Static Spherically Symmetric Chaplygin and Polytropic Fluid Solutions in Teleparallel F(T) Gravity

We investigate static, spherically symmetric (SS) spacetimes in covariant teleparallel $F(T)$ gravity sourced by nonlinear Chaplygin and polytropic fluids. Using the covariant coframe/spin-connection (CSC) formalism, we derive the corresponding field equations and conservation laws governing admissible matter distributions and nonlinear torsion sectors. A general reconstruction procedure is developed, allowing the systematic determination of teleparallel $F(T)$ models for arbitrary coframe ans\"atze and fluid equations of state. Focusing on power-law configurations, we obtain several classes of reconstructed solution branches, including constant-radius, compact-object-like, black-hole-like (BH-like), and wormhole-like (WH-like) branches. The Chaplygin sector naturally generates effective dark-energy and exotic-matter regimes capable of supporting traversable wormhole geometries, while the polytropic sector provides physically relevant models for stellar interiors and compact objects. We discuss the associated horizon and throat structures, torsion singularities, energy conditions, and stability properties of the reconstructed branches. The resulting geometries are organized within the Coley--Landry invariant classification framework, highlighting the role of nonlinear torsion corrections in shaping the solution space. Overall, this work provides a unified covariant framework for the construction and interpretation of compact objects, effective cosmological sectors, and regular-core strong-field geometries beyond General Relativity.