Wormhole solutions in f(Q,T)=αQ+βT gravity exist for Lm=-T and Lm=ρ, with non-exotic asymptotically flat geometries supported by ordinary fluids whose properties depend on the Lm choice.
Taking into account pr(r) = ωρ (r), (42) and applying Eqs.(35) and (36) it can be obtained b(r) = rn1(ω,β ), (43) n1(ω,β ) = 1 + 3β β − ω (1 + 2β )
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Wormholes in $f(Q,T)$ gravity with different matter Lagrangian density
Wormhole solutions in f(Q,T)=αQ+βT gravity exist for Lm=-T and Lm=ρ, with non-exotic asymptotically flat geometries supported by ordinary fluids whose properties depend on the Lm choice.