pith. sign in

arxiv: 1807.01791 · v1 · pith:Z6PTBW2Nnew · submitted 2018-07-04 · 🌀 gr-qc · astro-ph.CO· hep-th

The Case for Nonlocal Modifications of Gravity

classification 🌀 gr-qc astro-ph.COhep-th
keywords darkgravitymodificationsenergygeneralinflationmattermodels
0
0 comments X
read the original abstract

The huge amounts of undetected and exotic dark matter and dark energy needed to make general relativity work on large scales argue that we should investigate modifications of gravity. The only stable, metric-based and invariant alternative to general relativity is $f(R)$ models. These models can explain primordial inflation, but they cannot dispense with either dark matter or dark energy. I advocate nonlocal modifications of gravity, not as new fundamental theories but rather as the gravitational vacuum polarization engendered by infrared quanta produced during primordial inflation. I also discuss some of the many objections which have been raised to this idea.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Inverse-Scattering Reconstruction of Inflation from Scalar and Tensor Primordial Spectra

    astro-ph.CO 2026-06 unverdicted novelty 7.0

    An inverse-scattering method reconstructs inflationary potentials from primordial power spectra using Jost functions derived from the Mukhanov-Sasaki equation.