Standard

Black holes in N>4 gravity. / Alexeyev, S.; Starodubceva, D.
In: Proceedings of Science, No. 1, 2010.

Research output: Contribution to journal › Conference article › peer-review

Harvard

Alexeyev, S & Starodubceva, D 2010, 'Black holes in N>4 gravity', Proceedings of Science, no. 1.

APA

Alexeyev, S., & Starodubceva, D. (2010). Black holes in N>4 gravity. Proceedings of Science, (1).

Vancouver

Alexeyev S, Starodubceva D. Black holes in N>4 gravity. Proceedings of Science. 2010;(1).

Author

Alexeyev, S. ; Starodubceva, D. / Black holes in N>4 gravity. In: Proceedings of Science. 2010 ; No. 1.

BibTeX

@article{17de321fa44e4663b3ad499ad76103a3,
title = "Black holes in N>4 gravity",
abstract = "We consider geodesic equations for a black hole solution in the Randall-Sundrum II scenario presented in [1]. This solution is a generalization of the Schwarzschild one and has the mathematical form of the Reissner-N{\"o}rdstrom solution, but with an additional {"}tidal charge{"} instead of the electric charge. We examine the behavior of geodesic parameters and show that the solution does not contradict the observational data and does not predict any fundamentally new effects. A more serious restriction on the {"}tidal charge{"} value can be extracted from the circular orbit equation. {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.",
author = "S. Alexeyev and D. Starodubceva",
year = "2010",
language = "English",
journal = "Proceedings of Science",
issn = "1824-8039",
publisher = "Sissa Medialab Srl",
number = "1",

}

RIS

TY - JOUR

T1 - Black holes in N>4 gravity

AU - Alexeyev, S.

AU - Starodubceva, D.

PY - 2010

Y1 - 2010

N2 - We consider geodesic equations for a black hole solution in the Randall-Sundrum II scenario presented in [1]. This solution is a generalization of the Schwarzschild one and has the mathematical form of the Reissner-Nördstrom solution, but with an additional "tidal charge" instead of the electric charge. We examine the behavior of geodesic parameters and show that the solution does not contradict the observational data and does not predict any fundamentally new effects. A more serious restriction on the "tidal charge" value can be extracted from the circular orbit equation. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

AB - We consider geodesic equations for a black hole solution in the Randall-Sundrum II scenario presented in [1]. This solution is a generalization of the Schwarzschild one and has the mathematical form of the Reissner-Nördstrom solution, but with an additional "tidal charge" instead of the electric charge. We examine the behavior of geodesic parameters and show that the solution does not contradict the observational data and does not predict any fundamentally new effects. A more serious restriction on the "tidal charge" value can be extracted from the circular orbit equation. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=84887373198

M3 - Conference article

JO - Proceedings of Science

JF - Proceedings of Science

SN - 1824-8039

IS - 1

ER -

ID: 37962234