Artian A2 Endurance and the Einstein-Field Infrared Theorem

From finite endurance currents to Einstein-field dynamics This paper asks a sharply typed question: when a finite completed-address ledger is read through an infrared metric camera, which field equation is forced, and which source receipts must be supplied before its coefficient is universal? The A2 source begins with the dimensionless Artian mass count and its endurance rate, \[ B=\frac{M}{m_A}, \qquad \dot N_{\rm sink}=\frac{B}{\tilde t_A}. \] The ruler package fixes the structural gravity conversion, while the physical endpoint is kept as an explicitly typed family: \[ \boxed{ G_A=\frac{\tilde\ell_A^{2}c^3}{\hbar}, \qquad G_{\rm end}=\chi_g G_A, \qquad 0