pith. sign in

Post-Newtonian parameters gamma and beta of scalar-tensor gravity with a general potential

2 Pith papers cite this work. Polarity classification is still indexing.

2 Pith papers citing it
abstract

We calculate the PPN parameters gamma and beta for scalar-tensor gravity with a generic coupling function omega and scalar potential V in the Jordan conformal frame in the case of a static spherically symmetric source. Since the potential generally introduces a radial dependence to the effective gravitational constant as well as to gamma and beta, we discuss the issue of defining these PPN parameters and compare our expressions with previous calculations in simpler cases. We confront our results with current observational constraints on the values of gamma and beta and thus draw restrictions on the form of the functions omega and V around their asymptotic background values.

citation-role summary

background 1

citation-polarity summary

fields

gr-qc 2

years

2026 2

verdicts

UNVERDICTED 2

roles

background 1

polarities

background 1

representative citing papers

Parameterized Post-Newtonian Analysis of Quadratic Gravity and Solar System Constraints

gr-qc · 2026-01-09 · unverdicted · novelty 6.0

Quadratic gravity with Weyl-squared and Ricci-squared terms produces PPN parameters that equal their GR values except for exponentially decaying corrections, with gamma identically 1 when the two mode masses are equal, yielding solar-system lower bounds m_R, m_W greater than or equal to 23 per AU.

Post-Newtonian Constraints on Scalar-Tensor Gravity

gr-qc · 2026-04-17 · unverdicted · novelty 6.0

Unified post-Newtonian analysis reveals that Palatini scalar-tensor theories often face weaker Solar System bounds than metric versions due to stronger Yukawa suppression, with Palatini f(R) reproducing GR limits for point sources unlike metric f(R).

citing papers explorer

Showing 2 of 2 citing papers.

  • Parameterized Post-Newtonian Analysis of Quadratic Gravity and Solar System Constraints gr-qc · 2026-01-09 · unverdicted · none · ref 42 · internal anchor

    Quadratic gravity with Weyl-squared and Ricci-squared terms produces PPN parameters that equal their GR values except for exponentially decaying corrections, with gamma identically 1 when the two mode masses are equal, yielding solar-system lower bounds m_R, m_W greater than or equal to 23 per AU.

  • Post-Newtonian Constraints on Scalar-Tensor Gravity gr-qc · 2026-04-17 · unverdicted · none · ref 46

    Unified post-Newtonian analysis reveals that Palatini scalar-tensor theories often face weaker Solar System bounds than metric versions due to stronger Yukawa suppression, with Palatini f(R) reproducing GR limits for point sources unlike metric f(R).