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Radiation of a quantized black hole. / Khriplovich, I. B.

в: Journal of Experimental and Theoretical Physics, Том 100, № 6, 23.08.2005, стр. 1075-1081.

Результаты исследований: Научные публикации в периодических изданиях › статья › Рецензирование

Harvard

Khriplovich, IB 2005, 'Radiation of a quantized black hole', Journal of Experimental and Theoretical Physics, Том. 100, № 6, стр. 1075-1081. https://doi.org/10.1134/1.1995791

APA

Khriplovich, I. B. (2005). Radiation of a quantized black hole. Journal of Experimental and Theoretical Physics, 100(6), 1075-1081. https://doi.org/10.1134/1.1995791

Vancouver

Khriplovich IB. Radiation of a quantized black hole. Journal of Experimental and Theoretical Physics. 2005 Авг. 23;100(6):1075-1081. https://doi.org/10.1134/1.1995791

Author

Khriplovich, I. B. / Radiation of a quantized black hole. в: Journal of Experimental and Theoretical Physics. 2005 ; Том 100, № 6. стр. 1075-1081.

BibTeX

@article{37b72cf6c0ba480db5a6e36e71e2a3ed,
title = "Radiation of a quantized black hole",
abstract = "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 and the value of the Barbero-Immirzi parameter are found. The discrete spectrum of thermal radiation of a black hole naturally fits the Wien profile. The natural widths of the lines are very small as compared to the distances between them. The total intensity of the thermal radiation is calculated.",
author = "Khriplovich, {I. B.}",
year = "2005",
month = aug,
day = "23",
doi = "10.1134/1.1995791",
language = "English",
volume = "100",
pages = "1075--1081",
journal = "Journal of Experimental and Theoretical Physics",
issn = "1063-7761",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "6",

}

RIS

TY - JOUR

T1 - Radiation of a quantized black hole

AU - Khriplovich, I. B.

PY - 2005/8/23

Y1 - 2005/8/23

N2 - 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 and the value of the Barbero-Immirzi parameter are found. The discrete spectrum of thermal radiation of a black hole naturally fits the Wien profile. The natural widths of the lines are very small as compared to the distances between them. The total intensity of the thermal radiation is calculated.

AB - 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 and the value of the Barbero-Immirzi parameter are found. The discrete spectrum of thermal radiation of a black hole naturally fits the Wien profile. The natural widths of the lines are very small as compared to the distances between them. The total intensity of the thermal radiation is calculated.

UR - http://www.scopus.com/inward/record.url?scp=23644456553&partnerID=8YFLogxK

U2 - 10.1134/1.1995791

DO - 10.1134/1.1995791

M3 - Article

AN - SCOPUS:23644456553

VL - 100

SP - 1075

EP - 1081

JO - Journal of Experimental and Theoretical Physics

JF - Journal of Experimental and Theoretical Physics

SN - 1063-7761

IS - 6

ER -

ID: 36642766