Forced reverse reactions in neutron star matter

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

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
How to Cite
TAKIBAYEV, N. Zh.. Forced reverse reactions in neutron star matter. Physical Sciences and Technology, [S.l.], v. 3, n. 1, mar. 2017. ISSN 2409-6121. Available at: <http://phst.kaznu.kz/index.php/journal/article/view/92>. Date accessed: 18 oct. 2017.
Section
Nuclear Physics and Related Techology

Keywords

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