Gravitational decoupling for axially symmetric systems and
rotating black holes

J 2021

Gravitational decoupling for axially symmetric systems and rotating black holes

CONTRERAS, E.; Jorge Iván OVALLE ARAYA and R. CASADIO

Basic information

Original name

Gravitational decoupling for axially symmetric systems and rotating black holes

Authors

CONTRERAS, E.; Jorge Iván OVALLE ARAYA (152 Chile, belonging to the institution) and R. CASADIO

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:

URL

Impact factor

Impact factor: 5.407

RIV identification code

RIV/47813059:19630/21:A0000167

Organization unit

Institute of physics in Opava

DOI

https://doi.org/10.1103/PhysRevD.103.044020

UT WoS

000617042600006

EID Scopus

2-s2.0-85101010440

Keywords in English

MINIMAL GEOMETRIC DEFORMATION;HORIZON QUANTUM-MECHANICS;CHARGED COMPACT STAR;BRANE-WORLD STARS;ANISOTROPIC SOLUTIONS;GENERAL-RELATIVITY;SPACE-TIME;SHADOW;OBJECTS;MODELS

Abstract

In the original language

We introduce a systematic and direct procedure to generate hairy rotating black holes by deforming a spherically symmetric seed solution. We develop our analysis in the context of the gravitational decoupling approach, without resorting to the Newman-Janis algorithm. As examples of possible applications, we investigate how the Kerr black hole solution is modified by a surrounding fluid with conserved energy-momentum tensor. We find nontrivial extensions of the Kerr and Kerr-Newman black holes with primary hair. We prove that a rotating and charged black hole can have the same horizon as Kerr's, Schwarzschild's, or Reissner-Nordstrom's, thus showing possible observational effects of matter around black holes.

Cite

CONTRERAS, E.; Jorge Iván OVALLE ARAYA and R. CASADIO. Gravitational decoupling for axially symmetric systems and rotating black holes. Physical Review D. College Park (USA): American Physical Society, 2021, vol. 103, No 4, p. "044020-1"-"044020-11", 11 pp. ISSN 2470-0010. Available from: https://doi.org/10.1103/PhysRevD.103.044020.

@article{59481,
   author = {Contreras, E. and Ovalle Araya, Jorge Iván and Casadio, R.},
   article_location = {College Park (USA)},
   article_number = {4},
   doi = {https://doi.org/10.1103/PhysRevD.103.044020},
   keywords = {MINIMAL GEOMETRIC DEFORMATION;HORIZON QUANTUM-MECHANICS;CHARGED COMPACT STAR;BRANE-WORLD STARS;ANISOTROPIC SOLUTIONS;GENERAL-RELATIVITY;SPACE-TIME;SHADOW;OBJECTS;MODELS},
   language = {eng},
   issn = {2470-0010},
   journal = {Physical Review D},
   title = {Gravitational decoupling for axially symmetric systems and rotating black holes},
   url = {https://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.044020},
   volume = {103},
   year = {2021}
}

TY  - JOUR
ID  - 59481
AU  - Contreras, E. - Ovalle Araya, Jorge Iván - Casadio, R.
PY  - 2021
TI  - Gravitational decoupling for axially symmetric systems and rotating black holes
JF  - Physical Review D
VL  - 103
IS  - 4
SP  - "044020-1"-"044020-11"
EP  - "044020-1"-"044020-11"
PB  - American Physical Society
SN  - 24700010
KW  - MINIMAL GEOMETRIC DEFORMATION;HORIZON QUANTUM-MECHANICS;CHARGED COMPACT STAR;BRANE-WORLD STARS;ANISOTROPIC SOLUTIONS;GENERAL-RELATIVITY;SPACE-TIME;SHADOW;OBJECTS;MODELS
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.044020
N2  - We introduce a systematic and direct procedure to generate hairy rotating black holes by deforming a spherically symmetric seed solution. We develop our analysis in the context of the gravitational decoupling approach, without resorting to the Newman-Janis algorithm. As examples of possible applications, we investigate how the Kerr black hole solution is modified by a surrounding fluid with conserved energy-momentum tensor. We find nontrivial extensions of the Kerr and Kerr-Newman black holes with primary hair. We prove that a rotating and charged black hole can have the same horizon as Kerr's, Schwarzschild's, or Reissner-Nordstrom's, thus showing possible observational effects of matter around black holes.
ER  -

CONTRERAS, E.; Jorge Iván OVALLE ARAYA and R. CASADIO. Gravitational decoupling for axially symmetric systems and rotating black holes. \textit{Physical Review D}. College Park (USA): American Physical Society, 2021, vol.~103, No~4, p.~''044020-1''-''044020-11'', 11 pp. ISSN~2470-0010. Available from: https://doi.org/10.1103/PhysRevD.103.044020.

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