Publication: Quasinormal modes of the electric potential in the 4 dimensional anti de sitter Reissner-norstöm black hole spacetime with scalar hair
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Issued Date
2021
Resource Type
Language
eng
File Type
application/pdf
ISSN
17426588
Other identifier(s)
2-s2.0-85100815009
Rights Holder(s)
มหาวิทยาลัยศรีนครินทรวิโรฒ
Bibliographic Citation
Journal of Physics: Conference Series. Vol 1719, No.1 (2021)
Suggested Citation
Kanjanaphomchom P., Musiri S. Quasinormal modes of the electric potential in the 4 dimensional anti de sitter Reissner-norstöm black hole spacetime with scalar hair. Journal of Physics: Conference Series. Vol 1719, No.1 (2021). doi:10.1088/1742-6596/1719/1/012039 Retrieved from: https://hdl.handle.net/20.500.14740/7898
Author(s)
Abstract
In this study, analytical calculations are performed to assess the quasinormal modes (qnm) of the perturbed electromagnetic potential within the a four-dimensional spacetime of the Reissner-Nordström (RN) anti-de Sitter (AdS) black holes which are dressed with scalar hair. The black holes serve as the solutions for the Einstein-Maxwell theory under a negative cosmological constant and conformally-coupled real self-interacting scalar field. When the strength of the scalar field is suitable, phase transition of the black holes occurs to create a new form of MTZ black holes. The electromagnetic field can then be perturbed and the qnm and their frequencies calculated in order to meet the boundary conditions both at the horizon and at the far distant region from the new MTZ black hole. In order to address a simplified version of this problem, this study investigates the case whereby the mass of the MTZ black hole is significantly less than the AdS radius. © Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence.