Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity

Abstract

In this work, we generalized the Kerr-Newman-NUT black hole solution in Rastall gravity from Ref. 1. Here we are more focused on the black hole dynamics such as the event horizons, ergosurface, ZAMO, thermodynamic properties, and the equatorial circular orbit around the black hole such as static radius limit, null equatorial circular orbit, and innermost stable circular orbit. We present how the NUT and Rastall parameter affects the dynamic of the black hole.

arXiv comment24 pages, 30 figures, Prepared for submission to IJMPD

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• CFT Duals on Rotating Charged Black Holes Surrounded by Quintessence
• Rotating black holes and exotic compact objects in the Kerr/CFT correspondence within Rastall gravity
• Chaos and fast scrambling delays of dyonic Kerr-Sen-AdS${}_4$ black hole and its ultra-spinning version
• Rotating and twisting charged black holes with cloud of strings and quintessence
• Effects of Rastall parameter on perturbation of dark sectors of the Universe
• Stationary Solution to Charged Hairy Black Hole in AdS4: Kasner Interior, Rotating Shock Waves, and Fast Scrambling
• Rotational mass of anisotropic neutron stars within Rastall gravity
• Rotating neutron stars with chaotic magnetic fields in general relativity and Rastall gravity