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This work is a study of some possible background sources in the XENON1T environment which might affect the energy spectrum of electronic recoil events in the lower side and might contribute to the observed excess.
N. F. Bell, V. Cirigliano, M. J. Ramsey-Musolf, P. Vogel, and M. B. Wise, “How magnetic is the Dirac neutrino?,” Phys. Rev. Lett
2005
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N. F. Bell, M. Gorchtein, M. J. Ramsey-Musolf, P. Vogel, and P. Wang, “Model independent bounds on magnetic moments of Majorana neutrinos,” Phys. Lett. B
2006
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2006
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2006
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2006
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2006
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2006
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2006
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2006
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2006
Cited alongside, same era.
2006
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2006
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H. M. Lee, “Exothermic Dark Matter for XENON1T Excess,” arXiv:2006.13183 [hep-ph]
2006
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A. E. Robinson, “XENON1T observes tritium,” arXiv:2006.13278 [hep-ex]
2006
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2006
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2006
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2006
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2006
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2006
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2007
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2008
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2015
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X. Mougeot, “Reliability of usual assumptions in the calculation of β \beta and ν \nu spectra,” Phys. Rev. C
2015
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2016
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2017
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PhD thesis, Zurich, U., 11, 2017
F. Piastra, Materials radioassay for the XENON1T dark matter experiment, and development of a time projection chamber for the study of low-energy nuclear recoils in liquid xenon · 2017
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E. Shockley (for XENON Collaboration), “Search for New Physics with Electronic-Recoil Events in XENON1T,” LNGS Webinar, June 17th, 2020
2020
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https://www-nds.iaea.org/livechart/ . IAEA, Nuclear Data Section, 2020
M. Verpelli and L. Vrapcenjak, LiveChart of Nuclides · 2020
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