Forced reverse reactions in neutron star matter

Authors

  • N. Zh. Takibayev Department of Physics and Technology, al-Faraby KazNU, Almaty, Institute of Experimental and Theoretical Physics, Almaty

DOI:

https://doi.org/10.26577/phst-2016-1-92

Keywords:

Neutron star, nonlinear interactions, neutron resonances with few-nuclei, electron capture reactions

Abstract

Nuclear reactions in neutron star envelopes are considered in the frame of complex interactions stimulated by huge pressures in the overdense crystalline structures in the envelopes. It leads to the inclusion of forced reverse reactions that transform the nuclei to neutron-rich states and the appearance of free neutrons. The free neutrons in the structures cause resonance interactions with nuclei that fixed in nodes of crystal. The neutron re-scattering on subsystem of few nucleus at the energy near the energy of resonance level of the nucleus creates the few-body resonances, which depend on the distances between the nuclei. 

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Published

2017-03-06

Issue

Section

Nuclear Physics and Related Techology

How to Cite

Forced reverse reactions in neutron star matter. (2017). Physical Sciences and Technology, 3(1), 36-41. https://doi.org/10.26577/phst-2016-1-92