Noncanonical Phase-Space Noncommutative Black Holes

TL;DR

This paper introduces a noncanonical phase-space noncommutative extension of a cosmological model to describe black hole interiors, analyzing thermodynamics and comparing with classical Hawking quantities.

Contribution

It presents a novel noncanonical phase-space noncommutative model for black hole interiors, extending previous frameworks and analyzing thermodynamic properties.

Findings

Temperature and entropy depend on mass similarly to Hawking quantities

The model provides a consistent thermodynamic description of noncommutative black holes

Comparison shows agreement with classical black hole thermodynamics

Abstract

In this contribution we present a noncanonical phase-space noncommutative (NC) extension of a Kantowski Sachs (KS) cosmological model to describe the interior of a Schwarzschild black hole (BH). We evaluate the thermodynamical quantities inside this NC Schwarzschild BH and compare with the well known quantities. We find that for a NCBH the temperature and entropy have the same mass dependence as the Hawking quantities for a Schwarzschild BH.