AdS Ellis wormholes with scalar field

In this paper, we study the spherically symmetric traversable wormholes with a scalar field supported by a phantom field in the anti-de Sitter (AdS) asymptotic spacetime. Despite coupling the scalar matter field, these wormholes remain massless and symmetric for reflection of the radial coordinate $r\to -r$. The solution possesses a finite Noether charge $Q$, which varies as a function of frequency $\omega$ with changes in the cosmological constant $\mathrm{\Lambda }$ and the throat size $r_0$. Under specific conditions, an approximate ``event horizon’’ will appear at the throat.