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Xinqi Wei

Publications and source records attributed to Xinqi Wei.

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Searching for elusive dark Higgs boson in spin-1/2 inelastic dark matter models at Belle II

Spin-1/2 inelastic dark matter (DM) models are popular among sub-GeV to GeV thermal DM scenarios due to the dominant role of co-annihilation in determining the DM relic abundance. In these models, the dark Higgs boson plays a crucial role in generating the mass of the new gauge boson, the dark photon ($A'$), and in establishing the mass splitting between the excited ($χ_2$) and ground ($χ_1$) states of DM. In particular, the Compton scattering $χ_1 A' \rightarrow χ_2^* \rightarrow χ_1 A'$ and its $t$-channel crossed process, $χ_1 χ_1 \rightarrow A' A'$, remain unitary for high energy longitudunal dark photon, only if the contribution of the dark Higgs boson is included. However, experimental searches for the dark Higgs boson have received relatively little attention. In particular, when the dark Higgs boson mass exceeds twice that of the DM excited state, its decay signatures become semi-visible or invisible, making detection challenging with current light scalar search strategies. In this work, we explore the prospects for detecting the elusive dark Higgs boson in spin-1/2 inelastic DM models at Belle II via dark Higgs-strahlung and rare $B$ meson decay processes. Our analysis indicates that both the inclusive signature of two displaced dilepton vertices and the additional missing energy from dark Higgs boson decays serve as robust indicators of its presence. Furthermore, we assess the future potential for detecting the dark Higgs boson with the proposed far detector related to Belle II, GAZELLE.

hep-ph

Probing long-lived doubly charged scalar in the Georgi-Machacek model at the LHC and in far detectors

Searching for long-lived particles (LLPs) beyond the Standard Model (SM) is a promising direction in collider experiments. The Georgi-Machacek (GM) model extends the scalar sector in the SM by introducing various new scalar bosons. In this study, we focus on the parameter space that allows the light doubly charged scalar to become long-lived. This light doubly charged scalar is fermophobic and predominantly decays into a pair of on-shell or off-shell same-sign $W$ bosons. We investigate three types of signal signatures at the LHC: displaced vertices in the inner tracking detector, displaced showers in the muon system, and heavy stable charged particles. Additionally, we analyze the potential for detecting such doubly charged scalars in far detectors, including ANUBIS, MATHUSLA, FACET, FASER, CODEX-b, MoEDAL-MAPP and AL3X. By combining the LLP searches at the LHC and in far detectors, we project that the limits on the mixing angle, $θ_H$, (between the doublet and triplets) can cover most of the parameter space with $\sinθ_H\lesssim 10^{-3}$ for the mass range of long-lived doubly charged scalars between $50$ GeV to $180$ GeV, assuming the full integrated luminosity at the LHC and HL-LHC.

hep-ph

Exploring muonphilic ALPs at muon colliders

Axion-like particles (ALPs) are new particles that extend beyond the standard model (SM) and are highly motivated. When considering ALPs within an effective field theory framework, their couplings with SM particles can be studied independently. It is a daunting task to search for GeV-scale ALPs coupled to muons in collider experiments because their coupling is proportional to the muon mass. However, a recent study by Altmannshofer, Dror, and Gori (2022) highlighted the importance of a four-point interaction, $W$-$μ$-$ν_μ$-$a$, as well as interactions from the chiral anomaly which couplings are not dependent on the muon mass. These interactions provide a new opportunity to explore muonphilic ALPs ($μ$ALPs) at the GeV scale. We have explored various $μ$ALPs production channels at muon colliders with $μ$ALPs decaying into a pair of muons. Especially, we found a pair of neutrinos accompanied by a $μ$ALP is a most effective channel to search for $μ$ALPs in the electrowek violating (EWV) scenario. In contract, a photon plus a $μ$ALP becomes a better channel to search for $μ$ALPs in the electroweak preserving (EWP) scenario because there is no $W$-$μ$-$ν_μ$-$a$ interaction in this situation. Most importantly, we found that the future bounds for $μ$ALPs in EWV scenario are much stronger than the ones in EWP scenario and the existing bounds for exploring $μ$ALPs with $1$ GeV $\leq m_a\lesssim M_W$.

hep-ph