Thermodynamics of Graviton Condensate

TL;DR

This paper explores the thermodynamics of a graviton condensate black hole model, incorporating topological defects and new metrics, revealing corrections to Hawking temperature and establishing formal equivalences with known solutions.

Contribution

It introduces a thermodynamic framework for graviton condensate black holes with topological defects and proposes a new BEC-Kiselev metric extending the model to various matter contents.

Findings

Derived correction to Hawking temperature.

Identified negative pressure associated with the black hole.

Proposed a new BEC-Kiselev metric for different matter contents.

Abstract

In this work, we present the thermodynamic study of a model that considers the black hole as a condensate of gravitons. In this model, the spacetime is not asymptotically flat because of a topological defect that introduces an angle deficit in the spacetime like in Global Monopole solutions. We have obtained a correction to the Hawking temperature plus a negative pressure associated with the black hole of mass $M$. In this way, the graviton condensate, which is assumed to be at the critical point defined by the condition $\mu_{ch}$=0, has well-defined thermodynamic quantities $P$, $V$, $T_{h}$, $S$, and $U$ as any other Bose-Einstein condensate (BEC). In addition, we present a formal equivalence between the Letelier spacetime and the line element that describes the graviton condensate. We also discuss the Kiselev black hole, which can parametrize the most well-known spherically symmetric black holes. Finally, we present a new metric, which we will call the BEC-Kiselev solution, that allows us to extend the graviton condensate to the case of solutions with different matter contents.