Thin accretion disk signatures in dynamical Chern–Simons-modified gravity

DOI10.1088/0264-9381/27/10/105010zbMath1190.83083arXiv0909.1267OpenAlexW2071228628WikidataQ125704151 ScholiaQ125704151MaRDI QIDQ3570096

Francisco S. N. Lobo, Zoltan Kovacs, Tiberiu Harko

Publication date: 24 June 2010

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/0909.1267

Mathematics Subject Classification ID

Black holes (83C57) Einstein's equations (general structure, canonical formalism, Cauchy problems) (83C05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15) Exact solutions to problems in general relativity and gravitational theory (83C15) Radiative transfer in astronomy and astrophysics (85A25)

Related Items (9)

Landau damping for gravitational waves in parity-violating theories ⋮ Thin accretion disk onto slowly rotating black holes in Einstein-Æther theory ⋮ Study of relativistic accretion flow around KTN black hole with shocks ⋮ A new slow-rotating black hole solution in Chern-Simons axion of Einstein gravity ⋮ Shadow revisiting and weak gravitational lensing with Chern-Simons modification ⋮ Thin accretion disks around traversable wormholes ⋮ Particle dynamics and geometric optics in Chern-Simons black holes ⋮ Hawking radiation and particle dynamics in accelerating non-Kerr black holes ⋮ Distinguishing black holes and naked singularities with iron line spectroscopy

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