Compact Objects in 4D Einstein Gauss Bonnet Gravity A Data Based Perspective

TL;DR

This paper investigates how dark energy models influence the mass accretion of black holes and wormholes within 4D Einstein Gauss-Bonnet gravity, using observational data to determine the most fitting models and their cosmic implications.

Contribution

It introduces a data-driven analysis of dark energy effects on compact objects in 4D EGB gravity, comparing multiple DE parameterizations with observational constraints.

Findings

Bayesian analysis favors CPL and BA models, with CPL providing the best fit.

Black holes show transitions between quintessence and phantom eras under certain DE models.

Wormholes tend to favor phantom-dominated eras, contrasting black hole behavior.

Abstract

Cosmic evolution is the most sensational topic among researchers of modern cosmology. This article explores cosmic evolution in 4D Einstein Gauss Bonnet gravity, focusing on mass accretion of compact objects (black holes and wormholes) by dark energy. Three DE models CPL, JBP, and BA parameterizations are studied within 4D EGB gravity, with their Hubble parameters derived and compared against observational data (Cosmic Chronometers, Type Ia Supernovae, and Baryon Acoustic Oscillations). Bayesian analysis favors the CPL and BA models, with CPL providing the best fit. For black holes, mass accretion of CPL and JBP DE shows transitions between quintessence and phantom eras, while BA and $\Lambda$CDM strictly exhibit quintessence-like behavior, driving cosmic acceleration. In contrast, wormholes exhibit the opposite trend, favoring a phantom-dominated era for the BA and $\Lambda$CDM models. The study highlights the dynamic nature of DE in 4D EGB gravity and its role in cosmic expansion.