Quantized black holes, their spectrum and radiation

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Quantized black holes, their spectrum and radiation. / Khriplovich, I. B.

In: Physics of Atomic Nuclei, Vol. 71, No. 4, 01.04.2008, p. 671-680.

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Author

Khriplovich, I. B. / Quantized black holes, their spectrum and radiation. In: Physics of Atomic Nuclei. 2008 ; Vol. 71, No. 4. pp. 671-680.

BibTeX

@article{fb3752413a074a6bb814b7b283cd0cf9,

title = "Quantized black holes, their spectrum and radiation",

abstract = "Under quite natural general assumptions, the following results are obtained. The maximum entropy of a quantized surface is demonstrated to be proportional to the surface area in the classical limit. The general structure of the horizon spectrum is found. In the special case of loop quantum gravity, the value of the Barbero-Immirzi parameter is found. The discrete spectrum of thermal radiation of a black hole fits the Wien profile. The natural widths of the lines are much smaller than the distances between them. The total intensity of the thermal radiation is estimated. If the density of quantized primordial black holes is close to the present upper limit on the dark-matter density in our Solar system, the sensitivity of modern detectors is close to that necessary for detecting this radiation.",

author = "Khriplovich, {I. B.}",

year = "2008",

month = apr,

day = "1",

doi = "10.1134/S1063778808040078",

language = "English",

volume = "71",

pages = "671--680",

journal = "Physics of Atomic Nuclei",

issn = "1063-7788",

publisher = "МАИК {"}Наука/Интерпериодика{"}",

number = "4",

}

RIS

TY - JOUR

T1 - Quantized black holes, their spectrum and radiation

AU - Khriplovich, I. B.

PY - 2008/4/1

Y1 - 2008/4/1

N2 - Under quite natural general assumptions, the following results are obtained. The maximum entropy of a quantized surface is demonstrated to be proportional to the surface area in the classical limit. The general structure of the horizon spectrum is found. In the special case of loop quantum gravity, the value of the Barbero-Immirzi parameter is found. The discrete spectrum of thermal radiation of a black hole fits the Wien profile. The natural widths of the lines are much smaller than the distances between them. The total intensity of the thermal radiation is estimated. If the density of quantized primordial black holes is close to the present upper limit on the dark-matter density in our Solar system, the sensitivity of modern detectors is close to that necessary for detecting this radiation.

AB - Under quite natural general assumptions, the following results are obtained. The maximum entropy of a quantized surface is demonstrated to be proportional to the surface area in the classical limit. The general structure of the horizon spectrum is found. In the special case of loop quantum gravity, the value of the Barbero-Immirzi parameter is found. The discrete spectrum of thermal radiation of a black hole fits the Wien profile. The natural widths of the lines are much smaller than the distances between them. The total intensity of the thermal radiation is estimated. If the density of quantized primordial black holes is close to the present upper limit on the dark-matter density in our Solar system, the sensitivity of modern detectors is close to that necessary for detecting this radiation.

UR - http://www.scopus.com/inward/record.url?scp=43049141495&partnerID=8YFLogxK

U2 - 10.1134/S1063778808040078

DO - 10.1134/S1063778808040078

M3 - Article

AN - SCOPUS:43049141495

VL - 71

SP - 671

EP - 680

JO - Physics of Atomic Nuclei

JF - Physics of Atomic Nuclei

SN - 1063-7788

IS - 4

ER -

ID: 36641914