The influence of a net charge on the critical mass of a neutron star

Details The influence of a net charge on the critical mass of a neutron star The influence of a net charge on the critical mass of a neutron star

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ap%26ss..88...81z&link_type=abstract

Astrophysics and Space Science, vol. 88, no. 1, Nov. 1982, p. 81-88.

Astronomy and Astrophysics

Astrophysics

10

Critical Mass, Electric Charge, Neutron Stars, Relativity, Stellar Mass, Charge Distribution, Stellar Gravitation, Stellar Models

Scientific paper

The set of equations determining the structure of a spherically symmetric charged star are derived within the framework of general relativity (modified Oppenheimer-Volkoff equations). The equations have been solved for a completely degenerate Fermi gas with a charge density assumed to be proportional to the matter density. It is shown that the presence of a net charge does not affect the existence of a critical mass. The value, however, could be substantially altered, in some cases doubled.

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