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相关论文: Massive vector field perturbations in the Schwarzs…

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The decay of massive scalar field in the Schwarzschild black hole background is investigated here by consideration its quasinormal spectrum. It has been proved that the so-called $quasi-resonant$ modes, which are arbitrary long living…

广义相对论与量子宇宙学 · 物理学 2009-11-10 R. A. Konoplya , A. V. Zhidenko

We study perturbations of massive and massless vector fields on a Schwarzschild black-hole background, including a non-minimal coupling between the vector field and the curvature. The coupling is given by the Horndeski vector-tensor…

广义相对论与量子宇宙学 · 物理学 2022-06-08 Sebastian Garcia-Saenz , Aaron Held , Jun Zhang

We revisit the peculiar electromagnetic quasinormal mode spectrum of an asymptotically anti-de Sitter Schwarzschild black hole. Recent numerical calculations have shown that some quasinormal mode frequencies become purely overdamped at some…

广义相对论与量子宇宙学 · 物理学 2022-10-21 Sean Fortuna , Ian Vega

We compute precise values of quasinormal modes of a massive scalar field in the background of the Schwarzschild-like brane-localised black holes. It is shown that the quasinormal spectrum of the massive field differs qualitatively from that…

广义相对论与量子宇宙学 · 物理学 2024-03-12 Antonina F. Zinhailo

We find the high overtones of gravitational and electromagnetic quasinormal spectrum of the Schwarzschild-de Sitter black hole. The calculations show that the real parts of the electromagnetic modes asymptotically approach zero. The…

高能物理 - 理论 · 物理学 2009-11-10 R. A. Konoplya , A. Zhidenko

We investigate the late-time behavior of the massive vector field in the background of the Schwarzschild and Schwarzschild-de Sitter black holes. For Schwarzschild black hole, at intermediately late times the massive vector field is…

广义相对论与量子宇宙学 · 物理学 2008-11-26 R. A. Konoplya , C. Molina , A. Zhidenko

We present the quasinormal frequencies of the massive scalar field in the background of a Schwarzchild black hole surrounded by quintessence with the third-order WKB method. The mass of the scalar field $u$ plays an important role in…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Chunrui Ma , Yuanxing Gui , Wei Wang , Fujun Wang

We investigate the classical stability of the higher-dimensional Schwarzschild black holes against linear perturbations, in the framework of a gauge-invariant formalism for gravitational perturbations of maximally symmetric black holes,…

高能物理 - 理论 · 物理学 2009-11-10 Akihiro Ishibashi , Hideo Kodama

We investigate the pseudospectrum of a Schwarzschild-like spacetime within the framework of black hole perturbation theory to analyze a counterintuitive assertion regarding the instability of quasinormal modes. Recent findings suggest that…

广义相对论与量子宇宙学 · 物理学 2025-05-14 Pedro Henrique Croti Siqueira , Lucas Tobias de Paula , Rodrigo Panosso Macedo , Maurício Richartz

We study quasinormal spectrum of massive scalar field in the $D$-dimensional black hole background. We found the qualitatively different dependence on the field mass of the fundamental modes for $D\geq6$. The behaviour of higher modes is…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Alexander Zhidenko

We study in special limiting cases quasinormal modes of massive scalar fields in the Schwarzschild-de Sitter black hole backgrounds. We determine the lower limit on the mass parameter of the scalar field that allows the waves with…

广义相对论与量子宇宙学 · 物理学 2017-07-25 Bobir Toshmatov , Zdeněk Stuchlík

Recent work applying the notion of pseudospectrum to gravitational physics showed that the quasinormal mode spectrum of black holes is unstable, with the possible exception of the longest-lived (fundamental) mode. The fundamental mode…

广义相对论与量子宇宙学 · 物理学 2022-03-29 Mark Ho-Yeuk Cheung , Kyriakos Destounis , Rodrigo Panosso Macedo , Emanuele Berti , Vitor Cardoso

We find the gravitational resonance (quasinormal) modes of the higher dimensional Schwarzschild and Reissner-Nordstrem black holes. The effect on the quasinormal behavior due to the presence of the $\lambda$ term is investigated. The QN…

高能物理 - 理论 · 物理学 2009-11-10 R. A. Konoplya

Disturbing of a spacetime geometry may result in the appearance of an oscillating and damped radiation - the so-called quasinormal modes. Their periods of oscillations and damping coefficients carry unique information about the mass and the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Janusz Karkowski , Edward Malec , Zdobyslaw Swierczynski

We analyze the evolution of perturbations of a (charged) massive scalar field near a regular Simpson-Visser black hole, allowing for a non-zero external magnetic field. We show that the damping rate of the quasinormal frequencies is…

广义相对论与量子宇宙学 · 物理学 2024-12-13 Akbar Davlataliev , Bakhtiyor Narzilloev , Ibrar Hussain , Ahmadjon Abdujabbarov , Bobomurat Ahmedov

The quasinormal-mode spectrum of the Schwarzschild-de Sitter black hole is studied in the limit of near-equal black-hole and cosmological radii. It is found that the mode_frequencies_ agree with the P"oschl-Teller approximation to one more…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Alec Maassen van den Brink

We have studied quasinormal modes of scalar perturbations of a black hole in massive gravity. The parameters of the theory, such as the mass of the black hole, the scalar charge of the black hole and the spherical harmonic index is varied…

广义相对论与量子宇宙学 · 物理学 2015-06-23 Sharmanthie Fernando , Tyler Clark

Besides the well-known quasinormal modes, the gravitational spectrum of a Schwarzschild black hole also has a continuum part on the negative imaginary frequency axis. The latter is studied numerically for quadrupole waves. The results show…

广义相对论与量子宇宙学 · 物理学 2009-11-10 P. T. Leung , Alec Maassen van den Brink , K. W. Mak , K. Young

We present a thorough analysis for the quasinormal (QN) behavior, associated with the decay of scalar, electromagnetic and gravitational perturbations, of Schwarzschild-anti-de Sitter black holes. As it is known the anti-de Sitter (AdS) QN…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Vitor Cardoso , Roman Konoplya , Jose' P. S. Lemos

The quasinormal modes (QNMs) associated with the decay of Dirac field perturbation around a Schwarzschild black hole is investigated by using continued fraction and Hill-determinant approaches. It is shown that the fundamental quasinormal…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Jiliang Jing
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