https://doi.org/10.1140/epjc/s10052-024-13123-8
Regular Article - Experimental Physics
First measurement of Gallium Arsenide as a low-temperature calorimeter
1
INFN-Laboratori Nazionali del Gran Sasso, Assergi, 67100, L’Aquila, Italy
2
Dipartimento di Scienze Fisiche e Chimiche, Università degli Studi dell’Aquila, 67100, L’Aquila, Italy
3
Gran Sasso Science Institute, 67100, L’Aquila, Italy
4
INFN and Università degli studi di Milano-Bicocca, 20126, Milan, Italy
5
Istituto Nazionale di Ricerca Metrologica Torino, 10135, Turin, Italy
6
CNR-SPIN, Università degli studi dell’Aquila, 67100, L’Aquila, Italy
a
dounia.helis@lngs.infn.it
b
andrea.melchiorre@lngs.infn.it
c
andrei.puiu@lngs.infn.it
Received:
11
April
2024
Accepted:
11
July
2024
Published online:
27
July
2024
In the quest for direct dark matter detection, innovative approaches to lower the detection threshold and explore the sub-GeV mass range, have gained high relevance in the last decade. This study presents the pioneering use of Gallium Arsenide (GaAs) as a low-temperature calorimeter for probing dark matter-electron interactions within the DAREDEVIL (DARk-mattEr DEVIces for Low energy detection) project. Our experimental setup features a GaAs crystal at an ultralow temperature of 15 mK, coupled with a Neutron Transmutation Doped Germanium (NTD-Ge) thermal sensor for precise energy estimation. This configuration is the first step towards detecting single electrons scattered by dark matter particles within the GaAs crystal, to improve the sensitivity to low-mass dark matter candidates significantly. Taking advantage of the production of optical phonons in polar materials such as GaAs gives the possibility to study the scattering of sub-MeV dark matter. This paper presents a detailed analysis of the detector’s response, using a calibration spectrum using 
particles and X-ray events. While the results do not meet the ambitious eV scale threshold yet, they establish a solid benchmark for assessing the detector’s current performance and sensitivity. This work not only highlights the detector’s potential but also sets the stage for future enhancements aimed at achieving the eV threshold, underscoring the promising direction of this detector technology. These findings demonstrate the feasibility of using GaAs as a cryogenic calorimeter and hence open new avenues for investigating the elusive nature of dark matter through innovative direct detection techniques.
© The Author(s) 2024
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Funded by SCOAP3.
