Quasinormal Modes of Phantom Scalar Perturbation in Background of Reissner—Nordström Black Hole

2011 ◽  
Vol 55 (2) ◽  
pp. 221-226 ◽  
Author(s):  
Qi-Yuan Pan ◽  
Ru-Keng Su
Keyword(s):  
Black Hole ◽  
Quasinormal Modes ◽  
Scalar Perturbation ◽  
Phantom Scalar

scholarly journals Stability and phase transition of rotating Kaluza–Klein black holes

2021 ◽  
Vol 81 (12) ◽  
Author(s):  
Seyed Hossein Hendi ◽  
Somayeh Hajkhalili ◽  
Mubasher Jamil ◽  
Mehrab Momennia
Keyword(s):  
Black Hole ◽  
Black Hole Solution ◽  
Canonical Ensemble ◽  
Quasinormal Modes ◽  
Scalar Perturbation ◽  
Thermodynamic Quantities ◽  
Resonance Modes ◽  
Maxwell Electrodynamics ◽  
The Stability ◽  
Kaluza Klein

AbstractIn this paper, we investigate the thermodynamics and phase transitions of a four-dimensional rotating Kaluza–Klein black hole solution in the presence of Maxwell electrodynamics. Calculating the conserved and thermodynamic quantities shows that the first law of thermodynamics is satisfied. To find the stable black hole’s criteria, we check the stability in the canonical ensemble by analyzing the behavior of the heat capacity. We also consider a massive scalar perturbation minimally coupled to the background geometry of the four-dimensional static Kaluza–Klein black hole and investigate the quasinormal modes by employing the Wentzel–Kramers–Brillouin (WKB) approximation. The anomalous decay rate of the quasinormal modes spectrum is investigated by using the sixth-order WKB formula and quasi-resonance modes of the black hole are studied with averaging of Padé approximations as well.

scholarly journals Wave dynamics of phantom scalar perturbation in the background of Schwarzschild black hole

2009 ◽  
Vol 670 (4-5) ◽  
pp. 276-280 ◽  
Author(s):  
Songbai Chen ◽  
Jiliang Jing ◽  
Qiyuan Pan
Keyword(s):  
Black Hole ◽  
Scalar Perturbation ◽  
Schwarzschild Black Hole ◽  
Wave Dynamics ◽  
Phantom Scalar

Quasinormal modes of scalar perturbation around a quantum-corrected Schwarzschild black hole

2014 ◽  
Vol 350 (2) ◽  
pp. 721-726 ◽  
Author(s):  
Mahamat Saleh ◽  
Bouetou Bouetou Thomas ◽  
Timoleon Crepin Kofane
Keyword(s):  
Black Hole ◽  
Quasinormal Modes ◽  
Scalar Perturbation ◽  
Schwarzschild Black Hole

scholarly journals ASYMPTOTIC QUASINORMAL MODES OF A NONCOMMUTATIVE GEOMETRY INSPIRED SCHWARZSCHILD BLACK HOLE

2007 ◽  
Vol 22 (11) ◽  
pp. 2047-2056 ◽  
Author(s):  
PULAK RANJAN GIRI
Keyword(s):  
Black Hole ◽  
Noncommutative Geometry ◽  
Quasinormal Modes ◽  
Space Time ◽  
Hawking Temperature ◽  
Scalar Perturbation ◽  
Schwarzschild Black Hole ◽  
The Real ◽  
Quasinormal Frequency

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 proportional to ln (3). The effect of noncommutativity of space–time on quasinormal frequency arises through the constant of proportionality, which is Hawking temperature TH(θ). We also consider the two-horizons case and show that in this case also the real part of the asymptotic quasinormal frequency is proportional to ln (3).

CHOPTUIK SCALING AND QUASINORMAL MODES IN THE ADS/CFT CORRESPONDENCE

2002 ◽  
Vol 17 (20) ◽  
pp. 2750-2750
Author(s):  
DANNY BIRMINGHAM
Keyword(s):  
Black Hole ◽  
Imaginary Part ◽  
Three Dimensional ◽  
Quasinormal Modes ◽  
Particle Collision ◽  
Scalar Perturbation ◽  
Btz Black Hole ◽  
Return To Equilibrium ◽  
Scaling Parameter ◽  
Exact Analytic Expression

The exact quasinormal frequencies for scalar perturbations of the three-dimensional BTZ black hole were presented1. The timescale for the decay of the scalar perturbation is given by the imaginary part of the quasinormal frequencies. Via the AdS/CFT correspondence, one then obtains a prediction of the timescale for return to equilibrium of the dual conformal field theory. By studying a two-particle collision process, an exact analytic expression for the Choptuik scaling parameter of the BTZ black hole was obtained2. A possible connection between the Choptuik scaling parameter and the imaginary part of the quasinormal frequencies was explored1.

scholarly journals Gravitational Quasinormal Modes of Regular Phantom Black Hole

2017 ◽  
Vol 2017 ◽  
pp. 1-19 ◽  
Author(s):  
Jin Li ◽  
Kai Lin ◽  
Hao Wen ◽  
Wei-Liang Qian
Keyword(s):  
Black Hole ◽  
Scalar Field ◽  
Quasinormal Modes ◽  
De Sitter ◽  
Asymptotically Flat ◽  
Gravitational Perturbations ◽  
Phantom Scalar ◽  
Quantum Interpretation ◽  
The Stability ◽  
Phantom Scalar Field

We investigate the gravitational quasinormal modes (QNMs) for a type of regular black hole (BH) known as phantom BH, which is a static self-gravitating solution of a minimally coupled phantom scalar field with a potential. The studies are carried out for three different spacetimes: asymptotically flat, de Sitter (dS), and anti-de Sitter (AdS). In order to consider the standard odd parity and even parity of gravitational perturbations, the corresponding master equations are derived. The QNMs are discussed by evaluating the temporal evolution of the perturbation field which, in turn, provides direct information on the stability of BH spacetime. It is found that in asymptotically flat, dS, and AdS spacetimes the gravitational perturbations have similar characteristics for both odd and even parities. The decay rate of perturbation is strongly dependent on the scale parameterb, which measures the coupling strength between phantom scalar field and the gravity. Furthermore, through the analysis of Hawking radiation, it is shown that the thermodynamics of such regular phantom BH is also influenced byb. The obtained results might shed some light on the quantum interpretation of QNM perturbation.

scholarly journals Massive scalar perturbations on Myers-Perry–de Sitter black holes with a single rotation

2020 ◽  
Vol 80 (11) ◽  
Author(s):  
Supakchai Ponglertsakul ◽  
Bogeun Gwak
Keyword(s):  
Black Holes ◽  
Black Hole ◽  
Quasinormal Modes ◽  
Analytic Formula ◽  
Asymptotic Iteration Method ◽  
Scalar Perturbation ◽  
De Sitter ◽  
Spin Parameter ◽  
Higher Dimensional ◽  
The Stability

AbstractThis study investigates the stability of higher-dimensional singly rotating Myers-Perry–de Sitter (MP–dS) black holes against scalar field perturbations. The phase spaces of MP-dS black holes with one spin parameter are discussed. Additionally, the quasinormal modes (QNMs) of MP-dS black holes are calculated via the asymptotic iteration method and sixth-order Wentzel–Kramers–Brillouin approximation. For near-extremal MP-dS black holes, the event horizon may be considerably close to the cosmological horizon. In such cases, the Pöschl–Teller technique yields an accurate analytic formula for the QNMs. It is found that when the spin parameter of a black hole increases, the scalar perturbation modes oscillate at higher frequencies and decay faster. Furthermore, the MP-dS black hole with a single rotation is found to be stable under perturbation.

scholarly journals Significance of black hole quasinormal modes: A closer look

2020 ◽  
Vol 101 (10) ◽  
Author(s):  
Ramin G. Daghigh ◽  
Michael D. Green ◽  
Jodin C. Morey
Keyword(s):  
Black Hole ◽  
Quasinormal Modes
Sign in / Sign up

Export Citation Format

Share Document