New Black Hole Solutions in f(P) Gravity and their Thermodynamic Nature

TL;DR

This paper introduces new black hole solutions in f(P) gravity, demonstrating their thermodynamic properties and stability, including analytical calculations of entropy, temperature, and specific heat.

Contribution

It constructs the first static-spherically symmetric black hole solutions in f(P) gravity and analyzes their thermodynamic behavior.

Findings

Black hole solutions generalize Schwarzschild

Solutions are thermodynamically stable at small horizon radii

Analytical expressions for entropy, temperature, and specific heat

Abstract

Black holes are the fascinating objects in the universe. They represent extreme deformations in spacetime geometry. Here, we construct f(P) gravity and the first example of static-spherically symmetric black hole solution in f(P) gravity and discuss their thermodynamics. Using the numerical approach and series solution, we discover the solution and demonstrate that it is a generalization of Schwarzschild. The solution is characterized by a single function that satisfies a nonlinear fourth order differential equation. Interestingly, we can analytically calculate the solution s specific heat, Wald entropy, and Hawking temperature as a function of horizon radius. After analyzing the specific heat, we discovered that the black hole is thermodynamically stable over a small horizon radius.