The highly damped quasinormal modes of extremal Reissner–Nordström and Reissner–Nordström–de Sitter black holes
From MaRDI portal
Publication:5454608
DOI10.1088/0264-9381/25/5/055001zbMATH Open1136.83022arXiv0708.1333OpenAlexW2054929484MaRDI QIDQ5454608
Ramin G. Daghigh, Michael Green
Publication date: 31 March 2008
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Abstract: We analyze in detail the highly damped quasinormal modes of -dimensional extremal Reissner-Nordstrm and Reissner-Nordstrm-de Sitter black holes. We only consider the extremal case where the event horizon and the Cauchy inner horizon coincide. We show that, even though the topology of the Stokes/anti-Stokes lines in the extremal case is different than the non-extremal case, the highly damped quasinormal mode frequencies of extremal black holes match exactly with the extremal limit of the non-extremal black hole quasinormal mode frequencies.
Full work available at URL: https://arxiv.org/abs/0708.1333
Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47)
Related Items (3)
Area spectra of \(d\)-dimensional extreme Reissner-Nordström black holes ⋮ Damped modes for a bosonic quantum oscillator in the near-horizon geometry of the BTZ black hole ⋮ Asymptotic quasinormal frequencies of different spin fields in d-dimensional spherically-symmetric black holes
This page was built for publication: The highly damped quasinormal modes of extremal Reissner–Nordström and Reissner–Nordström–de Sitter black holes
Report a bug (only for logged in users!)Click here to report a bug for this page (MaRDI item Q5454608)