Why and How Do Black Holes Radiate? ()
Abstract
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.
Share and Cite:
Raitio, R. (2015) Why and How Do Black Holes Radiate?.
Open Access Library Journal,
2, 1-4. doi:
10.4236/oalib.1102254.
Conflicts of Interest
The authors declare no conflicts of interest.
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