paper

The gravitational constant and the cosmic microwave background

arXiv:2610.22128

Abstract

The CMB constrains the gravitational constant at recombination to a few percent of its laboratory value, but the effect of on recombination itself is usually absorbed into a global fit rather than made explicit. We return to the semi-analytic description of the acoustic spectrum to ask how the acoustic scale , the equality scale and the damping scale respond to a variation of during recombination, and where enters the residual ionization of the dark ages. We use a modified version of CLASS in which is varied through , scanning at fixed physical densities and CMB temperature, with helium recomputed for each model. Analytic rate arguments are confronted with the numerical ionization histories, the visibility function, the Hu & White damping integral and the TT spectra. While and are nearly independent of , non-equilibrium recombination gives . The dependence exists only above a critical value of , set by fundamental and cosmological parameters, a factor of 49 below . The dark-ages optical depth varies by only 16% for multiplied by 64, a negligible channel. Because enters only through the expansion rate, the imprint comes entirely from out-of-equilibrium recombination, and the competition between the atomic rates and the expansion is governed by one dimensionless combination, , with the mean mass of matter per photon. Each scale is the distance to last scattering divided by a length imprinted before it, so a late-time change of gravity rescales all three alike. The ratio therefore isolates at recombination and, up to lensing and screening, compares it directly with the laboratory value.

Submitted to A&A