| TOSHMATOV, Bobir, Cosimo BAMBI, Bobomurat AHMEDOV, Zdeněk STUCHLÍK a Jan SCHEE. Scalar perturbations of nonsingular nonrotating black holes in conformal gravity. Physical Review D. 2017, roč. 96, č. 6, s. „064028-1“-„064028-10“, 10 s. ISSN 2470-0010. Dostupné z: https://dx.doi.org/10.1103/PhysRevD.96.064028. |
Další formáty:
BibTeX
LaTeX
RIS
@article{29869,
author = {Toshmatov, Bobir and Bambi, Cosimo and Ahmedov, Bobomurat and Stuchlík, Zdeněk and Schee, Jan},
article_number = {6},
doi = {http://dx.doi.org/10.1103/PhysRevD.96.064028},
keywords = {scalar perturbations; black holes; conformal gravity},
language = {eng},
issn = {2470-0010},
journal = {Physical Review D},
title = {Scalar perturbations of nonsingular nonrotating black holes in conformal gravity},
url = {https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.064028},
volume = {96},
year = {2017}
}
TY - JOUR
ID - 29869
AU - Toshmatov, Bobir - Bambi, Cosimo - Ahmedov, Bobomurat - Stuchlík, Zdeněk - Schee, Jan
PY - 2017
TI - Scalar perturbations of nonsingular nonrotating black holes in conformal gravity
JF - Physical Review D
VL - 96
IS - 6
SP - „064028-1“-„064028-10“
EP - „064028-1“-„064028-10“
SN - 24700010
KW - scalar perturbations
KW - black holes
KW - conformal gravity
UR - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.064028
L2 - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.96.064028
N2 - We study scalar and electromagnetic perturbations of a family of nonsingular nonrotating black hole spacetimes that are solutions in a large class of conformally invariant theories of gravity. The effective potential for scalar perturbations depends on the exact form of the scaling factor. Electromagnetic perturbations do not feel the scaling factor, and the corresponding quasinormal mode spectrum is the same as in the Schwarzschild metric. We find that these black hole metrics are stable under scalar and electromagnetic perturbations. Assuming that the quasinormal mode spectrum for scalar perturbations is not too different from that for gravitational perturbations, we can expect that the calculation of the quasinormal mode spectrum and the observation with gravitational wave detectors of quasinormal modes from astrophysical black holes can constrain the scaling factor and test these solutions.
ER -
TOSHMATOV, Bobir, Cosimo BAMBI, Bobomurat AHMEDOV, Zdeněk STUCHLÍK a Jan SCHEE. Scalar perturbations of nonsingular nonrotating black holes in conformal gravity. \textit{Physical Review D}. 2017, roč.~96, č.~6, s.~„064028-1“-„064028-10“, 10 s. ISSN~2470-0010. Dostupné z: https://dx.doi.org/10.1103/PhysRevD.96.064028.
|
