Stellar modeling with quintessence field via embedding approach in Ratsall teleparallel gravity

This paper proposes a new model for anisotropic compact stars with quintessence in Rastall teleparallel gravity via embedding approach. In the gravity, the acquired field equations encompassing the anisotropic matter source as well as the quintessence field are studied using the specific character of the scalar torsion [Formula: see text] for the observed stars candidates PSRJ[Formula: see text]1416–2230, 4U[Formula: see text]1608–52, CenX–3, EXO 1785–248 and SMC[Formula: see text]X–1. All of the stellar structures under consideration are said to be advantageously independent of any central singularity and are stable. A thorough graphical analysis reveals that numerous physical properties critical for forming stellar structures are satisfied.