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This paper presents the study of dark-energy compact stars in the context ofmodified Rastall teleparallel gravity. It is the first time that dark energycelestial phenomena have been explored in this modified gravitational theory.Employing the torsion-based functions, $f(T)$ and $h(T)$, we analyzed theireffects in a spherically symmetric spacetime chosen as the interior geometry,while using the Schwarzschild geometry as an outer spacetime. In this study, weexplored various dark energy stellar properties, including dark energy pressurecomponents, energy conditions, and equation of state components. Our findingsreveal that the observed negative behavior of these stellar properties servedas compelling evidence, validating the presence of dark energy in stellarconfigurations. Detailed investigations of the energy conditions, pressureprofiles, sound speeds, TOV equation, adiabatic index, gradients, massfunction, compactness, and redshift function forecasts a comprehensiveassessment, affirming the acceptability and realism of the investigated stellarconfiguration.

Dark Energy Compact Stars in Extended Teleparallel Gravity