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Charged wormholes in f(R,T) extended theory of gravity

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arxiv 1710.07680 v2 pith:MBIZ4AEJ submitted 2017-10-19 gr-qc hep-th

classification gr-qchep-th
keywords conditionsenergyextendedgravitywormholeschargedmattersome
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abstract

Wormholes are a solution for General Relativity field equations which characterize a passage or a tunnel that connects two different regions of space-time and is filled by some sort of exotic matter, that does not satisfy the energy conditions. On the other hand, it is known that in extended theories of gravity, the extra degrees of freedom once provided may allow the energy conditions to be obeyed and, consequently, the matter content of the wormhole to be non-exotic. In this work, we obtain, as a novelty in the literature, solutions for charged wormholes in the $f(R,T)$ extended theory of gravity. We show that the presence of charge in these objects may be a possibility to respect some stability conditions for their metric. Also, remarkably, the energy conditions are respected in the present approach.

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Cited by 2 Pith papers

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

  1. Rotating traversable wormholes and particle dynamics in $f(R,T)$ gravity

    gr-qc 2026-05 unverdicted novelty 5.0 of 10

    Rotating traversable wormholes in f(R,T) gravity are supported by anisotropic fluid satisfying null and strong energy conditions in the slow-rotation approximation, with particle dynamics and gravitational lensing analyzed.

  2. Investigating Evolving Wormholes in $f(R,T)$ Gravity

    gr-qc 2025-01 conditional novelty 4.0 of 10

    Evolving wormhole solutions in f(R,T)=αR^m+βT gravity are shown to satisfy the null, weak, strong, and dominant energy conditions for tuned parameters, avoiding exotic matter at the throat.

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