Standard

Quantization of black holes. / Khriplovich, I. B.

в: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Том 431, № 1-2, 09.07.1998, стр. 19-21.

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

Harvard

Khriplovich, IB 1998, 'Quantization of black holes', Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, Том. 431, № 1-2, стр. 19-21. https://doi.org/10.1016/S0370-2693(98)00580-2

APA

Khriplovich, I. B. (1998). Quantization of black holes. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics, 431(1-2), 19-21. https://doi.org/10.1016/S0370-2693(98)00580-2

Vancouver

Khriplovich IB. Quantization of black holes. Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 1998 Июль 9;431(1-2):19-21. https://doi.org/10.1016/S0370-2693(98)00580-2

Author

Khriplovich, I. B. / Quantization of black holes. в: Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics. 1998 ; Том 431, № 1-2. стр. 19-21.

BibTeX

@article{ed57e124b64c4b77bc2a3f759d788553,
title = "Quantization of black holes",
abstract = "A simple argument is presented in favour of the equidistant spectrum for the horizon area of a black hole in semiclassical limit. The following quantization rules for the mass MN and horizon area ANj are proposed: MN = mp[N(N + 1)]1/4; ANj = 8πl2 p[√N(N + 1) + √N(N + 1) - j(j + 1)]. Here both N and j are nonnegative integers or half-integers.",
author = "Khriplovich, {I. B.}",
year = "1998",
month = jul,
day = "9",
doi = "10.1016/S0370-2693(98)00580-2",
language = "English",
volume = "431",
pages = "19--21",
journal = "Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics",
issn = "0370-2693",
publisher = "Elsevier",
number = "1-2",

}

RIS

TY - JOUR

T1 - Quantization of black holes

AU - Khriplovich, I. B.

PY - 1998/7/9

Y1 - 1998/7/9

N2 - A simple argument is presented in favour of the equidistant spectrum for the horizon area of a black hole in semiclassical limit. The following quantization rules for the mass MN and horizon area ANj are proposed: MN = mp[N(N + 1)]1/4; ANj = 8πl2 p[√N(N + 1) + √N(N + 1) - j(j + 1)]. Here both N and j are nonnegative integers or half-integers.

AB - A simple argument is presented in favour of the equidistant spectrum for the horizon area of a black hole in semiclassical limit. The following quantization rules for the mass MN and horizon area ANj are proposed: MN = mp[N(N + 1)]1/4; ANj = 8πl2 p[√N(N + 1) + √N(N + 1) - j(j + 1)]. Here both N and j are nonnegative integers or half-integers.

UR - http://www.scopus.com/inward/record.url?scp=0345826312&partnerID=8YFLogxK

U2 - 10.1016/S0370-2693(98)00580-2

DO - 10.1016/S0370-2693(98)00580-2

M3 - Article

AN - SCOPUS:0345826312

VL - 431

SP - 19

EP - 21

JO - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

JF - Physics Letters, Section B: Nuclear, Elementary Particle and High-Energy Physics

SN - 0370-2693

IS - 1-2

ER -

ID: 36645712