Bohr-like black holes

Journal Article · Tue Mar 10 00:00:00 EDT 2015 · AIP Conference Proceedings

DOI:https://doi.org/10.1063/1.4912308· OSTI ID:22391035

Corda, Christian ^[1]

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1. Dipartimento di Fisica e Chimica, Istituto Universitario di Ricerca Scientifica 'Santa Rita', Centro di Scienze Naturali, Via di Galceti, 74, 59100 Prato (Italy)

The idea that black holes (BHs) result in highly excited states representing both the “hydrogen atom” and the “quasi-thermal emission” in quantum gravity is today an intuitive but general conviction. In this paper it will be shown that such an intuitive picture is more than a picture. In fact, we will discuss a model of quantum BH somewhat similar to the historical semi-classical model of the structure of a hydrogen atom introduced by Bohr in 1913. The model is completely consistent with existing results in the literature, starting from the celebrated result of Bekenstein on the area quantization.

• OSTI ID: 22391035
• Journal Information: AIP Conference Proceedings, Vol. 1648, Issue 1; Conference: ICNAAM-2014: International Conference on Numerical Analysis and Applied Mathematics 2014, Rhodes (Greece), 22-28 Sep 2014; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ATOMIC MODELS
ATOMS
BLACK HOLES
BOHR THEORY
EMISSION
EXCITED STATES
HYDROGEN
QUANTIZATION
QUANTUM GRAVITY
SEMICLASSICAL APPROXIMATION