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A study on existence of Wormhole in Lemaitre-Tolman-Bondi model

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arxiv 2409.01331 v1 pith:XMOOG7JD submitted 2024-09-02 gr-qc

classification gr-qc
keywords areabeenexistencelemaitre-tolman-bondiradiuswormholebackgroundconditions
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An investigation has been done for possible existence of evolving wormhole (WH) solution in the background of inhomogeneous Lemaitre-Tolman-Bondi (LTB) space-time geometry. Using separable product form of the geometric (or area) radius, the shape function can be evaluated in terms of the functional part of the radial coordinate in the area radius. The conditions for a viable WH configuration have been examined.

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  1. Gravitational lensing by Lema\^{\i}tre-Tolman-Bondi wormholes in a Friedmann universe

    gr-qc 2025-09 conditional novelty 6.0 of 10

    The angular size of a dust wormhole's shadow in a closed Friedmann universe first decreases, then increases with observation time, following a power-law relation in the wormhole size.

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