  In the present article we propose a new hybrid shape function for wormhole
(WH)s in the modified $f(R,T)$ gravity. The proposed shape function satisfied
the conditions of WH geometry. Geometrical behavior of WH solutions are
discussed in both anisotropic and isotropic cases respectively. Also, the
stability of this model is obtained by determining the equilibrium condition.
The radial null energy condition and weak energy condition are validated in the
proposed shape function indicating the absence of exotic matter in modified
$f(R,T)$ gravity.
