2020
DOI: 10.1103/physrevd.101.035029
|View full text |Cite
|
Sign up to set email alerts
|

Dynamical solution to the axion domain wall problem

Abstract: The domain wall problem and the isocurvature problem restrict possible combinations of axion models and inflation models. In this paper, we considered a new mechanism which solves those problems by dynamics of multiple scalar fields during/after inflation. The mechanism makes axion models with a non-trivial domain wall number compatible with inflation models with a large Hubble parameter, H I 10 7-8 GeV. The mechanism also avoids the isocurvature problem. This mechanism increases the freedom of choice of combi… Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1

Citation Types

0
4
0

Year Published

2020
2020
2024
2024

Publication Types

Select...
5
1

Relationship

1
5

Authors

Journals

citations
Cited by 7 publications
(4 citation statements)
references
References 68 publications
0
4
0
Order By: Relevance
“…This phenomenon, known as "clash-of-symmetries" [21][22][23], occurs when the unbroken symmetry subgroups H and H ′ on the two regions outside the wall are embedded differently in the broken symmetry group G. The symmetry group inside the wall will be the intersection H ∩ H ′ which can be smaller than the group H. Such mechanism was used in [21] in order to provide for a way to break symmetries using domain walls in the scenario where our 3+1-dimensional universe exists as a domain wall brane in a 4+1-dimensional spacetime with an action invariant under E 6 symmetry. The spontaneous breaking of E 6 symmetry to differently embedded unbroken SO(10) × U(1) subgroups H and H ′ outside the brane leads the unbroken symmetry group inside the domain wall H ∩ H ′ to be a smaller group containing SU (5). In our model we will show that, due to this mechanism, the symmetry group of electromagnetism can be broken inside the domain wall.…”
Section: Jhep04(2024)101mentioning
confidence: 73%
See 1 more Smart Citation
“…This phenomenon, known as "clash-of-symmetries" [21][22][23], occurs when the unbroken symmetry subgroups H and H ′ on the two regions outside the wall are embedded differently in the broken symmetry group G. The symmetry group inside the wall will be the intersection H ∩ H ′ which can be smaller than the group H. Such mechanism was used in [21] in order to provide for a way to break symmetries using domain walls in the scenario where our 3+1-dimensional universe exists as a domain wall brane in a 4+1-dimensional spacetime with an action invariant under E 6 symmetry. The spontaneous breaking of E 6 symmetry to differently embedded unbroken SO(10) × U(1) subgroups H and H ′ outside the brane leads the unbroken symmetry group inside the domain wall H ∩ H ′ to be a smaller group containing SU (5). In our model we will show that, due to this mechanism, the symmetry group of electromagnetism can be broken inside the domain wall.…”
Section: Jhep04(2024)101mentioning
confidence: 73%
“…Extensions of the SM scalar sector may lead to the existence of topological defects such as cosmic strings and domain walls. Such defects appear for example in axion models [4][5][6][7][8], supersymmetric models in the context of the spontaneous breaking of the R symmetry [9] and the Z 3 discrete symmetry in the NMSSM [10,11], discrete flavor symmetries [12,13] as well as in the Two-Higgs-Doublet model (2HDM) [14][15][16][17]. In this work we investigate the domain walls solutions in the 2HDM, where the SM scalar sector is extended with a second Higgs doublet of SU(2) L and charged under U Y (1).…”
Section: Introductionmentioning
confidence: 99%
“…Here, H denotes the Hubble expansion rate. This behavior of the scalar field is called the scaling solution [62][63][64]. We focus on this scaling solution with n ¼ 4 as an example in the rest of this section.…”
Section: Sub-kev Fermion Dm From Decay Of a Scalar Field Coherent mentioning
confidence: 99%
“…Nevertheless, ALP DW could exist up to the modern epoch in the post-inflation scenario since ALP fields are not restricted by the QCD phenomology [31][32][33][34]. If they indeed exist, such ALP DW dark matter would have a highly nonuniform local density.…”
Section: Introductionmentioning
confidence: 99%