# First Dark Matter Search Results from the XENON1T Experiment

**Authors:** E. Aprile, J. Aalbers, F. Agostini, M. Alfonsi, F. D. Amaro, M., Anthony, F. Arneodo, P. Barrow, L. Baudis, B. Bauermeister, M. L., Benabderrahmane, T. Berger, P. A. Breur, A. Brown, A. Brown, E. Brown, S., Bruenner, G. Bruno, R. Budnik, L. B\"utikofer, J. Calv\'en, J. M. R. Cardoso,, M. Cervantes, D. Cichon, D. Coderre, A. P. Colijn, J. Conrad, J. P., Cussonneau, M. P. Decowski, P. de Perio, P. Di Gangi, A. Di Giovanni, S., Diglio, G. Eurin, J. Fei, A. D. Ferella, A. Fieguth, W. Fulgione, A. Gallo, Rosso, M. Galloway, F. Gao, M. Garbini, R. Gardner, C. Geis, L. W. Goetzke,, L. Grandi, Z. Greene, C. Grignon, C. Hasterok, E. Hogenbirk, J. Howlett, R., Itay, B. Kaminsky, S. Kazama, G. Kessler, A. Kish, H. Landsman, R. F. Lang,, D. Lellouch, L. Levinson, Q. Lin, S. Lindemann, M. Lindner, F. Lombardi, J., A. M. Lopes, A. Manfredini, I. Mari\c{s}, T. Marrod\'an Undagoitia, J., Masbou, F. V. Massoli, D. Masson, D. Mayani, M. Messina, K. Micheneau, A., Molinario, K. Mor{\aa}, M. Murra, J. Naganoma, K. Ni, U. Oberlack, P., Pakarha, B. Pelssers, R. Persiani, F. Piastra, J. Pienaar, V. Pizzella, M.-C., Piro, G. Plante, N. Priel, L. Rauch, S. Reichard, C. Reuter, B. Riedel, A., Rizzo, S. Rosendahl, N. Rupp, R. Saldanha, J. M. F. dos Santos, G., Sartorelli, M. Scheibelhut, S. Schindler, J. Schreiner, M. Schumann, L., Scotto Lavina, M. Selvi, P. Shagin, E. Shockley, M. Silva, H. Simgen, M. v., Sivers, A. Stein, S. Thapa, D. Thers, A. Tiseni, G. Trinchero, C. Tunnell, M., Vargas, N. Upole, H. Wang, Z. Wang, Y. Wei, C. Weinheimer, J. Wulf, J. Ye, Y., Zhang, T. Zhu

arXiv: 1705.06655 · 2017-11-27

## TL;DR

The XENON1T experiment conducted the first dark matter search with a 2000-kg xenon detector, achieving unprecedented background levels and setting the most stringent limits on WIMP interactions for masses above 10 GeV/c².

## Contribution

This work presents the first results from XENON1T, demonstrating its low background and setting new leading limits on WIMP-nucleon cross sections at a ton-scale.

## Key findings

- Achieved the lowest electronic recoil background in a dark matter detector.
- Set the most stringent exclusion limits on WIMP-nucleon cross sections for masses above 10 GeV/c².
- Data is consistent with background-only hypothesis.

## Abstract

We report the first dark matter search results from XENON1T, a $\sim$2000-kg-target-mass dual-phase (liquid-gas) xenon time projection chamber in operation at the Laboratori Nazionali del Gran Sasso in Italy and the first ton-scale detector of this kind. The blinded search used 34.2 live days of data acquired between November 2016 and January 2017. Inside the (1042$\pm$12) kg fiducial mass and in the [5, 40] $\mathrm{keV}_{\mathrm{nr}}$ energy range of interest for WIMP dark matter searches, the electronic recoil background was $(1.93 \pm 0.25) \times 10^{-4}$ events/(kg $\times$ day $\times \mathrm{keV}_{\mathrm{ee}}$), the lowest ever achieved in a dark matter detector. A profile likelihood analysis shows that the data is consistent with the background-only hypothesis. We derive the most stringent exclusion limits on the spin-independent WIMP-nucleon interaction cross section for WIMP masses above 10 GeV/c${}^2$, with a minimum of 7.7 $\times 10^{-47}$ cm${}^2$ for 35-GeV/c${}^2$ WIMPs at 90% confidence level.

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/1705.06655/full.md

## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1705.06655/full.md

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Source: https://tomesphere.com/paper/1705.06655