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相关论文: Quasinormal modes and Stability Analysis for 4-dim…

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We study z=4 Topological black hole in 4+1 dimensional Horava-Lifshitz gravity and we calculate analytically the quasinormal modes of scalar perturbations and from these quasinormal modes we show that z=4 Topological black hole in 4+1…

广义相对论与量子宇宙学 · 物理学 2015-06-11 Ramon Becar , P. A. Gonzalez , Yerko Vasquez

In this work, we probe the stability of a $z=3$ three-dimensional Lifshitz black hole by using scalar and spinorial perturbations. We found an analytical expression for the quasinormal frequencies of the scalar probe field, which perfectly…

高能物理 - 理论 · 物理学 2013-05-30 Bertha Cuadros-Melgar , Jeferson de Oliveira , C. E. Pellicer

We study scalar perturbations for a four-dimensional asymptotically Lifshitz black hole in conformal gravity with dynamical exponent z=0, and spherical topology for the transverse section, and we find analytically and numerically the…

广义相对论与量子宇宙学 · 物理学 2015-10-14 Marcela Catalan , Eduardo Cisternas , P. A. Gonzalez , Yerko Vasquez

We study scalar perturbations in the background of a Topological Lifshitz black hole in four dimensions. We compute analytically the quasinormal modes and from these modes we show that Topological Lifshitz black hole is stable. On the other…

广义相对论与量子宇宙学 · 物理学 2015-06-05 P. A. Gonzalez , Felipe Moncada , Yerko Vasquez

We consider scalar field perturbations about asymptotically Lifshitz black holes with dynamical exponent z in D dimensions. We show that, for suitable boundary conditions, these Lifshitz black holes are stable under scalar field…

高能物理 - 理论 · 物理学 2012-06-05 Alex Giacomini , Gaston Giribet , Mauricio Leston , Julio Oliva , Sourya Ray

We consider scalar and spinorial perturbations on a background described by a $z=3$ three-dimensional Lifshitz black hole. We obtained the corresponding quasinormal modes which perfectly agree with the analytical result for the quasinormal…

高能物理 - 理论 · 物理学 2013-11-21 B. Cuadros-Melgar , Jeferson de Oliveira , C. E. Pellicer

We study scalar perturbations of four dimensional topological nonlinear charged Lifshitz black holes with spherical and plane transverse sections, and we find numerically the quasinormal modes for scalar fields. Then, we study the stability…

广义相对论与量子宇宙学 · 物理学 2016-03-23 Ramon Becar , P. A. Gonzalez , Yerko Vasquez

We study the quasinormal modes of scalar field perturbations in the background of non-Abelian hyperscaling violating Lifshitz black holes. We find that the quasinormal frequencies have no real part so there is no oscillatory behavior in the…

高能物理 - 理论 · 物理学 2016-12-09 Ramón Bécar , P. A. González , Yerko Vásquez

Motivated by the recent interest in the study of the spacetimes that are asymptotically Lifshitz and in order to extend some previous results, we calculate exactly the quasinormal frequencies of the electromagnetic field in a D-dimensional…

广义相对论与量子宇宙学 · 物理学 2015-06-19 A. Lopez-Ortega

In this article, we study the stability of black hole solutions found in the context of dilatonic Horava-Lifshitz gravity in $1+1$ dimensions by means of the quasinormal modes approach. In order to find the corresponding quasinormal modes,…

广义相对论与量子宇宙学 · 物理学 2016-02-22 Miguel Cruz , Manuel Gonzalez-Espinoza , Joel Saavedra , Diego Vargas-Arancibia

We study neutral massless scalar field perturbations around an extreme dilaton black hole in 2 +1 dimensions: the wave equations of the massless scalar field is shown to be exactly solvable in terms of Whittaker functions. Thus, the…

广义相对论与量子宇宙学 · 物理学 2022-07-27 Sharmanthie Fernando , P. A. González , Yerko Vásquez

In a D-dimensional Lifshitz black hole we calculate exactly the quasinormal frequencies of a test Dirac field in the massless and zero angular eigenvalue limits. These results are an extension of the previous calculations in which the…

广义相对论与量子宇宙学 · 物理学 2014-09-26 A. Lopez-Ortega

We study quasi-normal modes for a higher dimensional black hole with Lifshitz scaling, as these quasi-normal modes can be used to test Lifshitz models with large extra dimensions. Furthermore, as the effective Planck scale is brought down…

高能物理 - 理论 · 物理学 2020-02-20 S. Sedigheh Hashemi , Mahdi Kord Zangeneh , Mir Faizal

We find the connection between thermodynamic quantities and quasinormal frequencies in Lifshitz black holes. It is shown that the globally stable Lifshitz black holes have pure imaginary quasinormal frequencies. We also show that by…

高能物理 - 理论 · 物理学 2013-05-30 Yun Soo Myung , Taeyoon Moon

We study the quasinormal modes of fermionic perturbations for an asymptotically Lifshitz black hole in 4-dimensions with dynamical exponent z=2 and plane topology for the transverse section, and we find analytically and numerically the…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Marcela Catalan , Eduardo Cisternas , P. A. Gonzalez , Yerko Vasquez

We study the stability of black holes that are solutions of the dilaton gravity derived from string-theoretical models in two and five dimensions against to scalar field perturbations, using the Quasinormal Modes (QNMs) approach. In order…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Ramón Becar , Samuel Lepe , Joel Saavedra

In this paper, we investigate massive charged scalar perturbations in four-dimensional charged Lifshitz-AdS black holes with scalar hair, within the framework of Einstein--Maxwell--Dilaton (EMD) gravity. Using the improved asymptotic…

高能物理 - 理论 · 物理学 2025-09-18 Xufen Zhang , Shan Wu , Rui-Hong Yue , Ming Zhang , De-Cheng Zou

We have studied the scalar perturbation of static charged dilaton black holes in 2+1 dimensions. The black hole considered here is a solution to the low-energy string theory in 2+1 dimensions. It is asymptotic to the anti-de Sitter space.…

高能物理 - 理论 · 物理学 2014-08-21 Sharmanthie Fernando

We study the quasinormal modes of the massless scalar perturbation in the background of a deformed black hole in the Ho\v{r}ava-Lifshitz gravity with coupling constant $\lambda=1$. Our results show that the quasinormal frequencies depend on…

广义相对论与量子宇宙学 · 物理学 2015-03-13 Songbai Chen , Jiliang Jing

Black holes have their proper oscillations, which are called the quasi-normal modes. The proper oscillations of astrophysical black holes can be observed in the nearest future with the help of gravitational wave detectors. Quasi-normal…

广义相对论与量子宇宙学 · 物理学 2009-05-26 Alexander Zhidenko
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