Results from a Calibration of XENON100 Using a Source of Dissolved Radon-220

A Rn-220 source is deployed on the XENON100 dark matter detector in order to address the challenges in calibration of tonne-scale liquid noble element detectors. We show that the Pb-212 beta emission can be used for low-energy electronic recoil calibration in searches for dark matter. The isotope sp...

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Veröffentlicht in:arXiv.org 2017-04
Hauptverfasser: Aprile, E, Aalbers, J, Agostini, F, Alfonsi, M, Amaro, F D, Barrow, P, Baudis, L, Bauermeister, B, Benabderrahmane, M L, Berger, T, Breur, P A, Brown, E, Bruenner, S, Bruno, G, Butikofer, L, Cardoso, J M R, Cervantes, M, Cichon, D, Coderre, D, Colijn, A P, Conrad, J, Cussonneau, J P, Decowski, M P, DiGangi, P, DiGiovanni, A, Diglio, S, Fei, J, Ferella, A D, Fieguth, A, Franco, D, Fulgione, W, A Gallo Rosso, Galloway, M, Garbini, M, Geis, C, Goetzke, L W, Grandi, L, Greene, Z, Grignon, C, Hasterok, C, Hogenbirk, E, Itay, R, Kaminsky, B, Kessler, G, Kish, A, Landsman, H, Lang, R F, Levinson, L, Lin, Q, Lindemann, S, Lindner, M, Lopes, J A M, Manfredini, A, Maris, I, Undagoitia, T Marrodan, Masbou, J, Massoli, F V, Masson, D, Mayani, D, Meng, Y, Messina, M, Micheneau, K, Miguez, B, Molinario, A, Murra, M, Naganoma, J, K Ni, Oberlack, U, Pakarha, P, Pelssers, B, Persiani, R, Piastra, F, Pienaar, J, Priel, N, Rauch, L, Reichard, S, Reuter, C, Rizzo, A, Rosendahl, S, Rupp, N, Saldanha, R, dosSantos, J M F, Sartorelli, G, Scheibelhut, M, Schindler, S, Schreiner, J, Schumann, M, Selvi, M, Shagin, P, Shockley, E, Silva, M, Simgen, H, Sivers, M v, Stein, A, Tiseni, A, Wang, H, Wei, Y, Weinheimer, C, J Ye, Zhang, Y
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Sprache:eng
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Zusammenfassung:A Rn-220 source is deployed on the XENON100 dark matter detector in order to address the challenges in calibration of tonne-scale liquid noble element detectors. We show that the Pb-212 beta emission can be used for low-energy electronic recoil calibration in searches for dark matter. The isotope spreads throughout the entire active region of the detector, and its activity naturally decays below background level within a week after the source is closed. We find no increase in the activity of the troublesome Rn-222 background after calibration. Alpha emitters are also distributed throughout the detector and facilitate calibration of its response to Rn-222. Using the delayed coincidence of Rn-220/Po-216, we map for the first time the convective motion of particles in the XENON100 detector. Additionally, we make a competitive measurement of the half-life of Po-212, t = 293.9+-(1.0)+-(0.6) ns.
ISSN:2331-8422
DOI:10.48550/arxiv.1611.03585