Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior

@article{57604,
   author = {Konoplya, Roman},
   article_location = {College Park (USA)},
   article_number = {4},
   doi = {http://dx.doi.org/10.1103/PhysRevD.103.044033},
   keywords = {RELATIVISTIC GRAVITATIONAL COLLAPSE;HOLE NORMAL-MODES;BLACK-HOLE;NONSPHERICAL PERTURBATIONS;WAVE-PROPAGATION;TESTS},
   language = {eng},
   issn = {2470-0010},
   journal = {Physical Review D},
   title = {Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior},
   url = {https://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.044033},
   volume = {103},
   year = {2021}
}

TY  - JOUR
ID  - 57604
AU  - Konoplya, Roman
PY  - 2021
TI  - Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior
JF  - Physical Review D
VL  - 103
IS  - 4
SP  - "044033-1"-"044033-6"
EP  - "044033-1"-"044033-6"
PB  - American Physical Society
SN  - 24700010
KW  - RELATIVISTIC GRAVITATIONAL COLLAPSE;HOLE NORMAL-MODES;BLACK-HOLE;NONSPHERICAL PERTURBATIONS;WAVE-PROPAGATION;TESTS
UR  - https://journals.aps.org/prd/abstract/10.1103/PhysRevD.103.044033
N2  - Black hole (BH) solution in the conformal Weyl gravity is a generalization of the Schwarzschild spacetime which includes two additional constants appearing when integrating the third order differential equations for gravitational field. One constant looks like the effective cosmological constant providing the de Sitter asymptotic of the solution. The other constant allows one to describe flat rotation of galaxies without introducing of the dark matter. Here we show that the effective "dark matter" term in the metric function drastically changes the asymptotic behavior of the evolution of the wave function of a scalar field: after the Schwarzschild-like ringing phase, the ringing at another, non-Schwarzschildian, longer-lived frequency takes place before the beginning of the exponential asymptotic tail. Thus the evolution of the scalar field consists of the three qualitatively different stages: the Schwarzschild-like ringing phase, the effective dark matter ringing phase and the de Sitter phase characterized by exponential tails. The late-time behavior of the electromagnetic field is qualitatively different as well: the exponential tails appear even in the absence of the effective de Sitter term.
ER  - 

KONOPLYA, Roman. Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior. \textit{Physical Review D}. College Park (USA): American Physical Society, 2021, roč.~103, č.~4, s.~''044033-1''-''044033-6'', 6 s. ISSN~2470-0010. Dostupné z: https://dx.doi.org/10.1103/PhysRevD.103.044033.