On the Formation of a Nonequilibrium Chemical Composition in the Shells of Neutron Stars
Astrophysics, ISSN: 1573-8191, Vol: 64, Issue: 2, Page: 228-243
2021
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Article Description
The chemical composition of the shell of a neutron star (SNS) at high temperatures and densities is discussed in this paper. A model for nucleosynthesis is proposed based on the approximation of nuclear statistical equilibrium (NSE). The dependence of the results of the nucleosynthesis on the parameters of the medium in a static approximation is studied. The results of this paper are qualitatively similar to earlier work by other authors. It is shown that the proposed model provides a fair description of the abundance of nuclei even in the static approximation.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85108108388&origin=inward; http://dx.doi.org/10.1007/s10511-021-09684-1; https://link.springer.com/10.1007/s10511-021-09684-1; https://link.springer.com/content/pdf/10.1007/s10511-021-09684-1.pdf; https://link.springer.com/article/10.1007/s10511-021-09684-1/fulltext.html; https://dx.doi.org/10.1007/s10511-021-09684-1; https://link.springer.com/article/10.1007/s10511-021-09684-1
Springer Science and Business Media LLC
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