Quasinormal modes of an improved Schwarzschild black hole
نویسندگان
چکیده
منابع مشابه
Black Hole Determinants and Quasinormal Modes
We derive an expression for functional determinants in thermal spacetimes as a product over the corresponding quasinormal modes. As simple applications we give efficient computations of scalar determinants in thermal AdS, BTZ black hole and de Sitter spacetimes. We emphasize the conceptual utility of our formula for discussing ‘1/N ’ corrections to strongly coupled field theories via the hologr...
متن کاملAsymptotic quasinormal modes of a noncommutative geometry inspired Schwarzschild black hole
We study the asymptotic quasinormal modes for the scalar perturbation of the noncommutative geometry inspired Schwarzschild black hole in (3+1) dimensions. We have considered M ≥ M0, which effectively correspond to a single horizon Schwarzschild black hole with correction due to noncommutativity. We have shown that for this situation the real part of the asymptotic quasinormal frequency is prop...
متن کاملM ay 2 00 2 On quasinormal modes of small Schwarzschild - Anti - de - Sitter black hole
We compute the quasinormal modes associated with decay of the massless scalar filed around a small Schwarzschild-Anti-de-Sitter black hole. The computations shows that when the horizon radius is much less than the anti-de-Sitter radius, the imaginary part of the frequency goes to zero as r d−2 + while the real part of ω decreases to its minimum and then goes to d − 1. Thus the quasinormal modes...
متن کاملAsymptotic Quasinormal Modes of d Dimensional Schwarzschild Black Hole with Gauss-Bonnet Correction
We obtain an analytic expression for the highly damped asymptotic quasinormal mode frequencies of the d ≥ 5-dimensional Schwarzschild black hole modified by the GaussBonnet term, which appears in string derived models of gravity. The analytic expression is obtained under the string inspired assumption that there exists a mimimum length scale in the system and in the limit when the coupling in f...
متن کاملScalar gravitational perturbations and quasinormal modes in the five dimensional Schwarzschild black hole
We calculate the quasinormal modes (QNMs) for gravitational perturbations of the Schwarzschild black hole in the five dimensional (5D) spacetime with a continued fraction method. As shown by Kodama and Ishibashi, the gravitational perturbations of higher-dimensional (higher-D) Schwarzschild black holes can be divided into three decoupled classes, namely scalar-gravitational, vectorgravitational...
متن کاملذخیره در منابع من
با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید
ژورنال
عنوان ژورنال: Physics of the Dark Universe
سال: 2020
ISSN: 2212-6864
DOI: 10.1016/j.dark.2020.100639