Published 2024 | Version v1
Journal article

Light dark matter search using a diamond cryogenic detector

  • 1. Max-Planck-Institut für Physik, München (Germany)
  • 2. Atominstitut, Technische Universität Wien (Austria)
  • 3. Institut für Hochenergiephysik, Österreichische Akademie der Wissenschaften, Wien (Austria)
  • 4. INFN, Laboratori Nazionali del Gran Sasso, Assergi (Italy)

Description

Diamond operated as a cryogenic calorimeter is an excellent target for direct detection of low-mass dark matter candidates. Following the realization of the first low-threshold cryogenic detector that uses diamond as absorber for astroparticle physics applications, we now present the resulting exclusion limits on the elastic spin-independent interaction cross-section of dark matter with diamond. We measured two 0.175 g CVD (Chemical Vapor Deposition) diamond samples, each instrumented with a Transition Edge Sensor made of Tungsten (W-TES). Thanks to the energy threshold of just 16.8 eV of one of the two detectors, we set exclusion limits on the elastic spin-independent interaction of dark matter particles with carbon nuclei down to dark matter masses as low as 0.122 GeV/c2. This work shows the scientific potential of cryogenic detectors made from diamond and lays the foundation for the use of this material as target for direct detection dark matter experiments.

Availability note (English)

Available from: http://dx.doi.org/10.1140/epjc/s10052-024-12647-3

Additional details

Publishing Information

Journal Title
European Physical Journal. C, Particles and Fields (Online)
Journal Volume
84
Journal Issue
3
Journal Page Range
vp.
ISSN
1434-6052
CODEN
EPCFFB

INIS

Country of Publication
Germany
Country of Input or Organization
Germany
INIS RN
56000300
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Descriptors DEI
CHEMICAL VAPOR DEPOSITION; CRYOGENICS; DIAMONDS; NONLUMINOUS MATTER
Descriptors DEC
CARBON; CHEMICAL COATING; DEPOSITION; ELEMENTS; MATTER; MINERALS; NONMETALS; SURFACE COATING

Optional Information

Notes
AID: 324
Collaborations
CRESST Collaboration