• Charge and/or spin limits for black holes at a non-commutative scale

• Fulltext

https://www.ias.ac.in/article/fulltext/pram/089/02/0026

• Keywords

Quantum gravity; non-commutative black hole; extremity

• Abstract

In the commutative geometrical background, one finds the total charge $\mathcal{(Q)}$ and/or the total angular momentum $\mathcal{(J)}$ of a generalized black hole of mass $M$ to be bounded by the condition $\mathcal{Q^{2} + (J/M)^{2} \leq M^{2}}$, whereas the inclusion of the concept of non-commutativity in geometry leads to a much more richer result. It predicts that the upper limit to $\mathcal{Q}$ and/or $\mathcal{J}$ is not fixed but depends on the mass/length scale of black holes; it (the upper limit to $\mathcal{Q}$ and/or $\mathcal{J}$ ) goes towards a ‘commutative limit’ when $M \gg \sqrt{\vartheta} (\sqrt{\vartheta}$ characterizes the minimal length scale) and rapidly diminishes towards zero with $M$ decreasing in the strongly non-commutative regime, until approaching a perfect zero value for $M \simeq 1.904\sqrt{\vartheta}$. We have performed separate calculations for a pure Kerr or a pure Reissner–Nordström black hole, and briefly done it for a generalized black hole.

• Author Affiliations

1. Rautara MNM High School, Rautara, Block: Habra-1, PS: Habra, (N) 24 Parganas 743 234, India

• Pramana – Journal of Physics

Volume 96, 2022
All articles
Continuous Article Publishing mode

• Editorial Note on Continuous Article Publication

Posted on July 25, 2019