Exclusion of leptophilic dark matter models using XENON100 electronic recoil data

Autoria(s): Aprile, E.; Agostini, F.; Alfonsi, M.; Arazi, L.; Arisaka, K.; Arneodo, F.; Auger, M.; Balan, C.; Barrow, P.; Baudis, L.; Bauermeister, B.; Behrens, A.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Bütikofer, Lukas; Cardoso, J. M. R.; Cervantes, M.; Coderre, Daniel; Colijn, A. P.; Contreras, H.; Cussonneau, J. P.; Decowski, M. P.; Di Giovanni, A.; Duchovni, E.; Fattori, S.; Ferella, A. D.; Fieguth, A.; Fulgione, W.; Gao, F.; Garbini, M.; Geis, C.; Goetzke, L. W.; Grignon, C.; Gross, E.; Hampel, W.; Itay, R.; Kaether, F.; Kaminsky, Jan Basho; Kessler, G.; Kish, A.; Landsman, H.; Lang, R. F.; Le Calloch, M.; Lellouch, D.; Levinson, L.; Levy, C.; Lindemann, S.; Lindner, M.; Lopes, J. A. M.; Lyashenko, A.; Macmullin, S.; Undagoitia, T. M.; Masbou, J.; Massoli, F. V.; Mayani, D.; Fernandez, A. J. M.; Meng, Y.; Messina, M.; Miguez, B.; Molinario, A.; Morana, G.; Murra, M.; Naganoma, J.; Ni, K.; Oberlack, U.; Orrigo, S. E. A.; Pakarha, P.; Pantic, E.; Persiani, R.; Piastra, F.; Pienaar, J.; Plante, G.; Priel, N.; Rauch, L.; Reichard, S.; Reuter, C.; Rizzo, A.; Rosendahl, S.; dos Santos, J. M. F.; Sartorelli, G.; Schindler, S.; Schreiner, J.; Schumann, Marc; Lavina, L. S.; Selvi, M.; Shagin, P.; Simgen, H.; Teymourian, A.; Thers, D.; Tiseni, A.; Trinchero, G.; Tunnell, C.; Vitells, O.; Wall, R.; Wang, H.; Weber, M.; Weinheimer, C.
Data(s)

2015

31/12/1969
Resumo

We have searched for periodic variations of the electronic recoil event rate in the (2-6) keV energy range recorded between February 2011 and March 2012 with the XENON100 detector, adding up to 224.6 live days in total. Following a detailed study to establish the stability of the detector and its background contributions during this run, we performed an un-binned profile likelihood analysis to identify any periodicity up to 500 days. We find a global significance of less than 1 sigma for all periods suggesting no statistically significant modulation in the data. While the local significance for an annual modulation is 2.8 sigma, the analysis of a multiple-scatter control sample and the phase of the modulation disfavor a dark matter interpretation. The DAMA/LIBRA annual modulation interpreted as a dark matter signature with axial-vector coupling of WIMPs to electrons is excluded at 4.8 sigma.
Formato

application/pdf

application/pdf
Identificador

http://boris.unibe.ch/81222/1/851.full.pdf

http://boris.unibe.ch/81222/8/1507.07747v1.pdf

Aprile, E.; Agostini, F.; Alfonsi, M.; Arazi, L.; Arisaka, K.; Arneodo, F.; Auger, M.; Balan, C.; Barrow, P.; Baudis, L.; Bauermeister, B.; Behrens, A.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Bütikofer, Lukas; Cardoso, J. M. R.; Cervantes, M.; ... (2015). Exclusion of leptophilic dark matter models using XENON100 electronic recoil data. Science, 349(6250), pp. 851-854. American Association for the Advancement of Science 10.1126/science.aab2069 <http://dx.doi.org/10.1126/science.aab2069>

doi:10.7892/boris.81222

info:doi:10.1126/science.aab2069

urn:issn:0036-8075
Idioma(s)

eng
Publicador

American Association for the Advancement of Science
Relação

http://boris.unibe.ch/81222/
Direitos

info:eu-repo/semantics/restrictedAccess

info:eu-repo/semantics/openAccess
Fonte

Aprile, E.; Agostini, F.; Alfonsi, M.; Arazi, L.; Arisaka, K.; Arneodo, F.; Auger, M.; Balan, C.; Barrow, P.; Baudis, L.; Bauermeister, B.; Behrens, A.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Bütikofer, Lukas; Cardoso, J. M. R.; Cervantes, M.; ... (2015). Exclusion of leptophilic dark matter models using XENON100 electronic recoil data. Science, 349(6250), pp. 851-854. American Association for the Advancement of Science 10.1126/science.aab2069 <http://dx.doi.org/10.1126/science.aab2069>
Palavras-Chave #530 Physics
Tipo

info:eu-repo/semantics/article

info:eu-repo/semantics/publishedVersion

PeerReviewed
Acesso ao item digital