Why and How Do Black Holes Radiate? - Open Access Library Journal

OALibJ > Vol.2 No.12, December 2015

Open Access Library Journal

Volume 2, Issue 12 (December 2015)

ISSN Print: 2333-9705 ISSN Online: 2333-9721

Google-based Impact Factor: 0.73 Citations

Why and How Do Black Holes Radiate? ()

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DOI: 10.4236/oalib.1102254 797 Downloads 1,799 Views Citations

Author(s)

Risto Raitio

Affiliation(s)

02230Espoo, Finland.

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.

KEYWORDS

Quantum Black Hole, Hawking Radiation, Standard Model, Grand Unified Theory

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.

Cited by

[1]	A Statistical Model of Spacetime, Black Holes and Matter
	Open Access Library Journal, 2016

[2]	Thermodynamics of Gravity and a Statistical Model of Black Holes
	2016

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