Structure of $3D$ gravastars in the context of massive gravity
Abstract
In this paper, we investigate a new model of dimensional () gravitational vacuum stars (gravastars) with an isotropic matter distribution anti-de Sitter (AdS) spacetime in the context of massive gravity. For this purpose, we explore free singularity models with a specific equation of state. Using Mazur-Mottola's approach, we predict gravastars as alternatives to BTZ black holes in massive gravity. We find analytical solutions to the interior of gravastars free of singularities and event horizons. For a thin shell containing an ultra-relativistic stiff fluid, we discuss length, energy, and entropy. In conclusion, the parameter of massive gravity plays a significant role in predicting the proper length, energy contents and entropyand parameters of gravastars.
Keywords
Cite
@article{arxiv.2310.18287,
title = {Structure of $3D$ gravastars in the context of massive gravity},
author = {H. Barzegar and B. Eslam Panah and G. H. Bordbar and M. Bigdeli},
journal= {arXiv preprint arXiv:2310.18287},
year = {2023}
}
Comments
12 pages, 7 figures