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Wormhole in $f(Q)$ gravity

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arxiv 2203.06374 v2 pith:FKR5HCR5 submitted 2022-03-12 gr-qc

Foad Parsaei , Sara Rastgoo , P. K. Sahoo This is my paper · ORCID
classification gr-qc
keywords gravityequationsfunctionsolutionssomewormholeasymptoticallyconditions
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abstract

In this paper, exact asymptotically flat wormhole solutions in the context of symmetric teleparallel gravity, i.e., $f(Q)$ theory of gravity, are investigated. Since modified theories of gravity provide new field equations, we have analyzed some possible wormhole solutions by using modified field equations. Four different forms of the $f(Q)$ function are considered then the shape function is calculated with some different equations of state. Also we have used a power-law shape function with these models, which lead to an asymptotically barotropic equation of state. Some physical and mathematical properties of the solutions, like energy conditions and boundary conditions, are addressed .

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Cited by 1 Pith paper

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  1. Solar system tests in covariant f(Q) gravity

    gr-qc 2024-12 conditional novelty 5.0 of 10

    Solar system data bound the parameter α in f(Q)=Q+αQ^n-2Λ gravity, with limits that depend strongly on the chosen affine connection.

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