# Constraints on Light Dark Matter Particles Interacting with Electrons   from DAMIC at SNOLAB

**Authors:** A. Aguilar-Arevalo, D. Amidei, D. Baxter, G. Cancelo, B.A. Cervantes, Vergara, A.E. Chavarria, E. Darragh-Ford, J.R.T. de Mello Neto, J.C. D'Olivo,, J. Estrada, R. Ga\"ior, Y. Guardincerri, T.W. Hossbach, B. Kilminster, I., Lawson, S.J. Lee, A. Letessier-Selvon, A. Matalon, V.B.B. Mello, P. Mitra,, Y.S. Mobarak, J. Molina, S. Paul, A. Piers, P. Privitera, K. Ramanathan, J., Da Rocha, M. Settimo, R. Smida, R. Thomas, J. Tiffenberg, D. Torres Machado,, R. Vilar, A.L. Virto

arXiv: 1907.12628 · 2020-04-09

## TL;DR

This paper presents new direct-detection constraints on light dark matter particles interacting with electrons, using the DAMIC detector's ultra-low leakage current to explore previously untested parameter space for masses from 0.6 to 100 MeV/c² and hidden-photon dark matter.

## Contribution

It introduces a novel detection method leveraging DAMIC's low leakage current to constrain light dark matter interactions with electrons and hidden photons.

## Key findings

- Constraints on dark matter masses between 0.6 and 100 MeV/c².
- New limits on hidden-photon dark matter in the 1.2-30 eV/c² range.
- Demonstrates the effectiveness of leakage current analysis for dark matter detection.

## Abstract

We report direct-detection constraints on light dark matter particles interacting with electrons. The results are based on a method that exploits the extremely low levels of leakage current of the DAMIC detector at SNOLAB of 2-6$\times$10$^{-22}$ A cm$^{-2}$. We evaluate the charge distribution of pixels that collect $<10~\rm{e^-}$ for contributions beyond the leakage current that may be attributed to dark matter interactions. Constraints are placed on so-far unexplored parameter space for dark matter masses between 0.6 and 100 MeV$c^{-2}$. We also present new constraints on hidden-photon dark matter with masses in the range $1.2$-$30$ eV$c^{-2}$.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1907.12628/full.md

## References

35 references — full list in the complete paper: https://tomesphere.com/paper/1907.12628/full.md

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Source: https://tomesphere.com/paper/1907.12628