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1/R gravity and Scalar-Tensor Gravity

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

3 Pith papers citing it
abstract

We point out that extended gravity theories, the Lagrangian of which is an arbitrary function of scalar curvature $R$, are equivalent to a class of the scalar tensor theories of gravity. The corresponding gravity theory is $\omega=0$ Brans-Dicke gravity with a potential for the Brans-Dicke scalar field, which is not compatible with solar system experiments if the field is very light: the case when such modifications are important recently.

representative citing papers

Evolving Dark Energy Is Vacuum Energy After All

astro-ph.CO · 2026-06-18 · conditional · novelty 5.0

A QCD-vacuum dark-energy model with a two-parameter switch reproduces the DESI-preferred late-time expansion and is mildly favoured over ΛCDM by Bayesian evidence (lnB≈2.7).

Modified Gravity and Cosmology

astro-ph.CO · 2011-06-13 · unverdicted · novelty 2.0

A comprehensive review of modified gravity theories and their cosmological consequences, including a parameterized post-Friedmannian formalism for constraining deviations from General Relativity.

citing papers explorer

Showing 3 of 3 citing papers.

  • Ordering-Independent Wheeler-DeWitt Equation for Flat Minisuperspace Models hep-th · 2025-12-29 · unverdicted · none · ref 34 · internal anchor

    Path-integral measures determine operator orderings for the Wheeler-DeWitt equation in flat minisuperspace models, with all consistent choices yielding identical physical observables via field redefinition Jacobians.

  • Evolving Dark Energy Is Vacuum Energy After All astro-ph.CO · 2026-06-18 · conditional · none · ref 72 · internal anchor

    A QCD-vacuum dark-energy model with a two-parameter switch reproduces the DESI-preferred late-time expansion and is mildly favoured over ΛCDM by Bayesian evidence (lnB≈2.7).

  • Modified Gravity and Cosmology astro-ph.CO · 2011-06-13 · unverdicted · none · ref 292

    A comprehensive review of modified gravity theories and their cosmological consequences, including a parameterized post-Friedmannian formalism for constraining deviations from General Relativity.