Gravastar under the framework of braneworld gravity II: effect of the Kuchowicz metric function
Saibal Ray, Shounak Ghosh, Rikpratik Sengupta

TL;DR
This paper develops an improved gravastar model within braneworld gravity using the Kuchowicz metric function, demonstrating its stability and ability to describe high-energy compact objects with both obeying and violating energy conditions.
Contribution
It introduces the use of the Kuchowicz metric function in braneworld gravastar models, enhancing physical features and stability analysis over previous models.
Findings
Model satisfies all stability criteria.
Supports solutions obeying and violating energy conditions.
Effective in describing high-energy compact objects.
Abstract
In recent years, a class of compact objects called gravastars have drawn immense interest as regular solutions to end state stellar collapse. Since the energy density involved in collapse process is expected to be high, it is a natural choice to study such compact objects in context of modified gravity theories which reduce to General Relativity (GR) in the low energy regime. We have already framed a model of gravastar in such a modified gravity framework involving extra dimensional Randall-Sundrum (RS) single brane gravity~[Phys. Rev. D \textbf{102}, 024037 (2020)] \cite{Sengupta1}. As a sequel in the present paper we substantially improve our previous model by choosing the Kuchowicz function as one of the metric potentials, which leads to many new interesting results and physical features from our analysis as discussed in this paper. Also, we provide essential additional stability…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Galaxies: Formation, Evolution, Phenomena
