Wormhole solutions through hyperbolic model in f(R,T) gravity

Abstract

In this paper, we employed a hyperbolic viable model in the [Formula: see text] gravity to inspect the presence of wormhole geometries combined with the configurations of relativistic matter. In this regard, the static form of spherically symmetric spacetime was taken into account and the validity of energy conditions was verified by considering a particular form of matter and a combination of shape functions. The equilibrium background of wormhole models was analyzed by using the concept of an anisotropic fluid and explored our findings graphically. These nonstandard astrophysical wormhole models were further supported by the gravitational entity resulting from the [Formula: see text] gravity in the form of extra-curvature quantities. Furthermore, in the presence of an anisotropic fluid and [Formula: see text] gravity, it was demonstrated that the wormhole models might actually exist in a couple of zones in the parameter space without the requirement of exotic matter.