J
2021
Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior
KONOPLYA, Roman
Základní údaje
Originální název
Conformal Weyl gravity via two stages of quasinormal ringing and late-time behavior
Vydání
Physical Review D, College Park (USA), American Physical Society, 2021, 2470-0010
Další údaje
Typ výsledku
Článek v odborném periodiku
Stát vydavatele
Spojené státy
Utajení
není předmětem státního či obchodního tajemství
Kód RIV
RIV/47813059:19630/21:A0000111
Organizační jednotka
Fyzikální ústav v Opavě
Klíčová slova anglicky
RELATIVISTIC GRAVITATIONAL COLLAPSE;HOLE NORMAL-MODES;BLACK-HOLE;NONSPHERICAL PERTURBATIONS;WAVE-PROPAGATION;TESTS
Příznaky
Mezinárodní význam, Recenzováno
Návaznosti
GA19-03950S, projekt VaV.
V originále
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.
Zobrazeno: 25. 12. 2024 10:19