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- W4213012904 abstract "This research work provides an exhaustive investigation of the viability of different coupled wormhole (WH) geometries with the relativistic matter configurations in the $f(R,G,T)$ extended gravity framework. We consider a specific model in the context of $f(R,G,T)$-gravity for this purpose. Also, we assume a static spherically symmetric space-time geometry and a unique distribution of matter with a set of shape functions ($beta(r)$) for analyzing different energy conditions (ECs). In addition to this, we examined WH-models in the equilibrium scenario by employing anisotropic fluid. The corresponding results are obtained using numerical methods and then presented using different plots. In this case, $f(R,G,T)$ gravity generates additional curvature quantities, which can be thought of as gravitational objects that maintain irregular WH-situations. Based on our findings, we conclude that in the absence of exotic matter, WH can exist in some specific regions of the parametric space using modified gravity model as, $f(R,G,T) = R +alpha R^2+beta G^n+gamma Gln(G)+lambda T$." @default.
- W4213012904 created "2022-02-24" @default.
- W4213012904 creator A5041694650 @default.
- W4213012904 creator A5083850387 @default.
- W4213012904 date "2022-03-07" @default.
- W4213012904 modified "2023-10-18" @default.
- W4213012904 title "Some specific wormhole solutions in f(R, T) gravity" @default.
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- W4213012904 doi "https://doi.org/10.1088/1402-4896/ac55bd" @default.
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