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://dx.doi.org/10.1103/PhysRevD.103.044020. |
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@article{59481, author = {Contreras, E. and Ovalle Araya, Jorge Iván and Casadio, R.}, article_location = {College Park (USA)}, article_number = {4}, doi = {http://dx.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://dx.doi.org/10.1103/PhysRevD.103.044020.
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