Published March 7, 2024
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Search for Daily Modulation of MeV Dark Matter Signals with DAMIC-M
Creators
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Arnquist, I.1
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Avalos, N.2
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Baxter, D.3
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Bertou, X.2
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Castelló-Mor, N.4
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Chavarria, A. E.5
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Cuevas-Zepeda, J.3
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Dastgheibi-Fard, A.6
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De Dominicis, C.7
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Deligny, O.8
- Duarte-Campderros, J.4
- Estrada, E.2
- Gadola, N.9
- Gaïor, R.7
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Hossbach, T.1
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Iddir, L.7
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Kavanagh, B. J.4
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Kilminster, B.9
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Lantero-Barreda, A.4
- Lawson, I.10
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Munagavalasa, S.3
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Norcini, D.3
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Paul, S.3
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Privitera, P.3
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Smida, R.3
- Yajur, R.3
- 1. Pacific Northwest National Laboratory
- 2. Comisión Nacional de Energía Atómica
- 3. University of Chicago
- 4. Universidad de Cantabria
- 5. University of Washington
- 6. Université Grenoble-Alpes
- 7. Sorbonne Université
- 8. Université Paris-Saclay
- 9. Universität Zürich Physik Institut
- 10. SNOLAB
Description
Dark matter (DM) particles with sufficiently large cross sections may scatter as they travel through Earth's bulk. The corresponding changes in the DM flux give rise to a characteristic daily modulation signal in detectors sensitive to DM-electron interactions. Here, we report results obtained from the first underground operation of the DAMIC-M prototype detector searching for such a signal from DM with MeV-scale mass. A model-independent analysis finds no modulation in the rate of $1 e^−$ events with sidereal period, where a DM signal would appear. We then use these data to place exclusion limits on DM in the mass range $[0.53,2.7] MeV/c^2$ interacting with electrons via a dark photon mediator. Taking advantage of the time-dependent signal we improve by $∼2$ orders of magnitude on our previous limit obtained from the total rate of $1 e^−$ events, using the same dataset. This daily modulation search represents the current strongest limit on DM-electron scattering via ultralight mediators for DM masses around $1 MeV/c^2$.
Notes
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PhysRevLett.132.101006.pdf
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Additional details
Identifiers
- DOI
- 10.1103/PhysRevLett.132.101006
- Other
- oai:uchicago.tind.io:14240
Funding
- European Research Council
- European Union’s Horizon 2020 research and innovation programme
- National Science Foundation
- PHY-1812654
- National Science Foundation
- PHY-2110585
- University of Chicago
- Kavli Foundation
- MCIN/AEI/10.13039/501100011033
- PID2019–109829 GB-I00
- MCIN/AEI/10.13039/501100011033
- Ramón y Cajal Grant
- European Union
- Agencia Nacional de Promoción Científica y Tecnológica
- PICT-2018-03069
- Swiss National Science Foundation
- U.S. Department of Energy
- DE-AC02-05CH11231