Abstract: (919 Views)
The minimum-maximum behavior of orbital velocity of a rotating test body around a Kerr black hole is known as the Aschenbach effect. In this paper, we generalize this idea for the charged Kerr black hole(Kerr-Newman) in the de Sitter spacetime to find an indirect measurement of the charge of a black hole or rotating objects same as the other hair of the black hole.
Type of Study:
Research |
Subject:
Special Received: 2022/05/24 | Accepted: 2023/02/15 | Published: 2023/03/6