In this paper, the formation of specific static wormhole models is discussed, by assuming an $f(R,T)=R+2\ensuremath{\lambda}T$ extended theory of gravity, $T=\ensuremath{-}\ensuremath{\rho}+{P}_{r}+2{P}_{l}$ being the trace of the energy momentum tensor. In the first part, wormhole solutions are con...
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