Three wormhole models are constructed in linear f(Q) gravity using varying Chaplygin, generalized Chaplygin, and varying barotropic equations of state, all of which violate the null energy condition at the throat.
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Study of Wormhole in $f(Q)$ gravity with some dark energy models
Three wormhole models are constructed in linear f(Q) gravity using varying Chaplygin, generalized Chaplygin, and varying barotropic equations of state, all of which violate the null energy condition at the throat.