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28 March 2024
 
  » arxiv » 1704.5804

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Search for magnetic inelastic dark matter with XENON100
XENON collaboration ; E. Aprile ; J. Aalbers ; F. Agostini ; M. Alfonsi ; F. D. Amaro ; M. Anthony ; F. Arneodo ; P. Barrow ; L. Baudis ; B. Bauermeister ; M. L. Benabderrahmane ; T. Berger ; P. A. Breur ; A. Brown ; E. Brown ; S. Bruenner ; G. Bruno ; R. Budnik ; L. Bütikofer ; J. Calvén ; J. M. R. Cardoso ; M. Cervantes ; D. Cichon ; D. Coderre ; A. P. Colijn ; J. Conrad ; J. P. Cussonneau ; M. P. Decowski ; P. de Perio ; P. Di Gangi ; A. Di Giovanni ; S. Diglio ; G. Eurin ; J. Fei ; A. D. Ferella ; A. Fieguth ; D. Franco ; W. Fulgione ; A. Gallo Rosso ; M. Galloway ; F. Gao ; M. Garbini ; C. Geis ; L. W. Goetzke ; 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 ; Q. Lin ; S. Lindemann ; M. Lindner ; F. Lombardi ; J. A. M. Lopes ; A. Manfredini ; I. Maris ; T. Marrodán Undagoitia ; J. Masbou ; F. V. Massoli ; D. Masson ; D. Mayani ; M. Messina ; K. Micheneau ; A. Molinario ; M. Murra ; J. Naganoma ; K. Ni ; U. Oberlack ; P. Pakarha ; B. Pelssers ; R. Persiani ; F. Piastra ; J. Pienaar ; V. Pizzella ; M.-C. Piro ; G. Plante ; N. Priel ; L. Rauch ; S. Reichard ; C. Reuter ; A. Rizzo ; S. Rosendahl ; N. Rupp ; J. M. F. dos Santos ; G. Sartorelli ; M. Scheibelhut ; S. Schindler ; J. Schreiner ; M. Schumann ; L. Scotto Lavina ; M. Selvi ; P. Shagin ; M. Silva ; H. Simgen ; M. v. Sivers ; A. Stein ; D. Thers ; A. Tiseni ; G. Trinchero ; C. Tunnell ; M. Vargas ; H. Wang ; Y. Wei ; C. Weinheimer ; J. Wulf ; J. Ye ; Y. Zhanga ;
Date 19 Apr 2017
AbstractWe present the first search for dark matter-induced delayed coincidence signals in a dual-phase xenon time projection chamber, using the 224.6,live days of the XENON100 science run~II. This very distinct signature is predicted in the framework of magnetic inelastic dark matter which has been proposed to reconcile the modulation signal reported by the DAMA/LIBRA collaboration with the null results from other direct detection experiments. No candidate event has been found in the region of interest and upper limits on the WIMP’s magnetic dipole moment are derived. The scenarios proposed to explain the DAMA/LIBRA modulation signal by magnetic inelastic dark matter interactions of WIMPs with masses of 58.0,GeV/c$^2$ and 122.7,GeV/c$^2$ are excluded at 3.3,$sigma$ and 9.3,$sigma$, respectively.
Source arXiv, 1704.5804
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