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Embeddings of the black holes in a flat space. / Sheykin, A.A.; Grad, D.A.; Paston, S.A.

In: Proceedings of Science, Vol. PoS(QFTHEP 2013), 2013, p. 091_1-7.

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Sheykin AA, Grad DA, Paston SA. Embeddings of the black holes in a flat space. Proceedings of Science. 2013;PoS(QFTHEP 2013):091_1-7.

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Sheykin, A.A. ; Grad, D.A. ; Paston, S.A. / Embeddings of the black holes in a flat space. In: Proceedings of Science. 2013 ; Vol. PoS(QFTHEP 2013). pp. 091_1-7.

BibTeX

@article{27433ba8dc55440c80d38f2fc5fc6142,
title = "Embeddings of the black holes in a flat space",
abstract = "We study the explicit embeddings of static black holes. We obtain two new minimal embeddings of the Schwarzchild-de Sitter metric which smoothly cover both horizons of this metric. The lines of time for these embeddings are more complicated than hyperbolas. Also we shortly discuss the possibility of using non-hyperbolic embeddings for calculation of the black hole Hawking temperature in the Deser and Levin approach.",
author = "A.A. Sheykin and D.A. Grad and S.A. Paston",
year = "2013",
language = "English",
volume = "PoS(QFTHEP 2013)",
pages = "091_1--7",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",

}

RIS

TY - JOUR

T1 - Embeddings of the black holes in a flat space

AU - Sheykin, A.A.

AU - Grad, D.A.

AU - Paston, S.A.

PY - 2013

Y1 - 2013

N2 - We study the explicit embeddings of static black holes. We obtain two new minimal embeddings of the Schwarzchild-de Sitter metric which smoothly cover both horizons of this metric. The lines of time for these embeddings are more complicated than hyperbolas. Also we shortly discuss the possibility of using non-hyperbolic embeddings for calculation of the black hole Hawking temperature in the Deser and Levin approach.

AB - We study the explicit embeddings of static black holes. We obtain two new minimal embeddings of the Schwarzchild-de Sitter metric which smoothly cover both horizons of this metric. The lines of time for these embeddings are more complicated than hyperbolas. Also we shortly discuss the possibility of using non-hyperbolic embeddings for calculation of the black hole Hawking temperature in the Deser and Levin approach.

M3 - Article

VL - PoS(QFTHEP 2013)

SP - 091_1-7

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

ER -

ID: 5703240