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Scalar radiation emitted by a source around a spherically symmetric black hole

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Publication:4963834
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DOI10.1142/S0218271820410084zbMath1454.83026arXiv2004.09446OpenAlexW3044700822MaRDI QIDQ4963834

Rafael P. Bernar

Publication date: 23 February 2021

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.09446


zbMATH Keywords

gravitational wavescircular motionstatic spacetime


Mathematics Subject Classification ID

Black holes (83C57) Gravitational waves (83C35)




Cites Work

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  • Generic instability of rotating relativistic stars
  • Regular black hole metrics and the weak energy condition
  • On the viability of regular black holes
  • Scalar waves in regular Bardeen black holes: Scattering, absorption and quasinormal modes
  • Corrigendum: Scalar radiation emitted from a source rotating around a black hole (2000 Class. Quantum Grav. 17 19)
  • Quasinormal modes of black holes and black branes
  • Quasinormal modes: the characteristic `sound' of black holes and neutron stars
  • Scalar radiation emitted from a source rotating around a black hole
  • Bardeen regular black hole with an electric source
  • The Large Scale Structure of Space-Time
  • The Bardeen model as a nonlinear magnetic monopole
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