Equilibrium configurations of degenerate superstars in the quantum limit of the frozen-in magnetic field

Details Equilibrium configurations of degenerate superstars in the quantum limit of the frozen-in magnetic field Equilibrium configurations of degenerate superstars in the quantum limit of the frozen-in magnetic field

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..759s&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, July-Aug. 1989, p. 759-766. In Russian.

Statistics

6

Degenerate Matter, Quantum Statistics, Stellar Magnetic Fields, Supermassive Stars, Cosmic Gases, Density (Mass/Volume), Equilibrium Equations, Fermi-Dirac Statistics, Stellar Cores, Stellar Mass

Scientific paper

In the framework of the appproximate energy method, the magnetic field strength in the center of a degenerate superstar and averaged over the whole star is estimated for a given mass of the equilibrium star and a number of given values of the mass density in the center of the degenerate configuration. It is found that the mass of the star in the quantum limit of the frozen-in magnetic field, which is necessary for equilibrium of the configuration, must attain values equal to or greater than 800 solar masses.

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