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/c. 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/s10052-024-12647-3Additional details
Identifiers
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