This work presents a structural interpretation of the Baryonic Tully–Fisher Relation (BTFR) using the SPARC sample of 175 disk galaxies. We show that: • The BTFR slope emerges from Newtonian disk equilibrium combined with empirical size–mass scaling (Rd ∝ Mb⁰. 5). • The intrinsic scatter floor (~0. 09 dex) arises from structural dispersion in disk scale length. • A mass-independent acceleration scale (~10^-10 m s^-2) appears as a stability fixed point under Toomre Q ≈ 1. • Structural regulation is strongest in low-mass galaxies. The results suggest that the BTFR and galactic acceleration scale reflect structural self-organization in rotating stellar disks rather than modified gravity.
Alim ul haq khan (Mon,) studied this question.