Standard

Explicit isometric embeddings of black holes geometry with non-singular matter distribution. / Kapustin, A. D.; Paston, S. A.

в: Journal of Physics: Conference Series, Том 1697, № 1, 012082, 17.12.2020.

Результаты исследований: Научные публикации в периодических изданиях › статья в журнале по материалам конференции › Рецензирование

Harvard

Kapustin, AD & Paston, SA 2020, 'Explicit isometric embeddings of black holes geometry with non-singular matter distribution', Journal of Physics: Conference Series, Том. 1697, № 1, 012082. https://doi.org/10.1088/1742-6596/1697/1/012082

APA

Kapustin, A. D., & Paston, S. A. (2020). Explicit isometric embeddings of black holes geometry with non-singular matter distribution. Journal of Physics: Conference Series, 1697(1), [012082]. https://doi.org/10.1088/1742-6596/1697/1/012082

Vancouver

Kapustin AD, Paston SA. Explicit isometric embeddings of black holes geometry with non-singular matter distribution. Journal of Physics: Conference Series. 2020 Дек. 17;1697(1). 012082. https://doi.org/10.1088/1742-6596/1697/1/012082

Author

Kapustin, A. D. ; Paston, S. A. / Explicit isometric embeddings of black holes geometry with non-singular matter distribution. в: Journal of Physics: Conference Series. 2020 ; Том 1697, № 1.

BibTeX

@article{028398c0a87040d1be4bdb5cfff3e1c3,
title = "Explicit isometric embeddings of black holes geometry with non-singular matter distribution",
abstract = "The work is devoted to the construction of explicit embeddings for the metrics of the black holes, formed by nonsingular matter distribution. One of the possible examples of such type of solutions is regular black holes. Using the existing classification of minimal symmetric embeddings of the Schwarzschild metric as a base, we construct embeddings for regular black holes with de Sitter interior. Another simple example is black hole, formed by collapsing homogeneous spherically symmetric cloud of dustlike matter. We discuss embeddings for two variants of such black holes -the one with the eternally existing horizon, when dust ball never leaves the interior of the horizon, and another variant with the dynamically forming horizon. ",
author = "Kapustin, {A. D.} and Paston, {S. A.}",
note = "Funding Information: The work is supported by RFBR Grant No. 20-01-00081. Publisher Copyright: {\textcopyright} Published under licence by IOP Publishing Ltd. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.; International Conference PhysicA.SPb 2020 ; Conference date: 19-10-2020 Through 23-10-2020",
year = "2020",
month = dec,
day = "17",
doi = "10.1088/1742-6596/1697/1/012082",
language = "English",
volume = "1697",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",
url = "http://physica.spb.ru/, http://physica.spb.ru/archive/physicaspb2020/",

}

RIS

TY - JOUR

T1 - Explicit isometric embeddings of black holes geometry with non-singular matter distribution

AU - Kapustin, A. D.

AU - Paston, S. A.

N1 - Funding Information: The work is supported by RFBR Grant No. 20-01-00081. Publisher Copyright: © Published under licence by IOP Publishing Ltd. Copyright: Copyright 2020 Elsevier B.V., All rights reserved.

PY - 2020/12/17

Y1 - 2020/12/17

N2 - The work is devoted to the construction of explicit embeddings for the metrics of the black holes, formed by nonsingular matter distribution. One of the possible examples of such type of solutions is regular black holes. Using the existing classification of minimal symmetric embeddings of the Schwarzschild metric as a base, we construct embeddings for regular black holes with de Sitter interior. Another simple example is black hole, formed by collapsing homogeneous spherically symmetric cloud of dustlike matter. We discuss embeddings for two variants of such black holes -the one with the eternally existing horizon, when dust ball never leaves the interior of the horizon, and another variant with the dynamically forming horizon.

AB - The work is devoted to the construction of explicit embeddings for the metrics of the black holes, formed by nonsingular matter distribution. One of the possible examples of such type of solutions is regular black holes. Using the existing classification of minimal symmetric embeddings of the Schwarzschild metric as a base, we construct embeddings for regular black holes with de Sitter interior. Another simple example is black hole, formed by collapsing homogeneous spherically symmetric cloud of dustlike matter. We discuss embeddings for two variants of such black holes -the one with the eternally existing horizon, when dust ball never leaves the interior of the horizon, and another variant with the dynamically forming horizon.

UR - http://www.scopus.com/inward/record.url?scp=85098323799&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/1697/1/012082

DO - 10.1088/1742-6596/1697/1/012082

M3 - Conference article

AN - SCOPUS:85098323799

VL - 1697

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012082

T2 - International Conference PhysicA.SPb 2020

Y2 - 19 October 2020 through 23 October 2020

ER -

ID: 72597140