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2019

Aprile, E., Aalbers, J., Agostini, F. et al.

We report constraints on light dark matter (DM) models using ionization signals in the XENON1T experiment.

We mitigate backgrounds with strong event selections, rather than requiring a scintillation signal, leaving an effective exposure of $(22 \pm 3)$ tonne-days.
Above $\sim\!0.4\,\mathrm{keV}_\mathrm{ee}$, we observe $<1 \, \text{event}/(\text{tonne} \times \text{day} \times \text{keV}_\text{ee})$, which is more than one thousand times lower than in similar searches with other detectors.
Despite observing a higher rate at lower energies, no DM or CEvNS detection may be claimed because we cannot model all of our backgrounds.

L. Roszkowski et al
Original
1902
Earlier work this paper cites.
E. Aprile et al
Original
1902
Earlier work this paper cites.
E. Aprile et al
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Earlier work this paper cites.
E. Aprile et al
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1906
Earlier work this paper cites.
E. Aprile et al
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Earlier work this paper cites.
S.A. Stouffer et al
1949
Earlier work this paper cites.
G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405
2005
Earlier work this paper cites.
M. Pospelov, A. Ritz, and M. Voloshin, Phys. Rev. D 78
Original
2008
Earlier work this paper cites.
C. E. Aalseth et al
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Earlier work this paper cites.
P. Sorensen, Nucl. Instr. Meth. A 635
Original
2011
Earlier work this paper cites.
A. M. Serenelli et al
Original
2011
Earlier work this paper cites.
N. Fornengo, P. Panci and M. Regis, Phys. Rev. D 84
Original
2011
Earlier work this paper cites.
R. Essig et al
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J. Angle et al
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Earlier work this paper cites.
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2015
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E. Del Nobile, M. Kaplinghat, and H.-B. Yu, JCAP 1510
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P. A. R. Ade et al
Original
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Later among the works it cites.
E. Aprile et al
Original
2018
Later among the works it cites.
R. F. Lang et al
2018
Later among the works it cites.
M. Szydagis et al
2018
Later among the works it cites.
X. Ren et al
Original
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Later among the works it cites.
T.-T. Yu, http://ddldm.physics.sunysb.edu/ddlDM (5 November 2018)
2018
Later among the works it cites.