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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.

Quasinormal modes of an electrically charged Kalb-Ramond black hole

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 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.

Paper Structure

This paper contains 12 sections, 46 equations, 6 figures, 4 tables.

Figures (6)

  • Figure 1: Error analysis.
  • Figure 2: The trend of gravitational fundamental QNF with respect to violation parameter $l$ under different boundary cutoff $r_\mathrm{inf}$.
  • Figure 3: Error analysis in RN cases under 3 order expansion at horizon and 5 order expansion at infinity.
  • Figure 4: Effective potential components compared with RN case.
  • Figure 5: Deviation of effective potential components from RN case at different violation parameter $l$.
  • ...and 1 more figures