Gravastar model in the structure of $f(R,L_{m}, T)$ modified theory of gravity
Meghanil Sinha, S. Surendra Singh

TL;DR
This paper explores the Gravastar model within the $f(R,L_{m}, T)$ modified gravity framework, analyzing its structure, properties, and junction conditions, offering an alternative to black holes with a focus on its theoretical characteristics.
Contribution
It introduces a Gravastar model in $f(R,L_{m}, T)$ gravity with a specific functional form, analyzing its internal structure, energy conditions, and junction conditions, extending previous models to modified gravity.
Findings
The interior region has negative energy density with $ ho = -p$.
The exterior is described by Schwarzschild-de-Sitter spacetime.
Junction conditions are analyzed using Darmois-Israel formalism.
Abstract
The Gravastar ( or the Gravitational Vacuum Star ) is a very serious alternatives proposed to the principle of the Black Hole, the model of which was originally developed by Mazur and Mottola. A Gravastar is an astronomically hypothetically condensed object which is a gravitationally dark vacuum star or a gravitational vacuum condensate star, which is singularity free, spherically symmetric and also super compact. The current study concerns about the model of the Gravastar in the modified gravity considering the form . From Mazur-Mottola \cite{Mazur}-\cite{Mottola}, we get to know that a Gravastar model has three distinct regions having various Equations of State (EoS). We have inquired into the interior portion with the space-time considering , for the dark sector of the interior region, here the negative matter-energy…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Cosmology and Gravitation Theories · Black Holes and Theoretical Physics
