Quasinormal modes and optical properties of 4-D black holes in Einstein Power-Yang–Mills gravity
Dhruba Jyoti GogoiDepartment of Physics, Dibrugarh University, Dibrugarh 786004, Assam, IndiaJyatsnasree BoraDepartment of Physics, Dibrugarh University, Dibrugarh 786004, Assam, IndiaM. KoussourQuantum Physics and Magnetism Team, LPMC, Faculty of Science Ben M’sik, Casablanca Hassan II University, MoroccoYassine SekhmaniDépartement de Physique, Equipe des Sciences de la matiére et du rayonnement, ESMaR, Faculté des Sciences, Université Mohammed V de Rabat, Rabat, Morocco
2023en
ABI
Abstract
This paper explores the impact of the Yang–Mills charge parameter and the exponent term on a 4D black hole solution in the Einstein Power-Yang–Mills theory. Through an investigation of the massless scalar quasinormal mode spectrum, black hole shadow, and emission rate, we have determined that the effects of these two parameters are opposite. Specifically, the Yang–Mills charge parameter causes an increase in the real quasinormal frequencies with a correspondingly smaller damping rate. It also results in a smaller black hole shadow and a lower evaporation rate .
Identifiers
Citations and references
Cited by 60 references