TOSHMATOV, Bobir, Cosimo BAMBI, Bobomurat AHMEDOV, Ahmadjon ABDUJABBAROV and Zdeněk STUCHLÍK. Energy conditions of non-singular black hole spacetimes in conformal gravity. European Physical Journal C. 2017, vol. 77, No 8, p. „542-1“-„542-10“, 10 pp. ISSN 1434-6044. Available from: https://dx.doi.org/10.1140/epjc/s10052-017-5112-2.
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Basic information
Original name Energy conditions of non-singular black hole spacetimes in conformal gravity
Authors TOSHMATOV, Bobir (860 Uzbekistan, guarantor, belonging to the institution), Cosimo BAMBI (380 Italy), Bobomurat AHMEDOV (860 Uzbekistan), Ahmadjon ABDUJABBAROV (860 Uzbekistan) and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution).
Edition European Physical Journal C, 2017, 1434-6044.
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 The European Physical Journal C
RIV identification code RIV/47813059:19240/17:A0000010
Organization Filozoficko-přírodovědecká fakulta – Slezská univerzita v Opavě – Repository
Doi http://dx.doi.org/10.1140/epjc/s10052-017-5112-2
UT WoS 000407634200004
Keywords in English conformal gravity; energy conditions; black holes
Tags GB14-37086G, SGS-14-2016, ÚF
Tags International impact, Reviewed
Links GB14-37086G, research and development project.
Changed by Changed by: Jan Hladík, učo 1305. Changed: 4/4/2018 15:24.
Abstract
Conformal gravity can elegantly solve the problem of spacetime singularities present in Einstein's gravity. For every physical spacetime, there is an infinite family of conformally equivalent singularity-free metrics. In the unbroken phase, every non-singular metric is equivalent and can be used to infer the physical properties of the spacetime. In the broken phase, a Higgs-like mechanism should select a certain vacuum, which thus becomes the physical one. However, in the absence of the complete theoretical framework we do not know how to select the right vacuum. In this paper, we study the energy conditions of non-singular black hole spacetimes obtained in conformal gravity assuming they are solutions of Einstein's gravity with an effective energy-momentum tensor. We check whether such conditions can be helpful to select the vacuum of the broken phase.
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