A Combined Dark-Sector Density Budget for the Limit Frame Against Planck Values

Individually, each dark-sector ingredient of the frame can be tuned or bounded; together they must sum to the observed budget. This paper assembles the budget explicitly. The cosmological-constant-like fifth-coordinate term is set to the observed dark-energy density, cold matter is taken at the Planck value, and the computed contributions of the spin correction, residual shear, and a sixth-power vacuum residue are added at their derived sizes. The total matches the Planck fractions within their uncertainties, but only because the additional ingredients are negligible; a variant in which the vacuum residue is given its sixth-power neutron value overshoots the total density and is excluded by the same budget. The exercise shows which ingredients are load-bearing and which are passengers. Headline values are: rho res6 kg m3 = 1.071e-18, rho res5 kg m3 = 1.391e+01, Omega DE residue only = 1.000e+00, deviation DE sigma residue only = 4.504e+01, spin plus shear kg m3 = 7.505e-112. This study is simulated and computed from stated assumptions; it is not a measurement.