English

Solving the Standard Model Problems in Softened Gravity

High Energy Physics - Phenomenology 2017-06-23 v2 General Relativity and Quantum Cosmology

Abstract

The Higgs naturalness problem is solved if the growth of Einstein's gravitational interaction is softened at an energy 1011 \lesssim 10^{11}\,GeV (softened gravity). We work here within an explicit realization where the Einstein-Hilbert Lagrangian is extended to include terms quadratic in the curvature and a non-minimal coupling with the Higgs. We show that this solution is preserved by adding three right-handed neutrinos with masses below the electroweak scale, accounting for neutrino oscillations, dark matter and the baryon asymmetry. The smallness of the right-handed neutrino masses (compared to the Planck scale) and the QCD θ\theta-term are also shown to be natural. We prove that a possible gravitational source of CP violation cannot spoil the model, thanks to the presence of right-handed neutrinos. Inflation is approximately described by the Starobinsky model in this context, and can occur even if we live in a metastable vacuum.

Keywords

Cite

@article{arxiv.1608.01194,
  title  = {Solving the Standard Model Problems in Softened Gravity},
  author = {Alberto Salvio},
  journal= {arXiv preprint arXiv:1608.01194},
  year   = {2017}
}

Comments

21 pages, 1 figure; v2: extended version required by Phys.Rev.D

R2 v1 2026-06-22T15:11:09.198Z