scholarly journals Quasinormal modes, quasiperiodic oscillations, and the shadow of rotating regular black holes in nonminimally coupled Einstein-Yang-Mills theory

2021 ◽  
Vol 103 (2) ◽  
Author(s):  
Kimet Jusufi ◽  
Mustapha Azreg-Aïnou ◽  
Mubasher Jamil ◽  
Shao-Wen Wei ◽  
Qiang Wu ◽  
...  

2015 ◽  
Vol 91 (8) ◽  
Author(s):  
Bobir Toshmatov ◽  
Ahmadjon Abdujabbarov ◽  
Zdeněk Stuchlík ◽  
Bobomurat Ahmedov


2021 ◽  
Vol 2021 (5) ◽  
Author(s):  
S. Prem Kumar ◽  
Andy O’Bannon ◽  
Anton Pribytok ◽  
Ronnie Rodgers

Abstract Four-dimensional $$ \mathcal{N} $$ N = 4 supersymmetric Yang-Mills theory, at a point on the Coulomb branch where SU(N) gauge symmetry is spontaneously broken to SU(N − 1) × U(1), admits BPS solitons describing a spherical shell of electric and/or magnetic charges enclosing a region of unbroken gauge symmetry. These solitons have been proposed as gauge theory models for certain features of asymptotically flat extremal black holes. In the ’t Hooft large N limit with large ’t Hooft coupling, these solitons are holographically dual to certain probe D3-branes in the AdS5 × S5 solution of type IIB supergravity. By studying linearised perturbations of these D3-branes, we show that the solitons support quasinormal modes with a spectrum of frequencies sharing both qualitative and quantitative features with asymptotically flat extremal black holes.



2020 ◽  
Vol 102 (10) ◽  
Author(s):  
M. Ghasemi-Nodehi ◽  
Mustapha Azreg-Aïnou ◽  
Kimet Jusufi ◽  
Mubasher Jamil


2017 ◽  
Vol 26 (14) ◽  
pp. 1750160 ◽  
Author(s):  
Wadbor Wahlang ◽  
Piyush A. Jeena ◽  
Sayan Chakrabarti

So far the study of black hole perturbations has been mostly focused upon the classical black holes with singularities at the origin and hidden by event horizon. Compared to that, the regular black holes are a completely new class of solutions arising out of modification of general theory of relativity by coupling gravity to an external form of matter. Therefore it is extremely important to study the behavior of such regular black holes under different types of perturbations. Recently a new regular Bardeen black hole solution with a de Sitter branch has been proposed by Fernando [ arXiv:1611.05337 [gr-qc]]. We compute the quasi-normal (QN) frequencies for the regular Bardeen de Sitter (BdS) black hole due to massless and massive scalar field perturbations as well as the massless Dirac perturbations. We analyze the behavior of both real and imaginary parts of QN frequencies by varying different parameters of the theory.



2021 ◽  
pp. 100930
Author(s):  
Javlon Rayimbaev ◽  
Bushra Majeed ◽  
Mubasher Jamil ◽  
Kimet Jusufi ◽  
Anzhong Wang




2021 ◽  
pp. 115539
Author(s):  
Chen Lan ◽  
Yan-Gang Miao ◽  
Hao Yang




2013 ◽  
Vol 87 (2) ◽  
Author(s):  
Antonino Flachi ◽  
José P. S. Lemos


2020 ◽  
Vol 102 (6) ◽  
Author(s):  
Yang Guo ◽  
Yan-Gang Miao


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