Article
Version 1
Preserved in Portico This version is not peer-reviewed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 CEST)
A peer-reviewed article of this Preprint also exists.
Tsekov, R. From Black Holes to Neutrino Stars. Preprints 2018, 2018090441. https://doi.org/10.20944/preprints201809.0441.v1. Tsekov, R. From Black Holes to Neutrino Stars. Preprints 2018, 2018090441. https://doi.org/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.
Keywords
self-gravitation, black holes, neutrino stars
Subject
Physical Sciences, Atomic and Molecular Physics
Copyright: This is an open access article distributed under the Creative Commons Attribution License which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
Comments (0)
We encourage comments and feedback from a broad range of readers. See criteria for comments and our Diversity statement.
Leave a public commentSend a private comment to the author(s)
* All users must log in before leaving a comment