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.
vahedi A, Moharami Zare M. Minimum-maximum structure of orbital velocity of a test body near Kerr-Newman-(A)dS spacetime. Journal title 2022; 6 (2) URL: http://jmrph.khu.ac.ir/article-1-208-en.html