Gravastar on the brane with a timelike extra dimension
Shounak Ghosh, Rikpratik Sengupta, Kazuharu Bamba

TL;DR
This paper constructs a stable, singularity-free gravastar model within the Shtanov-Sahni braneworld scenario, demonstrating how higher-dimensional effects naturally regularize the interior and support stability without thin-shell approximations.
Contribution
It provides the first fully analytic, finite-thickness gravastar solution in the SS braneworld, showing how higher-dimensional Weyl corrections induce stability and singularity avoidance.
Findings
Regularized interior geometry without singularities
Stable equilibrium solutions with negative effective mass
Intrinsic anisotropic pressures from Weyl corrections
Abstract
We construct a gravastar configuration within the Shtanov-Sahni (SS) braneworld scenario, characterized by a timelike extra dimension and negative brane tension. Unlike classical black holes, which inevitably culminate in central curvature singularities, our model demonstrates that the SS braneworld dynamics naturally regularize the interior geometry and prevent singularity formation. By solving the modified Einstein field equations induced on the brane, we obtain explicit interior, shell, and exterior solutions without invoking the idealized thin-shell approximation. The gravastar core is modeled as a Bose--Einstein condensate, while the intermediate shell consists of ultra-dense stiff matter. Bulk Weyl corrections induce anisotropic effective pressures on the brane, a feature that emerges intrinsically in this scenario and supports stability. We analyze the active gravitational mass,…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Astrophysical Phenomena and Observations · Cosmology and Gravitation Theories
