Light Dark Matter Detection with Hydrogen-rich Crystals and Low-Tc TES Detectors
G. Wang, C. L. Chang, M. Lisovenko, V. Novosad, V. G. Yefremenko and, J. Zhang

TL;DR
This paper explores hydrogen-rich crystals and low-temperature TES detectors for direct detection of sub-GeV dark matter, focusing on their signal mechanisms and potential to probe unexplored parameter space.
Contribution
It introduces hydrogen-rich crystals as detection media and discusses the development of ultra-sensitive low-Tc TES detectors for light dark matter searches.
Findings
Hydrogen-rich crystals emit infrared photons and phonons under excitation.
Low-Tc TES detectors can measure single photons and phonons with high sensitivity.
The approach can explore large uncharted parameter space of light DM.
Abstract
Direct detection of nuclear scatterings of sub-GeV Dark Matter (DM) particles favors low-Z nuclei. Hydrogen nucleus, which has a single proton, provides the best kinematic match to a light dark matter particle. The characteristic nuclear recoil energy is boosted by a factor of a few tens from those for larger nuclei used in traditional Weakly Interacting Massive Particle (WIMP) searches. Furthermore, hydrogen is optimal not only for spin-independent nuclear scatterings of sub-GeV DM, but also for spin-dependent nuclear scatterings, where large parameter space remains unconstrained. In this paper, we first introduce hydrogen-rich crystals, which include water ice, acetylene, anthracene, trans-stilbene, and naphthalene. These crystals emit two classes of signals under kinetic excitations. One class of the signals is infrared photons, which are from optically active fundamental vibrational…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Atomic and Subatomic Physics Research · Chemical and Physical Properties of Materials
