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25 April 2024

» arxiv » 1709.2222

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Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment
XENON collaboration ; E. Aprile ; J. Aalbers ; F. Agostini ; M. Alfonsi ; L. Althueser ; F. D. Amaro ; M. Anthony ; F. Arneodo ; P. Barrow ; L. Baudis ; B. Bauermeister ; M. L. Benabderrahmane ; T. Berger ; P. A. Breur ; A. Brown ; A. Brown ; E. Brown ; S. Bruenner ; G. Bruno ; R. Budnik ; Bütikofer ; J. Calven ; C. Capelli ; J. M. R. Cardoso ; 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 ; W. Fulgione ; A. Gallo Rosso ; M. Galloway ; F. Gao ; M. Garbini ; C. Geis ; L. W. Goetzke ; Z. Greene ; C. Grignon ; C. Hasterok ; E. Hogenbirk ; J. Howlett ; R. Itay ; B. Kaminsky ; S. Kazama ; 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 ; K. Morå ; 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 ; D. Ramírez García ; L. Rauch ; S. Reichard ; C. Reuter ; A. Rizzo ; 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 ; Z. Wang ; Y. Wei ; C. Weinheimer ; C. Wittweg ; J. Wulf ; J. Ye ; Y. Zhang ; T. Zhu ;
Date:	7 Sep 2017
Abstract:	We present results of searches for vector and pseudo-scalar bosonic super-WIMPs, which are dark matter candidates with masses at the keV-scale, with the XENON100 experiment. XENON100 is a dual-phase xenon time projection chamber operated at the Laboratori Nazionali del Gran Sasso. A profile likelihood analysis of data with an exposure of 224.6 live days $ imes$ 34,kg showed no evidence for a signal above the expected background. We thus obtain new and stringent upper limits in the $(8-125)$,keV/c$^2$ mass range, excluding couplings to electrons with coupling constants of $g_{ae} > 3 imes10^{-13}$ for pseudo-scalar and $alpha’/alpha > 2 imes10^{-28}$ for vector super-WIMPs, respectively. These limits are derived under the assumption that super-WIMPs constitute all of the dark matter in our galaxy.
Source:	arXiv, 1709.2222
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