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The XENON experiment aims at the direct detection of dark matter in the form of WIMPs (Weakly Interacting Massive Particles) via their elastic scattering off Xe nuclei. A fiducial mass of 1000 kg, distributed in ten independent liquid xenon…

A search for inelastic scattering of Weakly Interacting Massive Particles (WIMPs) on the isotope $^{129}$Xe was done in data taken with the single phase liquid xenon detector XMASS at the Kamioka Observatory. Using a restricted volume…

The PICASSO experiment at SNOLAB reports new results for spin-dependent WIMP interactions on $^{19}$F using the superheated droplet technique. A new generation of detectors and new features which enable background discrimination via the…

We report results of a search for light weakly interacting massive particle (WIMP) dark matter from the CDEX-1 experiment at the China Jinping Underground Laboratory (CJPL). Constraints on WIMP-nucleon spin-independent (SI) and…

Very light particles with CP-violating couplings to ordinary matter, such as axions or axion-like particles, can mediate long-range forces between polarized and unpolarized fermions. We describe a new experimental search for such forces…

High Energy Physics - Experiment · Physics 2018-04-25 Junyi Lee , Attaallah Almasi , Michael Romalis

Weakly interacting massive particles (WIMPs) form a promising solution to the dark matter problem and many experiments are now searching for these particles. Using effective field theories to describe the interaction of the WIMP with the…

High Energy Physics - Phenomenology · Physics 2013-08-22 Daniel Schmeier

XENONnT is a dark matter direct detection experiment, utilizing 5.9 t of instrumented liquid xenon, located at the INFN Laboratori Nazionali del Gran Sasso. In this work, we predict the experimental background and project the sensitivity of…

Instrumentation and Detectors · Physics 2020-11-18 The XENON collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , L. Althueser , F. D. Amaro , V. C. Antochi , E. Angelino , J. R. Angevaare , F. Arneodo , D. Barge , L. Baudis , B. Bauermeister , L. Bellagamba , M. L. Benabderrahmane , T. Berger , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , C. Capelli , J. M. R. Cardoso , D. Cichon , B. Cimmino , M. Clark , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , A. Depoian , P. Di Gangi , A. Di Giovanni , R. Di Stefano , S. Diglio , A. Elykov , G. Eurin , A. D. Ferella , W. Fulgione , P. Gaemers , R. Gaior , M. Galloway , F. Gao , L. Grandi , C. Hasterok , C. Hils , K. Hiraide , L. Hoetzsch , J. Howlett , M. Iacovacci , Y. Itow , F. Joerg , N. Kato , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , Q. Lin , S. Lindemann , M. Lindner , F. Lombardi , J. Long , J. A. M. Lopes , E. López Fune , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , A. Manfredini , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , K. Morå , S. Moriyama , Y. Mosbacher , M. Murra , J. Naganoma , K. Ni , U. Oberlack , K. Odgers , J. Palacio , B. Pelssers , R. Peres , J. Pienaar , V. Pizzella , G. Plante , J. Qin , H. Qiu , D. Ramírez García , S. Reichard , A. Rocchetti , N. Rupp , J. M. F. dos Santos , G. Sartorelli , N. Šarčević , M. Scheibelhut , J. Schreiner , D. Schulte , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , E. Shockley , M. Silva , H. Simgen , A. Takeda , C. Therreau , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , K. Valerius , M. Vargas , G. Volta , H. Wang , Y. Wei , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , Z. Xu , M. Yamashita , J. Ye , G. Zavattini , Y. Zhang , T. Zhu , J. P. Zopounidis

It is shown that weakly interacting massive particles (WIMPs), which are possible cold dark matter candidates, can be studied by exclusive measurements of X-rays following WIMPs nuclear interactions. Inner-shell atomic electrons are ionized…

High Energy Physics - Phenomenology · Physics 2009-11-11 H. Ejiri , Ch. C. Moustakidis , J. D. Vergados

The XENON100 experiment, in operation at the Laboratori Nazionali del Gran Sasso in Italy, is designed to search for dark matter WIMPs scattering off 62 kg of liquid xenon in an ultra-low background dual-phase time projection chamber. In…

The EDELWEISS collaboration is searching for WIMP dark matter using natural Ge cryogenic detectors. The whole data set of the first phase of the experiment contains a fiducial exposure of 4.8 kg.day on Ge-73, the naturally present (7.8%),…

XENON100 is a liquid xenon (LXe) time projection chamber built to search for rare collisions of hypothetical, weakly interacting massive particles (WIMPs). Operated in a low-background shield at the Gran Sasso underground laboratory in…

Instrumentation and Methods for Astrophysics · Physics 2012-06-29 P. R. Scovell , XENON100 Collaboration

We report experimental upper limits on WIMP-nucleon elastic scattering cross sections from the second science run of ZEPLIN-III at the Boulby Underground Laboratory. A raw fiducial exposure of 1,344 kg.days was accrued over 319 days of…

We study the prospects for detecting Weakly Interacting Massive Particles (WIMPs), in a number of phenomenological scenarios, with a detector composed of a target simultaneously sensitive to both spin-dependent and spin-independent…

Astrophysics · Physics 2008-11-26 G. Bertone , D. G. Cerdeno , J. I. Collar , B. Odom

We present constraints on the existence of weakly interacting massive particles (WIMPs) from an 11 kg-day target exposure of the DAMIC experiment at the SNOLAB underground laboratory. The observed energy spectrum and spatial distribution of…

We present the results of indirect searches for Weakly Interacting Massive Particles (WIMPs) with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced upward through-going muons. The search is performed by…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , S. Desai , Y. Ashie , S. Fukuda , Y. Fukuda , K. Ishihara , Y. Itow , Y. Koshio , A. Minamino , M. Miura , S. Moriyama , M. Nakahata , T. Namba , R. Nambu , Y. Obayashi , N. Sakurai , M. Shiozawa , Y. Suzuki , H. Takeuchi , Y. Takeuchi , S. Yamada , M. Ishitsuka , T. Kajita , K. Kaneyuki , S. Nakayama , A. Okada , T. Ooyabu , C. Saji , M. Earl , E. Kearns , J. L. Stone , L. R. Sulak , C. W. Walter , W. Wang , M. Goldhaber , T. Barszczak , D. Casper , J. P. Cravens , W. Gajewski , W. R. Kropp , S. Mine , D. W. Liu , M. B. Smy , H. W. Sobel , C. W. Sterner , M. R. Vagins , K. S. Ganezer , J. Hill , W. E. Keig , J. Y. Kim , I. T. Lim , R. W. Ellsworth , S. Tasaka , G. Guillian , A. Kibayashi , J. G. Learned , S. Matsuno , D. Takemori , M. D. Messier , Y. Hayato , A. K. Ichikawa , T. Ishida , T. Ishii , T. Iwashita , J. Kameda , T. Kobayashi , T. Maruyama , K. Nakamura , K. Nitta , Y. Oyama , M. Sakuda , Y. Totsuka , A. T. Suzuki , M. Hasegawa , K. Hayashi , T. Inagaki , I. Kato , H. Maesaka , T. Morita , T. Nakaya , K. Nishikawa , T. Sasaki , S. Ueda , S. Yamamoto , T. J. Haines , S. Dazeley , S. Hatakeyama , R. Svoboda , E. Blaufuss , J. A. Goodman , G. W. Sullivan , D. Turcan , K. Scholberg , A. Habig , C. K. Jung , T. Kato , K. Kobayashi , M. Malek , C. Mauger , C. McGrew , A. Sarrat , E. Sharkey , C. Yanagisawa , T. Toshito , C. Mitsuda , K. Miyano , T. Shibata , Y. Kajiyama , Y. Nagashima , M. Takita , M. Yoshida , H. I. Kim , H. Okazawa , T. Ishizuka , Y. Choi , H. K. Seo , Y. Gando , T. Hasegawa , K. Inoue , J. Shirai , A. Suzuki , M. Koshiba , T. Hashimoto , Y. Nakajima , K. Nishijima , T. Harada , H. Ishino , M. Morii , R. Nishimura , Y. Watanabe , D. Kielczewska , J. Zalipska , R. Gran , K. K. Shiraishi , K. Washburn , R. J. Wilkes

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional analysis and Standard Model particle physics are sufficient to…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Halzen

Guided by the non-relativistic effective field theory of interactions between Weakly Interacting Massive Particles (WIMPs) of spin 1/2 and nuclei we study direct detection exclusion plots for an example of non-standard spin-dependent…

High Energy Physics - Phenomenology · Physics 2018-10-26 Sunghyun Kang , Stefano Scopel , Gaurav Tomar , Jong-Hyun Yoon

The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first…

The XENON100 collaboration has recently released new dark matter limits, placing particular emphasis on their impact on searches known to be sensitive to light-mass (below 10 GeV/c^2) Weakly Interacting Massive Particles (WIMPs), such as…

Cosmology and Nongalactic Astrophysics · Physics 2010-05-14 J. I. Collar , D. N. McKinsey