A comparative study between EGB gravity and GTR by modelling compact stars

Abstract

In this paper we utilise the Krori-Barua ansatz to model compact stars within the framework of Einstein- Gauss-Bonnet (EGB) gravity. The thrust of our investigation is to carry out a comparative analysis of the physical properties of our models in EGB and classical general relativity theory.

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Cited by in corpus (14)

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• A conformally flat realistic anisotropic model for a compact star
• Orthogonal splitting of the Riemann curvature tensor and its implications in modeling compact stellar structures
• Compact star in Tolman Kuchowicz spacetime in background of Einstein Gauss Bonnet gravity
• Interior solutions of relativistic stars with anisotropic matter in scale-dependent gravity
• Charged compact star model in Einstein-Maxwell-Gauss-Bonnet gravity
• Linear and Riccati equations in generating functions for stellar models in general relativity
• Anisotropic Dark Matter Stars
• Anisotropic solution for polytropic stars in 4D Einstein-Gauss-Bonnet gravity
• Strange star with Krori-Barua potential in presence of anisotropy
• Quark stars with isotropic matter in Hořava gravity and Einstein-æther theory
• Properties of relativistic star in 5-D Einstein-Gauss-Bonnet gravity
• Compact star model in Einstein Gauss-Bonnet Gravity within the framework of Finch Skea space time
• Boson stars, neutron stars and black holes in five dimensions