Quasinormal modes of modified gravity (MOG) black holes

DOI10.1016/j.physletb.2017.11.006zbMath1383.83122arXiv1711.03199OpenAlexW2767710001WikidataQ125911779 ScholiaQ125911779MaRDI QIDQ1707904

Luciano Manfredi, John W. Moffat, Jonas R. Mureika

Publication date: 4 April 2018

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1711.03199

Mathematics Subject Classification ID

Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35)

Related Items (10)

Distinguishing regular and singular black holes in modified gravity ⋮ Linear cosmological perturbations in scalar-tensor-vector gravity ⋮ Gravitational synchrotron radiation and Penrose process in STVG theory ⋮ Scattering of quantum fields by a MOG black hole ⋮ Quantum tunneling and quasinormal modes in the spacetime of the alcubierre warp drive ⋮ Exact cosmological black hole solutions in scalar tensor vector gravity ⋮ The Sagnac effect on a scale-dependent rotating BTZ black hole background ⋮ Photon trajectories on a first order scale-dependent static BTZ black hole ⋮ Shadows of Kerr-like black holes in a modified gravity theory ⋮ Superradiance in modified gravity (MOG)

Cites Work

• A new approach to black hole quasinormal modes: a review of the asymptotic iteration method
• On the gravitational instability in the Newtonian limit of MOG
• Perturbation theory in a framework of iteration methods
• Black hole quasinormal modes using the asymptotic iteration method
• Modified gravity (MOG), cosmology and black holes
• THE ASYMPTOTIC ITERATION METHOD FOR DIRAC AND KLEIN–GORDON EQUATIONS WITH A LINEAR SCALAR POTENTIAL
• Quasi-normal modes of stars and black holes

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