# First results on sub-GeV spin-dependent dark matter interactions with   $^{7}$Li

**Authors:** A.H. Abdelhameed, G. Angloher, P. Bauer, A. Bento, E. Bertoldo, C., Bucci, L. Canonica, A. D'Addabbo, X. Defay, S. Di Lorenzo, A. Erb, F. v., Feilitzsch, N. Ferreiro Iachellini, S. Fichtinger, A. Fuss, P. Gorla, D., Hauff, J. Jochum, A. Kinast, H. Kluck, H. Kraus, A. Langenk\"amper, M., Mancuso, V. Mokina, E. Mondragon, A. M\"unster, M. Olmi, T. Ortmann, C., Pagliarone, L. Pattavina, F. Petricca, W. Potzel, F. Pr\"obst, F. Reindl, J., Rothe, K. Sch\"affner, J. Schieck, V. Schipperges, D. Schmiedmayer, S., Sch\"onert, C. Schwertner, M. Stahlberg, L. Stodolsky, C. Strandhagen, R., Strauss, C. T\"urkoglu, I. Usherov, M. Willers, V. Zema, (The CRESST, Collaboration), M. Chapellier, A. Giuliani, C. Nones, D.V. Poda, V.N., Shlegel, M. Vel\'azquez, A.S. Zolotarova

arXiv: 1902.07587 · 2020-02-11

## TL;DR

This study explores lithium-based detectors for low-mass spin-dependent dark matter interactions, demonstrating competitive limits in a challenging environment, and highlighting lithium's potential in cryogenic dark matter searches.

## Contribution

First experimental results showing lithium's viability as a target for low-mass spin-dependent dark matter detection in cryogenic setups.

## Key findings

- Set competitive limits on dark matter interactions with protons and neutrons.
- Demonstrated detector operation in an above-ground environment.
- Focused on the low-mass dark matter parameter space (0.8-1.5 GeV/c$^2$).

## Abstract

In this work, we want to highlight the potential of lithium as a target for spin-dependent dark matter search in cryogenic experiments, with a special focus on the low-mass region of the parameter space. We operated a prototype detector module based on a Li$_2$MoO$_4$ target crystal in an above-ground laboratory. Despite the high background environment, the detector sets competitive limits on spin-dependent interactions of dark matter particles with protons and neutrons for masses between 0.8 GeV/c$^2$ and 1.5 GeV/c$^2$.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1902.07587/full.md

## References

55 references — full list in the complete paper: https://tomesphere.com/paper/1902.07587/full.md

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Source: https://tomesphere.com/paper/1902.07587