KONOPLYA, Roman and Olexandr ZHYDENKO. Simply rotating higher dimensional black holes in Einstein-Gauss-Bonnet theory. Physical Review D. US - Spojené státy americké, 2020, vol. 102, No 8, p. "084030-1"-"084030-13", 13 pp. ISSN 1550-7998. Available from: https://dx.doi.org/10.1103/PhysRevD.102.084030.
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Basic information
Original name Simply rotating higher dimensional black holes in Einstein-Gauss-Bonnet theory
Authors KONOPLYA, Roman (804 Ukraine, belonging to the institution) and Olexandr ZHYDENKO (804 Ukraine, belonging to the institution).
Edition Physical Review D, US - Spojené státy americké, 2020, 1550-7998.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher United States of America
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/20:A0000012
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.1103/PhysRevD.102.084030
UT WoS 000577074000001
Keywords in English ONE-LOOP DIVERGENCES; SYMMETRICAL-SOLUTIONS; SPACE
Tags , FÚ2020, GA19-03950S, RIV21
Tags International impact, Reviewed
Links GA19-03950S, research and development project.
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 19/4/2021 12:52.
Abstract
Using perturbative expansion in terms of powers of the rotation parameter a we construct the axisymmetric and asymptotically flat black-hole metric in the D-dimensional Einstein- Gauss-Bonnet theory. In five-dimensional spacetime we find two solutions to the field equations, describing the asymptotically flat black holes, though only one of them is perturbative in mass, that is, goes over into the Minkowski spacetime when the black-hole mass goes to zero. We obtain the perturbative black-hole solution up to the order O(alpha a(3)) for any D, where alpha is the Gauss-Bonnet coupling, while the D = 5 solution which is nonperturbative in mass is found in analytic form up to the order O(alpha a(7)). In order to check the convergence of the expansion in a we analyze characteristics of photon orbits in this spacetime and compute frequencies of the photon orbits and radius of the photon sphere.
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