Published April 28, 2023
| Version v1
Journal article
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First Constraints from DAMIC-M on Sub-GeV Dark-Matter Particles Interacting with Electrons
Creators
- Arnquist, I.1
- Avalos, N.2
- Baxter, D.3
- Bertou, X.2
- Castelló-Mor, N.4
- Chavarria, A. E.5
- Cuevas-Zepeda, J.3
- Cortabitarte Gutiérrez, J.4
- Duarte-Campderros, J.4
- Dastgheibi-Fard, A.6
- Deligny, O.7
- De Dominicis, C.8
- Estrada, E.9
- Gadola, N.10
- Gaïor, R.8
- Hossbach, T.1
- Iddir, L.8
- Khalil, L.8
- Kilminster, B.10
- Lantero-Barreda, A.4
- Matalon, A.3
- Munagavalasa, S.3
- Norcini, D.3
- Paul, S.3
- Privitera, P.3
- Ramanathan, K.3
- Smida, R.3
- Thomas, R.3
- Yajur, R.3
- 1. Pacific Northwest National Laboratory
- 2. Universidad Nacional de Cuyo
- 3. University of Chicago
- 4. Universidad de Cantabria
- 5. University of Washington
- 6. Université Grenoble-Alpes
- 7. Université Paris-Saclay
- 8. Sorbonne Université
- 9. Comisión Nacional de Energía Atómica
- 10. Universität Zürich Physik Institut
Description
We report constraints on sub-GeV dark matter particles interacting with electrons from the first underground operation of DAMIC-M detectors. The search is performed with an integrated exposure of 85.23 g days, and exploits the subelectron charge resolution and low level of dark current of DAMIC-M charge-coupled devices (CCDs). Dark-matter-induced ionization signals above the detector dark current are searched for in CCD pixels with charge up to $7e^−$. With this dataset we place limits on dark matter particles of mass between 0.53 and $1000 MeV/c^2$, excluding unexplored regions of parameter space in the mass ranges $[1.6,1000] MeV/c^2$ and $[1.5,15.1] MeV/c^2$ for ultralight and heavy mediator interactions, respectively.
Notes
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PhysRevLett.130.171003.pdf
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Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.130.171003
- Other
- oai:uchicago.tind.io:14251
Funding
- European Research Council
- 788137
- National Science Foundation
- PHY-1812654
- National Science Foundation
- PHY-2110585
- University of Chicago
- MCIN/ AEI /10.13039/501100011033
- PID2019–109829GB-I00
- Agencia Nacional de Promoción Científica y Tecnológica
- PICT-2018-03069
- Swiss National Science Foundation
- U.S. Department of Energy
- DE-AC02-05CH11231