Abstract
This paper explores static wormhole solutions through Noether symmetry technique in the framework of f(G,T) gravity, where G and T indicate the Gauss–Bonnet invariant and trace of the energy-momentum tensor, respectively. We consider isotropic fluid configuration to derive the symmetry generators with conserved parameters. We evaluate possible viable wormhole solutions and explore their stable behavior by considering the Tolman–Oppenheimer–Volkoff equation. For different forms of the red-shift parameter, we examine the effects of curvature-matter coupling as well as shape function on wormhole geometry. The graphical behavior of null/weak energy bounds for ordinary as well as effective energy-momentum tensor is investigated. We conclude that viable wormhole solutions exist for a specific functional form of this gravity.
Published Version
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