Semiclassical Corrections to the Cardy-Verlinde Formula of Kerr Black Holes

Abstract

In this letter, we compute the corrections to the Cardy-Verlinde formula of $4-$dimensional Kerr black hole. These corrections are considered within the context of KKW analysis and arise as a result of the self-gravitational effect. Then we show, one can taking into account the semiclassical corrections of the Cardy-Verlinde entropy formula by just redefining the Virasoro operator $L_0$ and the central charge $c$.

8 pages

References in corpus (1)

• Bouncing cosmological solutions due to the self-gravitational corrections and their stability

Cited by in corpus (3)

• Entropic corrections to Newton's law
• A note on the Hawking radiation calculated by the quasi-classical tunneling method
• Corrections to the Cardy-Verlinde formula from the modified dispersion relation in extra dimensions