A comparative study between EGB gravity and GTR by modelling compact stars
arXiv:1607.06664 · doi:10.1140/epjc/s10052-017-4675-2
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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