Relativistic magnetic partially degenerate isothermal gas spheres

Details Relativistic magnetic partially degenerate isothermal gas spheres Relativistic magnetic partially degenerate isothermal gas spheres

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ap%26ss.184..143s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 184, no. 1, Oct. 1991, p. 143-146.

Statistics

Fermi-Dirac Statistics, Gas Flow, Hydrostatics, Magnetic Field Configurations, Poloidal Flux, Relativistic Plasmas, Boundary Conditions, Differential Equations, Radiation Pressure

Scientific paper

The effect of a poloidal magnetic field on the structure of isothermal gas spheres in hydrostatic equilibrium under the pressure of partially degenerate relativistic electrons and radiation has been considered. An equation of state involving Fermi-Dirac functions F2 (psi) and F3 (psi) has been used. Modifications to the values of various structural parameters have been tabulated for the cases psi(c) = 0, 2, 3, 5, and 10, psi(c) being the central degeneracy parameter.

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