Supermassive Black Holes

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DOI: 10.4236/jhepgc.2019.53052    532 Downloads   1,513 Views  Citations
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ABSTRACT

In the following black hole model, electrons and positrons form a neutral gas which is confined by gravitation. The smaller masses are supported against gravity by electron degeneracy pressure. Larger masses are supported by ideal gas and radiation pressure. In each case, the gas is a polytrope which satisfies the Lane-Emden equation. Solutions are found that yield the physical properties of black holes, for the range 1000 to 100 billion solar masses.

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Dalton, K. (2019) Supermassive Black Holes. Journal of High Energy Physics, Gravitation and Cosmology, 5, 984-988. doi: 10.4236/jhepgc.2019.53052.

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