Signatures of afterglows from light dark matter boosted by supernova neutrinos in current and future large underground detectors
arxiv(2023)
摘要
Supernova neutrino boosted dark matter (SNν BDM) and its afterglow effect
have been shown to be a promising signature for beyond Standard Model (bSM)
physics. The time-evolution feature of SNν BDM allows for
direct inference of DM mass m_χ, and results in significant background
suppression with improving sensitivity. This paper extends the earlier study
and provides a general framework for computing the SNν BDM fluxes for a
supernova that occurs at any location in our galaxy. A bSM
U(1)_L_μ-L_τ model with its gauge boson coupling to both DM and the
second and third generation of leptons is considered, which allows for both
DM-ν and DM-e interactions. Detailed analysis of the temporal profile,
angular distribution, and energy spectrum of the SNν BDM are performed.
Unique signatures in SNν BDM allowing extraction of m_χ and detail
features that contain information of the underlying interaction type are
discussed. Expected sensitivities on the above new physics model from
Super-Kamiokande, Hyper-Kamiokande, and DUNE detections of BDM events induced
by the next galactic SN are derived and compared with the existing bounds.
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