QMU Gravitational Field Theory V: Rotational Closure Dynamics, Closure Stress-Energy, and Binary-System Energy Transport

This paper develops the rotational sector of QMU Gravitational Field Theory and introduces the first closure stress-energy ledger. The previous papers established the scalar closure sector through propagation-density curvature, closure-flow conservation, closure coupling constants, closure saturation, and post-Newtonian recovery. The present work extends that scalar framework by introducing an independent rotational closure potential and the corresponding rotational closure field. The paper derives coupled scalar-rotational closure equations, rotational closure waves, closure energy density, closure momentum density, and a closure-energy flux analogous to a gravitational Poynting vector. These quantities provide the weak-field stress-energy structure required for binary-system energy transport and gravitational radiation. The resulting framework is applied to compact binary systems, where the total closure luminosity is related to orbital decay. The standard Peters-Mathews luminosity is identified as the weak-field calibration condition for the combined scalar and rotational closure flux. The paper also outlines the observational roles of binary pulsars, interferometric gravitational-wave detectors, and RMFD-type detectors. It concludes that efficient gravitational radiation transport requires coupled scalar and rotational closure structure, while strong-field extensions involving frame dragging, rotating horizons, ergoregions, and Kerr-like closure geometry remain for subsequent work.