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Title: Direct detection of sub-GeV dark matter with scintillating targets

Journal Article · · Physical Review D
 [1];  [2];  [2];  [3];  [2]
  1. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
  2. Stony Brook Univ., NY (United States). C.N. Yang Inst. for Theoretical Physics
  3. Stony Brook Univ., NY (United States). Dept. of Physics and Astronomy

We suggest a novel experimental concept for detecting MeV-to-GeV-mass dark matter, in which the dark matter scatters off electrons in a scintillating target and produces a signal of one or a few photons. New large-area photodetectors are needed to measure the photon signal with negligible dark counts, which could be constructed from transition edge sensor (TES) or microwave kinetic inductance detector (MKID) technology. Alternatively, detecting two photons in coincidence may allow the use of conventional photodetectors like photomultiplier tubes. Here we describe why scintillators may have distinct advantages over other experiments searching for a low ionization signal from sub-GeV dark matter, as there are fewer potential sources of spurious backgrounds. 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), which in principle allows it to probe dark matter masses 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 dark matter down to MeV masses.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC); Sloan Foundation; National Science Foundation (NSF)
Grant/Contract Number:
AC02-05CH11231; FG02-09ER16052; PHY1316617; SC0008061
OSTI ID:
1430683
Alternate ID(s):
OSTI ID: 1373327
Journal Information:
Physical Review D, Vol. 96, Issue 1; ISSN 2470-0010
Publisher:
American Physical Society (APS)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 108 works
Citation information provided by
Web of Science

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Cited By (18)

Cryogenic scintillation properties of n -type GaAs for the direct detection of MeV/c 2 dark matter journal March 2018
Direct detection of strongly interacting sub-GeV dark matter via electron recoils journal September 2019
Refined bounds on MeV-scale thermal dark sectors from BBN and the CMB journal January 2020
New constraints and discovery potential of sub-GeV dark matter with xenon detectors journal August 2017
Direct detection of axion-like particles in Bismuth-based topological insulators journal August 2018
Directly Detecting Sub-GeV Dark Matter with Electrons from Nuclear Scattering text January 2018
Twin Higgs model with strongly interacting massive particle dark matter text January 2018
Searching for light WIMPS in view of neutron decay to dark matter journal August 2019
Phenomenology of self-interacting dark matter in a matter-dominated universe journal January 2019
New constraints and discovery potential of sub-GeV dark matter with xenon detectors text January 2017
New Constraints and Prospects for sub-GeV Dark Matter Scattering off Electrons in Xenon text January 2017
Resonant absorption of bosonic dark matter in molecules text January 2017
Light Dark Matter: Models and Constraints text January 2017
Phenomenology of Self-Interacting Dark Matter in a Matter-Dominated Universe text January 2018
Directional Detection of Light Dark Matter with Polar Materials text January 2018
Making dark matter out of light: freeze-in from plasma effects text January 2019
On the relation between Migdal effect and dark matter-electron scattering in isolated atoms and semiconductors text January 2019
Refined Bounds on MeV-scale Thermal Dark Sectors from BBN and the CMB text January 2019

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