2019
DOI: 10.1007/jhep11(2019)140
|View full text |Cite
|
Sign up to set email alerts
|

Fast-rolling relaxion

Abstract: We discuss new mechanisms to stop the relaxion field during inflation. They can be realized in a generic model, including the original model but in a quite different parameter region. We consider a fast-rolling relaxion field, which can go over the bumps created by QCD-like dynamics. Then, in one of the mechanisms, we stop it with a parametric resonance of the Higgs field. The mechanisms are free from a super-Planckian field excursion or a gigantic number of e-folds of inflation. The relaxion has a mass around… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1
1

Citation Types

0
11
0

Year Published

2020
2020
2022
2022

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 18 publications
(11 citation statements)
references
References 78 publications
0
11
0
Order By: Relevance
“…Finite temperature effects are used in [6]. In [7] the necessary friction is provided by parametric resonance of the Higgs zero mode. In [8] a potential instability is introduced to stop the field.…”
Section: Introductionmentioning
confidence: 99%
“…Finite temperature effects are used in [6]. In [7] the necessary friction is provided by parametric resonance of the Higgs zero mode. In [8] a potential instability is introduced to stop the field.…”
Section: Introductionmentioning
confidence: 99%
“…The appearance of the barriers as the Higgs mass scans through the origin and triggers a non-zero EW vacuum expectation value (VEV) acts as the trigger that stops the relaxion field, with Hubble friction and a small, technically natural slope ensuring the correct EW VEV is not overshot. Issues with the original model were addressed in [25] and alternative stopping mechanisms using, e.g., friction from the tachyonic production of EW gauge bosons [26][27][28][29], 1 friction from parametric resonance due to the Higgs zero mode [31], potential instabilities [32], fermion production [33], and dark photon production [34,35] have also been considered. The general idea of solving the hierarchy problem by means of the cosmological evolution has been the subject of a number of recent studies, see e.g.…”
Section: Jhep12(2021)037mentioning
confidence: 99%
“…A similar hierarchy is required for different models that exploit different mechanisms to dissipate away relaxion kinetic energy (124)(125)(126)(127)(128)(129)(130). Here we consider two examples in which dissipation is dominated by bosonic particle production (125,130).…”
Section: Coupling Hierarchy For the Relaxionmentioning
confidence: 99%