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Showing papers by "F. Gao published in 2016"


Journal ArticleDOI
Elena Aprile, Jelle Aalbers, F. Agostini, M. Alfonsi, D. Amaro, Matthew Anthony, F. Arneodo, P. Barrow, Laura Baudis, Boris Bauermeister, M. L. Benabderrahmane, T. Berger, A. Breur, April S. Brown, Ethan Brown, S. Bruenner, Giacomo Bruno, Ran Budnik, Lukas Bütikofer, J. Calvén, João Cardoso, M. Cervantes, D. Cichon1, D. Coderre1, Auke-Pieter Colijn, Jan Conrad, Jean-Pierre Cussonneau, M. P. Decowski, P. de Perio, P. Di Gangi, A. Di Giovanni, Sara Diglio, Ehud Duchovni, J. Fei, A. D. Ferella, A. Fieguth, D. Franco, W. Fulgione, A. Gallo Rosso, Michelle Galloway, F. Gao, M. Garbini, C. Geis, Luke Goetzke, Z. Greene, C. Grignon, C. Hasterok, E. Hogenbirk, R. Itay, B. Kaminsky, G. Kessler, A. Kish, H. Landsman, R. F. Lang, Daniel Lellouch, Lorne Levinson, M. Le Calloch, C. Levy, Qing Lin, Sebastian Lindemann1, Manfred Lindner1, J. A. M. Lopes1, A. Manfredini, T. Marrodán Undagoitia1, Julien Masbou1, F. V. Massoli, D. Masson, D. Mayani, Y. Meng, M. Messina, K. Micheneau, B. Miguez, A. Molinario, M. Murra, J. Naganoma, Kaixuan Ni, Uwe Oberlack, A. Orrigo, P. Pakarha, Bart Pelssers, R. Persiani, F. Piastra, J. Pienaar, C. Piro, G. Plante, N. Priel, L. Rauch, S. Reichard, C. Reuter, A. Rizzo, S. Rosendahl, N. Rupp, J. M. F. dos Santos, Gabriella Sartorelli, M. Scheibelhut, S. Schindler, Jochen Schreiner1, Marc Schumann1, L. Scotto Lavina, M. Selvi, P. Shagin, Manuel Gameiro da Silva, Hardy Simgen1, M. V. Sivers1, A. Stein, D. Thers, A. Tiseni, G. C. Trinchero, C. Tunnell, R. Wall, Hongwei Wang, Max Weber, Yuehuan Wei, Ch. Weinheimer, J. Wulf, Yanxi Zhang, F. D. Amaro, P. A. Breur, S. E. A. Orrigo, M.-C. Piro, J.M.F. dos Santos 
TL;DR: In this paper, a profile likelihood analysis using an energy range of (6.6 - 43.3) keV$_{\mathrm{nr}}$ sets a limit on the elastic, spin-independent WIMP-nucleon scattering cross section for WIMPs above 8 GeV/$c^2.
Abstract: We report on WIMP search results of the XENON100 experiment, combining three runs summing up to 477 live days from January 2010 to January 2014. Data from the first two runs were already published. A blind analysis was applied to the last run recorded between April 2013 and January 2014 prior to combining the results. The ultra-low electromagnetic background of the experiment, ~$5 \times 10^{-3}$ events/(keV$_{\mathrm{ee}}\times$kg$\times$day) before electronic recoil rejection, together with the increased exposure of 48 kg $\times$ yr improves the sensitivity. A profile likelihood analysis using an energy range of (6.6 - 43.3) keV$_{\mathrm{nr}}$ sets a limit on the elastic, spin-independent WIMP-nucleon scattering cross section for WIMP masses above 8 GeV/$c^2$, with a minimum of 1.1 $\times 10^{-45}$ cm$^2$ at 50 GeV/$c^2$ and 90% confidence level. We also report updated constraints on the elastic, spin-dependent WIMP-nucleon cross sections obtained with the same data. We set upper limits on the WIMP-neutron (proton) cross section with a minimum of 2.0 $\times 10^{-40}$ cm$^2$ (52$\times 10^{-40}$ cm$^2$) at a WIMP mass of 50 GeV/$c^2$, at 90% confidence level.

170 citations


Journal ArticleDOI
Elena Aprile, Jelle Aalbers, F. Agostini, M. Alfonsi, F. D. Amaro, M. Anthony, F. Arneodo, P. Barrow, Laura Baudis, Boris Bauermeister, M. L. Benabderrahmane, T. Berger, P. A. Breur, April S. Brown, Ethan Brown, S. Bruenner, Giacomo Bruno, Ran Budnik, L. Bütikofer, J. Calvén, João Cardoso, M. Cervantes, D. Cichon, D. Coderre, Auke-Pieter Colijn, Jan Conrad, Jean-Pierre Cussonneau, M. P. Decowski, P. de Perio, P. Di Gangi, A. Di Giovanni, Sara Diglio, Ehud Duchovni, G. Eurin, J. Fei, A. D. Ferella, A. Fieguth, D. Franco, W. Fulgione, A. Gallo Rosso, Michelle Galloway, F. Gao, M. Garbini, C. Geis, Luke Goetzke, L. Grandi, Z. Greene, C. Grignon, C. Hasterok, E. Hogenbirk, R. Itay, B. Kaminsky, G. Kessler, A. Kish, H. Landsman, R. F. Lang, D. Lellouch, L. Levinson, M. Le Calloch, Qing Lin, Sebastian Lindemann, Manfred Lindner, J. A. M. Lopes A. Manfredini, Ioana Codrina Maris, T. Marrodán Undagoitia, Julien Masbou, F. V. Massoli, D. Masson, D. Mayani, Y. Meng, M. Messina, K. Micheneau, B. Miguez, A. Molinario, M. Murra, J. Naganoma, Kaixuan Ni, Uwe Oberlack, S. E. A. Orrigo, P. Pakarha, Bart Pelssers, R. Persiani, F. Piastra, J. Pienaar, M.-C. Piro, V. Pizzella, G. Plante, N. Priel, L. Rauch, S. Reichard, C. Reuter, A. Rizzo, S. Rosendahl, N. Rupp, R. Saldanha, J.M.F. dos Santos, G. Sartorelli, M. Scheibelhut, S. Schindler, Jochen Schreiner, Marc Schumann, L. Scotto Lavina, M. Selvi, P. Shagin, E. Shockley, Manuel Gameiro da Silva, Hardy Simgen, M. v. Sivers, A. Stein, D. Thers, A. Tiseni, G. C. Trinchero, C. Tunnell, N. Upole, Hulin Wang, Yuehuan Wei, Ch. Weinheimer, J. Wulf, J. Ye, Yanxi Zhang, I. Cristescu 
TL;DR: In this paper, the design of a novel cryogenic distillation column using the common McCabe-Thiele approach is described, and the system demonstrated a krypton reduction factor of 6.4$\cdot$10$^5$ with thermodynamic stability at process speeds above 3 kg/h.
Abstract: The XENON1T experiment aims for the direct detection of dark matter in a cryostat filled with 3.3 tons of liquid xenon. In order to achieve the desired sensitivity, the background induced by radioactive decays inside the detector has to be sufficiently low. One major contributor is the $\beta$-emitter $^{85}$Kr which is an intrinsic contamination of the xenon. For the XENON1T experiment a concentration of natural krypton in xenon $\rm{^{nat}}$Kr/Xe < 200 ppq (parts per quadrillion, 1 ppq = 10$^{-15}$ mol/mol) is required. In this work, the design of a novel cryogenic distillation column using the common McCabe-Thiele approach is described. The system demonstrated a krypton reduction factor of 6.4$\cdot$10$^5$ with thermodynamic stability at process speeds above 3 kg/h. The resulting concentration of $\rm{^{nat}}$Kr/Xe < 26 ppq is the lowest ever achieved, almost one order of magnitude below the requirements for XENON1T and even sufficient for future dark matter experiments using liquid xenon, such as XENONnT and DARWIN.

27 citations