Quantum Gravity and String Theory

    

Why and How do Black Holes Radiate?

Authors: Risto Raitio

The phenomenological model proposed in this note indicates that the black hole radiation consists of two components: the standard thermal Hawking radiation and an additional non-thermal baryonic/leptonic component due to quantum number neutralization by the no-hair theorem. The particle radiation grows relatively stronger than the Hawking radiation with increasing black hole mass, and it can be tested in principle.

Comments: 6 Pages. Published version, Open Access Library Journal, 2: e2254. http://dx.doi.org/10.4236/oalib.1102254

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Submission history

[v1] 2015-11-17 08:11:23
[v2] 2015-12-21 09:59:47

Unique-IP document downloads: 352 times

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