English

Analytic solution for kinetic equilibrium of beta-processes in nucleonic plasma with relativistic pairs

High Energy Astrophysical Phenomena 2015-06-04 v3

Abstract

The analytic solution is obtained describing kinetic equilibrium of the β\beta-processes in the nucleonic plasma with relativistic pairs. The nucleons (n,p)(n,p) are supposed to be non-relativistic and non-degenerate, while the electrons and positrons are ultra-relativistic due to high temperature (T>6109(T>6\cdot 10^9K), or high density (ρ>μ106(\rho>\mu 10^6g/cm3^3), or both, where μ\mu is a number of nucleons per one electron. The consideration is simplified because of the analytic connection of the density with the electron chemical potential in the ultra-relativistic plasma, and Gauss representation of Fermi functions. Electron chemical potential and number of nucleons per one initial electron are calculated as functions of ρ\rho and TT.

Keywords

Cite

@article{arxiv.1203.0997,
  title  = {Analytic solution for kinetic equilibrium of beta-processes in nucleonic plasma with relativistic pairs},
  author = {G. S. Bisnovatyi-Kogan},
  journal= {arXiv preprint arXiv:1203.0997},
  year   = {2015}
}

Comments

16 pages, 6 figures