Direct Detection of sub-GeV Dark Matter with Scintillating Targets

TL;DR

This paper proposes a novel scintillation-based detection method for sub-GeV dark matter, utilizing low-noise photodetectors to detect photon emissions from electron excitations in crystals, potentially enabling detection of dark matter as light as 0.5 MeV.

Contribution

It introduces a new detection approach using scintillating targets and calculates expected scattering rates, highlighting gallium arsenide's advantage for low-mass dark matter detection.

Findings

GaAs can probe dark matter masses down to ~0.5 MeV.

Scintillating targets may offer technological advantages over existing methods.

The approach provides a complementary and potentially more sensitive detection pathway.

Abstract

We describe a novel search for MeV-to-GeV-mass dark matter, in which the dark matter scatters off electrons in a scintillating target. The excitation and subsequent de-excitation of the electron produces one or more photons, which could be detected with an array of cryogenic low-noise photodetectors, such as transition edge sensors (TES) or microwave kinetic inductance devices (MKID). Scintillators may have distinct advantages over other experiments searching for a low ionization signal from sub-GeV DM. First, the detection of one or a few photons may be technologically easier. Second, since no electric field is required to detect the photons, there may be far fewer dark counts mimicking a DM signal. We discuss various target choices, but focus on calculating the expected dark matter-electron scattering rates in three scintillating crystals, sodium iodide (NaI), cesium iodide (CsI), and gallium arsenide (GaAs). Among these, GaAs has the lowest band gap (1.52 eV) compared to NaI (5.9 eV) or CsI (6.4 eV), allowing it to probe dark matter masses possibly as low as ~0.5 MeV, compared to ~1.5 MeV with NaI or CsI. We compare these scattering rates with those expected in silicon (Si) and germanium (Ge). The proposed experimental concept presents an important complementary path to existing efforts, and its potential advantages may make it the most sensitive direct-detection probe of DM down to MeV masses.