The Schwarzschild's Braneworld Solution

J. Ovalle

The Schwarzschild's Braneworld Solution

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arxiv 1009.3674 v1 pith:UTPADHCD submitted 2010-09-20 gr-qc hep-th

J. Ovalle This is my paper · ORCID

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In the context of the Randall-Sundrum braneworld, the minimal geometric deformation approach, which has been successfully used to generate exact interior solutions to Einstein's field equations for static braneworld stars with local and non-local bulk terms, is used to obtain the braneworld version of the Schwarzschild's interior solution. Using this new solution, the behaviour of the Weyl functions is elucidated in terms of the compactness for different stellar distributions.

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Braneworld Neutron Stars: Constraining Brane Tension with Observational Data
gr-qc 2025-01 conditional novelty 6.0 of 10

Using six neutron star equations of state, braneworld gravity can support the 2.5 to 2.67 solar mass object seen in GW190814 and gives a lower bound on brane tension near 2×10^37 dyne/cm^2.

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