The generalized uncertainty principle impact onto the black hole thermodynamic phase transition

TL;DR

This paper investigates how the generalized uncertainty principle influences black hole thermodynamics and phase transitions, revealing new behaviors like remnants and multiple phase transitions depending on the sign of the GUP parameter.

Contribution

It introduces the effects of the generalized uncertainty principle on black hole thermodynamics, highlighting novel phase transition phenomena and remnant properties.

Findings

Positive GUP parameter leads to black hole remnants with finite temperature and zero heat capacity.

Black holes undergo multiple phase transitions, including Hawking-Page and Gross-Perry-Yaffe types.

Negative GUP parameter results in metastable remnants with finite temperature but zero mass.

Abstract

In this work, we conduct a study regarding the thermodynamic evolution and the phase transition of a black hole in a finite spherical cavity subject to the generalized uncertainty principle. The results demonstrate that both the positive and negative generalized uncertainty principle parameters $\beta_0$ can significantly affect the thermodynamic quantities, stability, critical behavior, and phase transition of the black hole. For $\beta_0>0$, the black hole forms a remnant with finite temperature, finite mass, and zero local heat capacity in the last stages of evolution, which can be regarded as an elementary particle. Meanwhile, it undergoes one second-order phase transition and two Hawking-Page-type phase transitions. The Gross-Perry-Yaffe phase transition occurs for both large black hole configuration and small black hole configuration. For $\beta_0<0$, the Gross-Perry-Yaffe phase transition occurs only for large black hole configuration, and the temperature and heat capacity of black hole remnant is finite, whereas its mass is zero. This indicates the remnant is metastable and would be in the Hawking-Page-type phase transition forever. Specifically, according to the viewpoint of corpuscular gravity, the remnant can be interpreted as an additional metastable tiny black hole configuration, which never appears in the original case and the positive correction case.