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

Gribov Memorial Volume: Quarks, Hadrons, and Strong Interactions - Proceedings of the Memorial Workshop Devoted to the 75th Birthday of V N Gribov. 2006. стр. 474-489.

Результаты исследований: Публикации в книгах, отчётах, сборниках, трудах конференций › статья в сборнике материалов конференции › научная › Рецензирование

Harvard

Khriplovich, IB 2006, Quantized black holes, their spectrum and radiation. в Gribov Memorial Volume: Quarks, Hadrons, and Strong Interactions - Proceedings of the Memorial Workshop Devoted to the 75th Birthday of V N Gribov. стр. 474-489, Gribov Memorial Workshop Devoted to the 75th Birthday of V N Gribov: Quarks, Hadrons, and Strong Interactions, Budapest, Венгрия, 22/05/05.

APA

Khriplovich, I. B. (2006). Quantized black holes, their spectrum and radiation. в Gribov Memorial Volume: Quarks, Hadrons, and Strong Interactions - Proceedings of the Memorial Workshop Devoted to the 75th Birthday of V N Gribov (стр. 474-489)

Vancouver

Khriplovich IB. Quantized black holes, their spectrum and radiation. в Gribov Memorial Volume: Quarks, Hadrons, and Strong Interactions - Proceedings of the Memorial Workshop Devoted to the 75th Birthday of V N Gribov. 2006. стр. 474-489

Author

Khriplovich, I. B. / Quantized black holes, their spectrum and radiation. Gribov Memorial Volume: Quarks, Hadrons, and Strong Interactions - Proceedings of the Memorial Workshop Devoted to the 75th Birthday of V N Gribov. 2006. стр. 474-489

BibTeX

@inproceedings{4d5b2731b0464e3888363906c4ed9e72,
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. 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. In the special case of loop quantum gravity, the value of the Barbero - Immirzi parameter is found. Other values for this parameter, obtained under an additional assumption that the horizon is described by a U(1) Chern - Simons theory, are demonstrated to be in conflict with the firmly established holographic bound.",
author = "Khriplovich, {I. B.}",
year = "2006",
month = dec,
day = "1",
language = "English",
isbn = "9812567569",
pages = "474--489",
booktitle = "Gribov Memorial Volume",
note = "Gribov Memorial Workshop Devoted to the 75th Birthday of V N Gribov: Quarks, Hadrons, and Strong Interactions ; Conference date: 22-05-2005 Through 24-05-2005",

}

RIS

TY - GEN

T1 - Quantized black holes, their spectrum and radiation

AU - Khriplovich, I. B.

PY - 2006/12/1

Y1 - 2006/12/1

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. 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. In the special case of loop quantum gravity, the value of the Barbero - Immirzi parameter is found. Other values for this parameter, obtained under an additional assumption that the horizon is described by a U(1) Chern - Simons theory, are demonstrated to be in conflict with the firmly established holographic bound.

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. 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. In the special case of loop quantum gravity, the value of the Barbero - Immirzi parameter is found. Other values for this parameter, obtained under an additional assumption that the horizon is described by a U(1) Chern - Simons theory, are demonstrated to be in conflict with the firmly established holographic bound.

UR - http://www.scopus.com/inward/record.url?scp=84894414197&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:84894414197

SN - 9812567569

SN - 9789812567567

SP - 474

EP - 489

BT - Gribov Memorial Volume

T2 - Gribov Memorial Workshop Devoted to the 75th Birthday of V N Gribov: Quarks, Hadrons, and Strong Interactions

Y2 - 22 May 2005 through 24 May 2005

ER -

ID: 36642588