Long lived quasinormal modes in the effective quantum gravity

Two models for Schwarzschild-like black holes with quantum corrections, derived from the Hamiltonian constraints approach to quantum gravity while preserving general covariance, have been developed in Zhang et al. (Phys. Rev. D 111, L081504, 2025, arXiv:2407.10168 [gr-qc]). In this work, we study the quasinormal modes of a massive scalar field and demonstrate that the spectrum includes arbitrarily long-lived modes, known as quasi-resonances. Precise calculations using the Leaver method show good agreement with WKB data and time-domain integration within the range where these methods are reliable, specifically for small field masses. © The Author(s) 2025.

Авторы
Издательство
Springer New York LLC
Номер выпуска
10
Язык
English
Статус
Published
Номер
1166
Том
85
Год
2025
Организации
  • 1 RUDN University, Moscow, Moscow Oblast, Russian Federation
Ключевые слова
Black holes; Gravitation; Quantum theory; Relativity; Data domains; General covariance; Quantum correction; Quantum gravity; Quasi-resonance; Quasinormal modes; Scalar fields; Schwarzschild; Spectra's; Time domain analysis
Цитировать
Поделиться

Другие записи