Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector

Aprile, E.; Aalbers, J.; Agostini, F.; Alfonsi, M.; Amaro, F. D.; Anthony, M.; Arneodo, F.; Barrow, P.; Baudis, L.; Bauermeister, B.; Benabderrahmane, M. L.; Berger, T.; Breur, P. A.; Brown, A.; Brown, E.; Bruenner, S.; Bruno, G.; Budnik, R.; Bütikofer, L.; Calvén, J.; Cardoso, J. M. R.; Cervantes, M.; Cichon, D.; Coderre, D.; Colijn, A. P.; Conrad, J.; Cussonneau, J. P.; Decowski, M. P.; De Perio, P.; Di Gangi, P.; Di Giovanni, A.; Diglio, S.; Eurin, G.; Fei, J.; Ferella, A. D.; Fieguth, A.; Fulgione, W.; Gallo Rosso, A.; Galloway, M.; Gao, F.; Garbini, M.; Geis, C.; Goetzke, L. W.; Greene, Z.; Grignon, C.; Hasterok, C.; Hogenbirk, E.; Itay, R.; Kaminsky, B.; Kazama, S.; Kessler, G.; Kish, A.; Landsman, H.; Lang, R. F.; Lellouch, D.; Levinson, L.; Lin, Q.; Lindemann, S.; Lindner, M.; Lombardi, F.; Lopes, J. A. M.; Manfredini, A.; Maris, I.; Marrodán Undagoitia, T.; Masbou, J.; Massoli, F. V.; Masson, D.; Mayani, D.; Messina, M.; Micheneau, K.; Molinario, A.; Morå, K.; Murra, M.; Naganoma, J.; Ni, K.; Oberlack, U.; Pakarha, P.; Pelssers, B.; Persiani, R.; Piastra, F.; Pienaar, J.; Pizzella, V.; Piro, M. -C.; Plante, G.; Priel, N.; Rauch, L.; Reichard, S.; Reuter, C.; Rizzo, A.; Rosendahl, S.; Rupp, N.; Dos Santos, J. M. F.; Sartorelli, G.; Scheibelhut, M.; Schindler, S.; Schreiner, J.; Schumann, M.; Scotto Lavina, L.; Selvi, M.; Shagin, P.; Silva, M.; Simgen, H.; Sivers, M. V.; Stein, A.; Thers, D.; Tiseni, A.; Trinchero, G.; Tunnell, C.; Vargas, M.; Wang, H.; Wang, Z.; Wei, Y.; Weinheimer, C.; Wulf, J.; Ye, J.; Farmer, B.; Zhang, Y.

doi:10.1103/PhysRevD.96.042004

We report on weakly interacting massive particles (WIMPs) search results in the XENON100 detector using a nonrelativistic effective field theory approach. The data from science run II (34 kgÃ224.6 live days) were reanalyzed, with an increased recoil energy interval compared to previous analyses, ranging from (6.6-240) keVnr. The data are found to be compatible with the background-only hypothesis. We present 90% confidence level exclusion limits on the coupling constants of WIMP-nucleon effective operators using a binned profile likelihood method. We also consider the case of inelastic WIMP scattering, where incident WIMPs may up-scatter to a higher mass state, and set exclusion limits on this model as well.

Aprile, E., Aalbers, J., Agostini, F., Alfonsi, M., Amaro, F.D., Anthony, M., et al. (2017). Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector. PHYSICAL REVIEW D, 96(4), 1-13 [10.1103/PhysRevD.96.042004].

Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector

Aprile, E.;Aalbers, J.;Alfonsi, M.;Amaro, F. D.;Anthony, M.;Arneodo, F.;Barrow, P.;Baudis, L.;Bauermeister, B.;Benabderrahmane, M. L.;Berger, T.;Breur, P. A.;Brown, A.;Brown, E.;Bruenner, S.;Bruno, G.;Budnik, R.;Bütikofer, L.;Calvén, J.;Cardoso, J. M. R.;Cervantes, M.;Cichon, D.;Coderre, D.;Colijn, A. P.;Conrad, J.;Cussonneau, J. P.;Decowski, M. P.;De Perio, P.;Di Gangi, P.^{Membro del Collaboration Group};Di Giovanni, A.;Diglio, S.;Eurin, G.;Fei, J.;Ferella, A. D.;Fieguth, A.;Fulgione, W.;Gallo Rosso, A.;Galloway, M.;Gao, F.;Garbini, M.^{Membro del Collaboration Group};Geis, C.;Goetzke, L. W.;Greene, Z.;Grignon, C.;Hasterok, C.;Hogenbirk, E.;Itay, R.;Kaminsky, B.;Kazama, S.;Kessler, G.;Kish, A.;Landsman, H.;Lang, R. F.;Lellouch, D.;Levinson, L.;Lin, Q.;Lindemann, S.;Lindner, M.;Lombardi, F.;Lopes, J. A. M.;Manfredini, A.;Maris, I.;Marrodán Undagoitia, T.;Masbou, J.;Massoli, F. V.;Masson, D.;Mayani, D.;Messina, M.;Micheneau, K.;Molinario, A.;Morå, K.;Murra, M.;Naganoma, J.;Ni, K.;Oberlack, U.;Pakarha, P.;Pelssers, B.;Persiani, R.;Piastra, F.;Pienaar, J.;Pizzella, V.;Piro, M. -C.;Plante, G.;Priel, N.;Rauch, L.;Reichard, S.;Reuter, C.;Rosendahl, S.;Rupp, N.;Dos Santos, J. M. F.;Sartorelli, G.^{Membro del Collaboration Group};Scheibelhut, M.;Schindler, S.;Schreiner, J.;Schumann, M.;Scotto Lavina, L.;Selvi, M.^{Membro del Collaboration Group};Shagin, P.;Silva, M.;Simgen, H.;Sivers, M. V.;Stein, A.;Thers, D.;Tiseni, A.;Trinchero, G.;Tunnell, C.;Vargas, M.;Wang, H.;Wang, Z.;Wei, Y.;Weinheimer, C.;Wulf, J.;Ye, J.;Farmer, B.;Zhang, Y.

2017

Abstract

We report on weakly interacting massive particles (WIMPs) search results in the XENON100 detector using a nonrelativistic effective field theory approach. The data from science run II (34 kgÃ224.6 live days) were reanalyzed, with an increased recoil energy interval compared to previous analyses, ranging from (6.6-240) keVnr. The data are found to be compatible with the background-only hypothesis. We present 90% confidence level exclusion limits on the coupling constants of WIMP-nucleon effective operators using a binned profile likelihood method. We also consider the case of inelastic WIMP scattering, where incident WIMPs may up-scatter to a higher mass state, and set exclusion limits on this model as well.

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	Anno
	
				2017
			
	Rivista
	
				PHYSICAL REVIEW D
			
	Codice DOI
	
				https://dx.doi.org/10.1103/PhysRevD.96.042004
			
	Citazione
	
				Aprile, E., Aalbers, J., Agostini, F., Alfonsi, M., Amaro, F.D., Anthony, M., et al. (2017). Effective field theory search for high-energy nuclear recoils using the XENON100 dark matter detector. PHYSICAL REVIEW D, 96(4), 1-13 [10.1103/PhysRevD.96.042004].
			
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						Aprile, E.; Aalbers, J.; Agostini, F.; Alfonsi, M.; Amaro, F.D.; Anthony, M.; Arneodo, F.; Barrow, P.; Baudis, L.; Bauermeister, B.; Benabderrahmane, ...espandi
						
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/627619

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