English

A Dynamical Weak Scale from Inflation

High Energy Physics - Phenomenology 2017-09-20 v2 Cosmology and Nongalactic Astrophysics

Abstract

Dynamical scanning of the Higgs mass by an axion-like particle during inflation may provide a cosmological component to explaining part of the hierarchy problem. We propose a novel interplay of this cosmological relaxation mechanism with inflation, whereby the backreaction of the Higgs vacuum expectation value near the weak scale causes inflation to end. As Hubble drops, the relaxion's dissipative friction increases relative to Hubble and slows it down enough to be trapped by the barriers of its periodic potential. Such a scenario raises the natural cut-off of the theory up to 1010\sim 10^{10} GeV, while maintaining a minimal relaxion sector without having to introduce additional scanning scalars or new physics coincidentally close to the weak scale.

Keywords

Cite

@article{arxiv.1701.09167,
  title  = {A Dynamical Weak Scale from Inflation},
  author = {Tevong You},
  journal= {arXiv preprint arXiv:1701.09167},
  year   = {2017}
}

Comments

20 pages, 2 figures. v2: typos and discussion in subsection 3.2 corrected, version accepted for publication in JCAP

R2 v1 2026-06-22T18:05:39.107Z