The $U(1)_{L_μ-L_τ}$ breaking phase transition, muon $g-2$, dark matter, collider and gravitational wave

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Auteurs principaux: Wang, Jie, Ma, Jinghong, Gao, Jing, Han, Xiao-Fang, Wang, Lei
Format: Preprint
Publié: 2023
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author Wang, Jie
Ma, Jinghong
Gao, Jing
Han, Xiao-Fang
Wang, Lei
author_facet Wang, Jie
Ma, Jinghong
Gao, Jing
Han, Xiao-Fang
Wang, Lei
contents Combining the dark matter and muon $g-2$ anomaly, we study the $U(1)_{L_μ-L_τ}$ breaking phase transition, gravitational wave spectra, and the direct detection at the LHC in an extra $U(1)_{L_μ-L_τ}$ gauge symmetry extension of the standard model. The new fields includes vector-like leptons ($E_1,~ E_2,~ N$), $U(1)_{L_μ-L_τ}$ breaking scalar $S$ and gauge boson $Z'$, as well as the dark matter candidate $X_I$ and its heavy partner $X_R$. A joint explanation of the dark matter relic density and muon $g-2$ anomaly excludes the region where both $min(m_{E_1},m_{E_2},m_N,m_{X_R})$ and $min(m_{Z'},m_S)$ are much larger than $m_{X_I}$. In the parameter space accommodating the DM relic density and muon $g-2$ anomaly, the model can achieve a first order $U(1)_{L_μ-L_τ}$ breaking phase transition, whose strength is sensitive to the parameters of Higgs potential. The corresponding gravitational wave spectra can reach the sensitivity of U-DECIGO. In addition, the direct searches at the LHC impose stringent bound on the mass spectra of the vector-like leptons and dark matter.
format Preprint
id arxiv_https___arxiv_org_abs_2309_09210
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle The $U(1)_{L_μ-L_τ}$ breaking phase transition, muon $g-2$, dark matter, collider and gravitational wave
Wang, Jie
Ma, Jinghong
Gao, Jing
Han, Xiao-Fang
Wang, Lei
High Energy Physics - Phenomenology
Combining the dark matter and muon $g-2$ anomaly, we study the $U(1)_{L_μ-L_τ}$ breaking phase transition, gravitational wave spectra, and the direct detection at the LHC in an extra $U(1)_{L_μ-L_τ}$ gauge symmetry extension of the standard model. The new fields includes vector-like leptons ($E_1,~ E_2,~ N$), $U(1)_{L_μ-L_τ}$ breaking scalar $S$ and gauge boson $Z'$, as well as the dark matter candidate $X_I$ and its heavy partner $X_R$. A joint explanation of the dark matter relic density and muon $g-2$ anomaly excludes the region where both $min(m_{E_1},m_{E_2},m_N,m_{X_R})$ and $min(m_{Z'},m_S)$ are much larger than $m_{X_I}$. In the parameter space accommodating the DM relic density and muon $g-2$ anomaly, the model can achieve a first order $U(1)_{L_μ-L_τ}$ breaking phase transition, whose strength is sensitive to the parameters of Higgs potential. The corresponding gravitational wave spectra can reach the sensitivity of U-DECIGO. In addition, the direct searches at the LHC impose stringent bound on the mass spectra of the vector-like leptons and dark matter.
title The $U(1)_{L_μ-L_τ}$ breaking phase transition, muon $g-2$, dark matter, collider and gravitational wave
topic High Energy Physics - Phenomenology
url https://arxiv.org/abs/2309.09210