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Braneworld stars and black holes

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arxiv hep-th/0606006 v1 pith:EXUTTERJ submitted 2006-06-01 hep-th astro-phgr-qc

classification hep-thastro-phgr-qc
keywords braneworldbulkblackbranefullsolutionsolutionscorrespond
verification ladder T0 review T1 audit T2 compute T3 formal
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We look for spherically symmetric star or black hole solutions on a Randall-Sundrum brane from the perspective of the bulk. We take a known bulk solution, and analyse possible braneworld trajectories within it that correspond, from the braneworld point of view, to solutions of the brane Tolman-Oppenheimer-Volkoff equations. Our solutions are therefore embedded consistently into a full bulk solution. We find the full set of static gravitating matter sources on a brane in a range of bulk spacetimes, analyzing which can correspond to physically sensible sources. Finally, we look at time-dependent trajectories in a Schwarzschild--anti de Sitter spacetime as possible descriptions of time-dependent braneworld black holes, highlighting some of the general features one might expect, as well as some of the difficulties involved in getting a full solution to the question.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. 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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