Noncommutative wormhole solutions in f(G) gravity

In this paper, we study noncommutative static spherically symmetric wormhole solutions in the context of modified Gauss-Bonnet gravity. We explore these solutions either by assuming a viable f(G) model to construct shape function or by specifying the shape function to deduce f(G) model. The energy conditions are discussed for both types of wormholes. In the first case, we find a physically acceptable wormhole solution threaded by normal matter for all values of radial coordinate r while the second case gives physical solution only for large values of r.