Quasinormal modes of an electrically charged Kalb-Ramond black hole
Yun-Tao Gu, Wen-Di Guo, Yu-Xiao Liu
TL;DR
This work analyzes quasinormal modes of an electrically charged Kalb-Ramond black hole in a framework with spontaneous Lorentz violation. The odd-parity perturbations of the coupled gravitational and electromagnetic fields form a two-component, undecouplable system governed by a 2×2 matrix of effective potentials, requiring matrix-valued Leaver continued fractions and direct integration for the QNM spectrum. A discriminant-based eigenvalue recognition method is developed to identify mode types when decoupling is incomplete. The results show that the LV parameter $l=\xi_2 b^2/2$ shifts the real part of the fundamental QNMs approximately linearly while leaving the imaginary part largely unaffected, with a careful error analysis addressing boundary effects and expansion order; the RN and Schwarzschild limits validate the numerical approaches. Overall, the findings provide a principled approach to probing Planck-scale LV through black hole ringdown signals and offer practical guidance on parameter regimes and mode identification in undecouplable multi-field perturbations.
Abstract
Lorentz violation serves as a significant feature in many modified theories of gravity. In particular, spontaneous Lorentz violation induced by the Kalb-Ramond field has attracted considerable attention. Recently, an electrically charged black hole solution within the Kalb-Ramond framework was proposed. In this study, we investigate the quasinormal modes of the resulting ``undecouplable'' system using both the matrix-valued continued fraction method and the matrix-valued direct integration method. Additionally, we develop a new approach to distinguish between different modes in such ``undecouplable'' systems. An error analysis is performed, and the influence of Lorentz violation on the fundamental quasinormal modes is systematically analyzed within a suitable parameter range.
