSMOLOGY
Synthesis of chemical elements in dynamo active supernovae
V. N. Kondratyevab, Yu. V. Korovinac a Department of Physics, Taras Shevchenko National University of Kyiv, 03022-UA, Kyiv, Ukraine
b Bogoliubov Laboratory of Theoretical Physics, Joint Institute for Nuclear Research, Dubna, Moscow region, 141980, Russia
c Moscow Institute of Open Education, Moscow, 125167, Russia
Abstract:
The model of nuclear statistical equilibrium is employed to investigate some features of synthesis of chemical elements in the ultramagnetized astrophysical plasma plausibly arising in supernovae and near neutron stars. By example of $^{44}$Ti and $^{56}$Ni, it is demonstrated that magnetic modification of nuclear structure leads to an increase in the yield of antimagic nuclei, and production of magic nuclides varies slightly. The correspondence of the results with observations is discussed.
Received: 20.02.2015 Revised: 18.06.2015
Citation:
V. N. Kondratyev, Yu. V. Korovina, “Synthesis of chemical elements in dynamo active supernovae”, Pis'ma v Zh. Èksper. Teoret. Fiz., 102:3 (2015), 155–158; JETP Letters, 102:3 (2015), 131–134
Linking options:
https://www.mathnet.ru/eng/jetpl4692 https://www.mathnet.ru/eng/jetpl/v102/i3/p155
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Abstract page: | 159 | Full-text PDF : | 35 | References: | 42 | First page: | 7 |
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