Static spherically symmetric wormholes in gravity
arXiv:2206.01184 · doi:10.1088/1674-1137/ac7f22
Abstract
In this article we obtain wormhole solutions in the recently proposed extension of symmetric teleparallel gravity called gravity. Here, the gravitational Lagrangian is defined by an arbitrary function of and (where is the non-metricity scalar, while is the trace of the energy-momentum tensor). In this study, we obtain the field equations for a static spherically symmetric wormhole metric in the context of a general gravity. We study the wormhole solutions with (i) linear EoS and (ii) anisotropy relation. We adopt two different forms of (a) linear and (b) non-linear to investigate these solutions. We investigate the various energy conditions to look for preservation and violation among the solutions that we obtained. We find that NEC is violated in both cases of our assumed forms of . Finally, we perform the stability analysis using Tolman-Oppenheimer-Volkov (TOV) equation.
Chinese Physics C accepted version
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