paper

Cosmographic Reconstruction of the Quintessence Potential in Scalar-Tensor Gravity

arXiv:2608.14183

Abstract

We generalise the cosmographic reconstruction programme of Chakraborty, Dunsby & Scherrer to scalar-tensor gravity. Working in the Jordan frame with a general non-minimal coupling , we derive exact closed-form expressions for the potential slope , the coupling slope , and their curvature parameters and in terms of the cosmographic parameters , the Planck-mass running and its derivatives. We express and its derivatives in terms of a set of coefficients describing the time variation of the gravitational constant , casting all four quantities in fully observable form. We then evaluate the reconstruction against current data, including DESI~DR2 baryon acoustic oscillation measurements and Lunar Laser Ranging constraints on , propagating the cosmographic uncertainties through to the reconstructed potential. All expressions reduce analytically to those of Chakraborty, Dunsby & Scherrer in the minimally-coupled limit, which we verify symbolically. We find that the potential slope is recovered at the few-tenths level while the curvature is essentially unconstrained. We further show that the positivity of the scalar kinetic term is equivalent to , so that the region of cosmographic parameter space closed to minimally-coupled quintessence is exactly the phantom region, and that the non-minimal coupling reopens it through a single coefficient of the gravitational tower. Because Lunar Laser Ranging forces while the reconstruction is sensitive to , the framework presupposes that is passing through zero at the present epoch, as expected on the Damour--Nordtvedt least-coupling attractor.

25 pages, 5 figures. The numerical analysis files used for the reproduction of the figures can be found at: https://github.com/leandros11/st-reconstruction