Equilibrium state of a degenerate magnetized electron-nuclear plasma

Details Equilibrium state of a degenerate magnetized electron-nuclear plasma Equilibrium state of a degenerate magnetized electron-nuclear plasma

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984afz....20..315l&link_type=abstract

(Astrofizika, vol. 20, Mar.-Apr. 1984, p. 315-320) Astrophysics (ISSN 0571-7132), vol. 20, no. 2, Sept. 1984, p. 169-172. Transl

Astronomy and Astrophysics

Astrophysics

1

Electron Plasma, Nuclear Reactions, Plasma Equilibrium, Pulsars, Thermodynamic Equilibrium, Cold Plasmas, Plasma Interactions

Scientific paper

The degenerate state of cold matter (at density 10 Mg - 10 Tg/cu cm and magnetic fields 2-50 TG) which is stable with regard to beta(-) processes and pycnonuclear reactions is characterized theoretically using a noninteracting-particle model. The thermodynamic and nuclear parameters for relatively and absolutely stable thermodynamic-equilibrium states are given in tables and graphs, and the applicability of the model is demonstrated. These electron-nuclear and electron-neutron-nuclear phases are qualitatively similar to those found in the exteriors of pulsars.

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