Area (or entropy) products for Newman-Unti-Tamburino class of Black Holes
arXiv:2006.15092 · doi:10.1016/j.physletb.2020.135521
Abstract
We compute area (or entropy) product formula for Newman-Unti-Tamburino (NUT) class of black holes. Specifically, we derive the area product of outer horizon and inner horizon () for Taub-NUT, Euclidean Taub-NUT black hole, Reissner-Nordström--Taub-NUT black hole, Kerr-Taub-NUT black hole and Kerr-Newman-Taub-NUT black hole under the formalism developed very recently by Wu et al. \cite{wu} [PRD 100, 101501(R) (2019)]. The formalism is that a generic four dimensional Taub-NUT spacetime should be described completely in terms of three or four different types of thermodynamic hairs. They are defined as the Komar mass (), the angular momentum (), the gravitomagnetic charge (), the dual (magnetic) mass . After incorporating this formalism, we show that the area (or entropy) product of both the horizons for NUT class of black holes are \emph{mass-independent}. Consequently, the area product of for these black holes are \emph{universal}. Which was previously known in the literature that the area product of said black holes are \emph{mass-dependent}. Finally, we can say that this universality is solely due to the presence of \emph{new conserved charges } which is closely analogue to the Kerr like angular momentum .
Published in PLB
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Cited by in corpus (6)
- Consistent mass formulas for the four-dimensional dyonic NUT-charged spacetimes
- Consistent mass formulas for higher even-dimensional Taub-NUT spacetimes and their AdS counterparts
- Energy Formula for Newman-Unti-Tamburino class of Black Holes
- Hidden conformal symmetry and pair production near the cosmological horizon in Kerr-Newman-Taub-NUT-de Sitter spacetime
- Entropy Product Function and Central charges in NUT Geometry
- Bekenstein-Hawking Entropy Products for NUT class of Black Holes in AdS Space