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Nucleosynthesis in Neutron Stars Crust

Journal: Journal of Nuclear Physics, Material Sciences, Radiation and Applications (Vol.3, No. 1)

Publication Date:

Authors : ; ; ;

Page : 103-109

Keywords : Neutron stars; r-process; NS e; Nucleosynthesis; Nuclear Statistical equilibrium;

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We address the problem of the origin of heavier and super heavy elements in nature. Believing rapid neutron capture process (r-process) is responsible for synthesis of heavy and super heavy elements in the remnants of supernovae explosions and neutron star crusts under extreme conditions, we developed a computer code in order to understand the formation of elements in extreme astrophysical systems. We carried out Nuclear Statistical e quilibrium (NS e ) as well as static r-process calculations for a wide range of input parameters.

Last modified: 2019-12-03 19:04:31