Stability Analysis of Scalar Perturbations Around a Magnetized Compact Object in General Relativity
The exterior region of a magnetized compact object, modeled using a modified Gutsunaev-Manko spacetime, is found to be stable under scalar perturbations, with the magnetization of the central object enhancing the stability by increasing the decay rate of perturbations.
Quasinormal Modes of a Massless Scalar Field in the Near-Nariai Limit of the Plebański-Demiański Black Hole
This paper analytically derives the quasinormal frequencies for a massless scalar field conformally coupled to gravity in the near-Nariai limit of the Plebański-Demiański black hole, demonstrating that the decay rate is quantized and depends only on the black hole's surface gravity.
Exploring the Impact of Semi-Classical Physics on the Quasinormal Mode Spectra of Black Holes
This paper investigates how semi-classical effects near the event horizon of a black hole, characterized by deviations from the Schwarzschild metric, influence the frequencies and damping times of its quasinormal modes, offering a potential method for detecting these subtle deviations through gravitational wave observations.
New Pairs of Purely Damped Quasinormal Modes Discovered in a Hot and Dense Strongly-Coupled Plasma
This research paper presents the discovery of a new structure of purely damped quasinormal modes (QNMs) in a hot and dense strongly-coupled plasma, modeled using the 2 R-Charge Black Hole (2RCBH) holographic construction. These new QNMs, characterized by purely imaginary frequencies, dominate the late-time equilibration of the plasma at high chemical potentials, suggesting upper bounds on equilibration times that cannot be surpassed by further doping.
Quasinormal Modes of Charged Lifshitz Black Holes with Scalar Hair in Einstein-Maxwell-Dilaton Gravity
This research paper investigates the stability and dynamic behavior of charged Lifshitz black holes with scalar hair in Einstein-Maxwell-Dilaton gravity by analyzing the impact of various black hole parameters on their quasinormal modes.
Quasinormal Modes of Slowly-Spinning Horizonless Compact Objects: An Analysis Using the Membrane Paradigm
Spinning horizonless compact objects, as opposed to black holes, can be differentiated by their unique quasinormal mode (QNM) spectrum, which is influenced by their compactness and reflectivity, properties best analyzed through the membrane paradigm framework.
다양한 스핀 필드에 대한 헤이워드 시공간에서의 해석적 QNM
본 논문에서는 역 멀티폴 수의 확장을 이용하여 스칼라, 디락 및 맥스웰 섭동에 대한 헤이워드 블랙홀 배경에서의 준정규 모드(QNM)에 대한 해석적 표현을 유도하고, 이 분석 공식이 ℓ>0에 대해 놀라운 정확도로 QNM을 근사화함을 보여줍니다.
ヘイワード時空における様々なスピンの場の解析的QNM
ヘイワードブラックホール時空におけるスカラー、ディラック、マクスウェルの摂動に対する準固有振動数（QNMs）の解析式を導出し、その精度を数値計算と比較検証した。
Analytical Expressions for Quasinormal Modes of Various Fields in the Hayward Spacetime and Their Accuracy Compared to Numerical Methods
This paper derives and validates accurate analytical expressions for the quasinormal modes of scalar, Dirac, and Maxwell fields in the Hayward black hole spacetime, providing insights into the behavior of quantum-corrected black holes.
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