The Stellar Black Hole ()
ABSTRACT
A black hole model is proposed in which a neutron star is surrounded by a neutral gas of electrons and positrons. The gas is in a completely degenerate quantum state and does not radiate. The pressure and density in the gas are found to be much less than those in the neutron star. The radius of the black hole is far greater than the Schwarzschild radius.
Share and Cite:
Dalton, K. (2018) The Stellar Black Hole.
Journal of High Energy Physics, Gravitation and Cosmology,
4, 651-654. doi:
10.4236/jhepgc.2018.44037.
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