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 44Ti and 56Ni, 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.
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Original Russian Text © V.N. Kondratyev, Yu.V. Korovina, 2015, published in Pis’ma v Zhurnal Eksperimental’noi i Teoreticheckoi Fiziki, 2015, Vol. 102, No. 3, pp. 155–158.
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Kondratyev, V.N., Korovina, Y.V. Synthesis of chemical elements in dynamo active supernovae. Jetp Lett. 102, 131–134 (2015). https://doi.org/10.1134/S0021364015150047
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DOI: https://doi.org/10.1134/S0021364015150047