Dynamics of Charged and Rotating NUT Black Holes in Rastall Gravity

Understand

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.