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Ish: Simulated image of the shadow of the Kerr–Newman–NUT–Kiselev black hole in the Rastall gravity with a thin accretion disk
Black hole shadow as a test of general relativity: quadratic gravity
Dimitry Ayzenberg, Nicolás Yunes
Maqola201811 iqtibosABITHE MASS DISTRIBUTION OF STELLAR-MASS BLACK HOLES
Will M. Farr, Niharika Sravan, Andrew G. Cantrell +4
Maqola20117 iqtibosABIThermodynamics and phase transition in rotational Kiselev black hole
Zhaoyi Xu, Yi Liao, Jiancheng Wang
Maqola20196 iqtibosABIThin accretion disks in<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>f</mml:mi><mml:mo stretchy="false">(</mml:mo><mml:mi>R</mml:mi><mml:mo stretchy="false">)</mml:mo></mml:math>modified gravity models
C. S. J. Pun, Zoltán Kovács, Tiberiu Harko
Maqola20085 iqtibosABIObservational signatures of wormholes with thin accretion disks
Suvankar Paul, Rajibul Shaikh, Pritam Banerjee +1
Maqola20205 iqtibosABIGYOTO: a new general relativistic ray-tracing code
F H Vincent, T Paumard, E Gourgoulhon +1
Maqola20114 iqtibosABIThin accretion disk onto slowly rotating black holes in Einstein-Æther theory
Cheng Liu, Sen Yang, Qiang Wu +1
Maqola20223 iqtibosABI