CONTRIBUTION OF MEDIUM FACTORS TO ELASTIC RELIC NEUTRINO-ELECTRON SCATTERING IN CLOSE VICINITY TO MAGNETIZED ASTROPHYSICAL OBJECTS
Vali A. Huseynov1,2,3*, Rasmiyya E. Gasimova4,5, Narmin A. Zeynalova2, Narmin R. Alizade3
2024   04   en   p.39-43

ABSTRACT

The presented work is devoted to the estimation of the contribution of medium factors (chemical potential and temperature) to the elastic relic neutrino-electron scattering in close vicinity to magnetized astrophysical objects like neutron stars and white dwarfs. It is determined that the contribution of medium factors to the elastic relic neutrino-electron scattering in close vicinity to magnetized astrophysical objects depends on the ratio of the energy of the electron in the final state and the temperature of the non-degenerate final-state electron gas. It is clarified that the influence of the medium to the elastic relic neutrino-electron scattering is determined by the temperature of the non-degenerate final-state electron gas.

Keywords: relic neutrinos; magnetic field; cosmic electrons; chemical potential, Fermi-Dirac distribution
DOI:10.70784/azip.1.2024439

Received: 25.11.2024
Internet publishing: 10.12.2024

AUTHORS & AFFILIATIONS

1. Department of Engineering Physics and Electronics, Azerbaijan Technical University, 25, H. Javid Ave., Baku, AZ 1073, Azerbaijan; veli.huseynov@aztu.edu.az
2. Laboratory for Physics of Cosmic Ray Sources, Institute of Physics, 131, H. Javid Ave., Baku, AZ 1073, Azerbaijan; vgusseinov@yahoo.com
3. Department of Physics, Baku Engineering University, 120, H. Aliyev Str., Khirdalan, AZ 0101, Azerbaijan
4. Department of General Physics, Azerbaijan State Pedagogical University, 68, U. Hajibayli Str., Baku, AZ 1000, Azerbaijan
5. Department of Theoretical Astrophysics and Cosmology, Shamakhy Astrophysical Observatory, 115 H. Javid Ave., (main building of ANAS, 10th floor), Baku, AZ 1073, Azerbaijan; gasimovar@yahoo.co.uk
E-mail: * Corresponding Author gasimovar@yahoo.co.uk

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