2021
Kerr-de Sitter black hole revisited
OVALLE ARAYA, Jorge Iván; E. CONTRERAS and Zdeněk STUCHLÍKBasic information
Original name
Kerr-de Sitter black hole revisited
Authors
OVALLE ARAYA, Jorge Iván (152 Chile, belonging to the institution); E. CONTRERAS and Zdeněk STUCHLÍK (203 Czech Republic, belonging to the institution)
Edition
Physical Review D, College Park (USA), American Physical Society, 2021, 2470-0010
Other information
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
References:
Impact factor
Impact factor: 5.407
RIV identification code
RIV/47813059:19630/21:A0000145
Organization unit
Institute of physics in Opava
UT WoS
000649079900003
EID Scopus
2-s2.0-85104744695
Keywords in English
FIELD;MASS
Tags
International impact, Reviewed
Changed: 8/2/2022 15:23, Mgr. Pavlína Jalůvková
Abstract
In the original language
We interpret the cosmological constant as the energy of the vacuum, and under a minimum amount of assumptions, we show that it is deformed in the vicinity of a black hole. This leads us to reexamine the Kerr-de Sitter solution. We provide a new solution, simpler and geometrically richer, which shows the impact of the rotation in form of a warped curvature. We carry out a detailed and exact study on the new black hole solution, and we conclude with a conjecture regarding the possible impact of our results on alternative theories.