Accretion of New Variable Modified Chaplygin Gas and Generalized Cosmic Chaplygin Gas onto Schwarzschild and Kerr-Newman Black holes

TL;DR

This paper investigates how dark energy fluids, specifically NVMCG and GCCG, accrete onto Schwarzschild and Kerr-Newman black holes, affecting their mass and angular momentum, with derived expressions for critical velocities and mass changes.

Contribution

It provides new analytical expressions for the critical velocity, mass change, and angular momentum variation during dark energy accretion onto these black holes.

Findings

Black hole mass increases due to dark energy accretion.

Angular momentum increases for Kerr-Newman black holes during accretion.

Critical velocity decreases as fluid flows towards the black holes.

Abstract

In this work, we have studied accretion of the dark energies NVMCG and GCCG onto the Schwarzschild and Kerr-Newman Black holes. We find the expression of the critical four velocity component which gradually decreases for the fluid flow towards the Schwarzschild as well as Kerr-Newman Black hole. We also find the expression for change of masses of the black hole in both cases. For the Kerr-Newman black hole which is rotating and charged we calculate the specific angular momentum and total angular momentum. We showed that in both cases due to accretion of the dark energy mass of the black hole increases and angular momentum increases in case of Kerr-Newman black hole.