Preprint Article Version 1 This version is not peer-reviewed

From Black Holes to Neutrino Stars

Version 1 : Received: 21 September 2018 / Approved: 21 September 2018 / Online: 21 September 2018 (16:41:04 UTC)

How to cite: Tsekov, R. From Black Holes to Neutrino Stars. Preprints 2018, 2018090441 (doi: 10.20944/preprints201809.0441.v1). Tsekov, R. From Black Holes to Neutrino Stars. Preprints 2018, 2018090441 (doi: 10.20944/preprints201809.0441.v1).

Abstract

Due to limitation of the binding energy of a self-gravitating matter, the radius of a body is at least twice larger than the Schwarzschild radius. The total energy is adsorbed at the body surface, giving rise of a size-dependent surface tension. Since the Hawking temperature appears to be the critical one, the black holes possess zero surface tension. Microscopic neutrino stars are also introduced.

Subject Areas

self-gravitation, black holes, neutrino stars

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