Related papers: Introduction of the CDEX experiment

Results from the Cryogenic Dark Matter Search experiment

The Cryogenic Dark Matter Search experiment uses low-temperature solid-state detectors to seek Weakly Interacting Massive Particles (WIMPs) and has the world's best exclusion limit on the spin-independent WIMP-nucleon cross section. The…

High Energy Physics - Experiment · Physics 2019-08-13 Oleg Kamaev

Light weakly interacting massive particles

Light WIMPs are dark matter particle candidates with weak scale interaction with the known particles, and mass in the GeV to 10's of GeV range. Hints of light WIMPs have appeared in several dark matter searches in the last decade. The…

High Energy Physics - Phenomenology · Physics 2017-12-13 Graciela B. Gelmini

Nuclear Spin in Direct Dark Matter Search

The Weakly Interacting Massive Particles (WIMPs) are among the main candidates for the relic dark matter (DM). The idea of the direct DM detection relies on elastic in-dependent (SD) and spin-independent (SI) interaction of WIMPs with…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. A. Bednyakov , F. Simkovic , I. V. Titkova

Studies of the Earth shielding effect to direct dark matter searches at the China Jinping Underground Laboratory

Dark matter direct detection experiments mostly operate at deep underground laboratories. It is necessary to consider shielding effect of the Earth, especially for dark matter particles interacting with a large cross section. We analyzed…

High Energy Physics - Experiment · Physics 2022-03-10 Z. Z. Liu , L. T. Yang , Q. Yue , C. H. Yeh , K. J. Kang , Y. J. Li , M. Agartioglu , H. P. An , J. P. Chang , J. H. Chen , Y. H. Chen , J. P. Cheng , W. H. Dai , Z. Deng , C. H. Fang , X. P. Geng , H. Gong , X. Y. Guo , Q. J. Guo , L. He , S. M. He , J. W. Hu , H. X. Huang , T. C. Huang , H. T. Jia , X. Jiang , H. B. Li , J. M. Li , J. Li , R. M. J. Li , X. Q. Li , Y. L. Li , B. Liao , F. K. Lin , S. T. Lin , S. K. Liu , Y. Liu , Y. D. Liu , Y. Y. Liu , H. Ma , Y. C. Mao , Q. Y. Nie , J. H. Ning , H. Pan , N. C. Qi , J. Ren , X. C. Ruan , K. Saraswat , V. Sharma , Z. She , M. K. Singh , T. X. Sun , C. J. Tang , W. Y. Tang , Y. Tian , G. F. Wang , L. Wang , Q. Wang , Y. Wang , Y. X. Wang , Z. Wang , H. T. Wong , S. Y. Wu , Y. C. Wu , H. Y. Xing , Y. Xu , T. Xue , Y. L. Yan , N. Yi , C. X. Yu , H. J. Yu , J. F. Yue , M. Zeng , Z. Zeng , B. T. Zhang , F. S. Zhang , Z. H. Zhang , Z. Y. Zhang , K. K. Zhao , M. G. Zhao , J. F. Zhou , Z. Y. Zhou , J. J. Zhu

Projected WIMP sensitivity of the LUX-ZEPLIN (LZ) dark matter experiment

LUX-ZEPLIN (LZ) is a next generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. Using a two-phase xenon detector with an…

Instrumentation and Methods for Astrophysics · Physics 2021-11-19 D. S. Akerib , C. W. Akerlof , S. K. Alsum , H. M. Araújo , M. Arthurs , X. Bai , A. J. Bailey , J. Balajthy , S. Balashov , D. Bauer , J. Belle , P. Beltrame , T. Benson , E. P. Bernard , T. P. Biesiadzinski , K. E. Boast , B. Boxer , P. Brás , J. H. Buckley , V. V. Bugaev , S. Burdin , J. K. Busenitz , C. Carels , D. L. Carlsmith , B. Carlson , M. C. Carmona-Benitez , C. Chan , J. J. Cherwinka , A. Cole , A. Cottle , W. W. Craddock , A. Currie , J. E. Cutter , C. E. Dahl , L. de Viveiros , A. Dobi , J. E. Y. Dobson , E. Druszkiewicz , T. K. Edberg , W. R. Edwards , A. Fan , S. Fayer , S. Fiorucci , T. Fruth , R. J. Gaitskell , J. Genovesi , C. Ghag , M. G. D. Gilchriese , M. G. D. van der Grinten , C. R. Hall , S. Hans , K. Hanzel , S. J. Haselschwardt , S. A. Hertel , S. Hillbrand , C. Hjemfelt , M. D. Hoff , J. Y-K. Hor , D. Q. Huang , C. M. Ignarra , W. Ji , A. C. Kaboth , K. Kamdin , J. Keefner , D. Khaitan , A. Khazov , Y. D. Kim , C. D. Kocher , E. V. Korolkova , H. Kraus , H. J. Krebs , L. Kreczko , B. Krikler , V. A. Kudryavtsev , S. Kyre , J. Lee , B. G. Lenardo , D. S. Leonard , K. T. Lesko , C. Levy , J. Li , J. Liao , F. -T. Liao , J. Lin , A. Lindote , R. Linehan , W. H. Lippincott , X. Liu , M. I. Lopes , B. López Paredes , W. Lorenzon , S. Luitz , J. M. Lyle , P. Majewski , A. Manalaysay , R. L. Mannino , C. Maupin , D. N. McKinsey , Y. Meng , E. H. Miller , J. Mock , M. E. Monzani , J. A. Morad , E. Morrison , B. J. Mount , A. St. J. Murphy , H. N. Nelson , F. Neves , J. Nikoleyczik , K. O'Sullivan , I. Olcina , M. A. Olevitch , K. C. Oliver-Mallory , K. J. Palladino , S. J. Patton , E. K. Pease , B. Penning , A. Piepke , S. Powell , R. M. Preece , K. Pushkin , B. N. Ratcliff , J. Reichenbacher , C. A. Rhyne , A. Richards , J. P. Rodrigues , R. Rosero , P. Rossiter , J. S. Saba , M. Sarychev , R. W. Schnee , M. Schubnell , P. R. Scovell , S. Shaw , T. A. Shutt , J. J. Silk , C. Silva , K. Skarpaas , W. Skulski , M. Solmaz , V. N. Solovov , P. Sorensen , I. Stancu , M. R. Stark , T. M. Stiegler , K. Stifter , M. Szydagis , W. C. Taylor , R. Taylor , D. J. Taylor , D. Temples , P. A. Terman , K. J. Thomas , M. Timalsina , W. H. To , A. Tomás , T. E. Tope , M. Tripathi , C. E. Tull , L. Tvrznikova , U. Utku , J. Va'vra , A. Vacheret , J. R. Verbus , E. Voirin , W. L. Waldron , J. R. Watson , R. C. Webb , D. T. White , T. J. Whitis , W. J. Wisniewski , M. S. Witherell , F. L. H. Wolfs , D. Woodward , S. D. Worm , M. Yeh , J. Yin , I. Young

Exclusion Limits on the WIMP-Nucleon Cross-Section from the Cryogenic Dark Matter Search

The Cryogenic Dark Matter Search (CDMS) employs Ge and Si detectors to search for WIMPs via their elastic-scattering interactions with nuclei while discriminating against interactions of background particles. CDMS data give limits on the…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

Development of new ultra-low-background particle detectors based on Micromegas technology for the search of Dark Matter at the low-mass frontier

Weakly Interacting Massive Particles (WIMPs) are one of the best motivated candidates to compose the Dark Matter of the Universe. The lack of experimental confirmation by direct detection experiments or collider searches has ruled out…

Instrumentation and Detectors · Physics 2025-07-04 Oscar Perez

The Direct and Indirect Detection of Weakly Interacting Dark Matter Particles

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

How well will ton-scale dark matter direct detection experiments constrain minimal supersymmetry?

Weakly interacting massive particles (WIMPs) are amongst the most interesting dark matter (DM) candidates. Many DM candidates naturally arise in theories beyond the standard model (SM) of particle physics, like weak-scale supersymmetry…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 Yashar Akrami , Christopher Savage , Pat Scott , Jan Conrad , Joakim Edsjö

The XENON Dark Matter Experiment

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 Xenon nuclei. With a fiducial mass of 1000 kg of liquid xenon, a sufficiently low…

Astrophysics · Physics 2007-05-23 XENON Collaboration , Elena Aprile

The Present and Future of Searching for Dark Matter with LUX and LZ

The LUX collaboration new results advance the search for dark matter candidate particles in the 4 GeV/c^2 and higher mass range, with a maximal spin-independent 90% C.L. limit of 2 x 10^-46 cm^2 at 50 GeV/c^2 for its 332 live-day run,…

Cosmology and Nongalactic Astrophysics · Physics 2019-08-15 M. Szydagis

Exclusion Limits on the WIMP-Nucleon Cross-Section from the First Run of the Cryogenic Dark Matter Search in the Soudan Underground Lab

The Cryogenic Dark Matter Search (CDMS-II) employs low-temperature Ge and Si detectors to seek Weakly Interacting Massive Particles (WIMPs) via their elastic scattering interactions with nuclei. Simultaneous measurements of both ionization…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

Deep Underground Science and Engineering Lab: S1 Dark Matter Working Group

A study of the current status of WIMP dark matter searches has been made in the context of scientific and technical planning for a Deep Underground Science and Engineering Laboratory (DUSEL) in the U.S. The table of contents follows: 1.…

Astrophysics · Physics 2009-09-29 D. S. Akerib , E. Aprile , E. A. Baltz , M. R. Dragowsky , R. J. Gaitskell , P. Gondolo , A. Hime , C. J. Martoff , D. -M. Mei , H. Nelson , B. Sadoulet , R. W. Schnee , A. H. Sonnenschein , L. E. Strigari

Direct Detection of Nonbaryonic Dark Matter

Weakly Interacting Massive Particles (WIMPs) are leading candidates for the dominant part of the mass density of the Universe. Here we will review direct WIMP detection techniques by giving examples of currently running experiments, and…

Astrophysics · Physics 2007-05-23 Laura Baudis , H. V. Klapdor-Kleingrothaus

Direct dark matter detection: the next decade

Direct dark matter searches are promising techniques to identify the nature of dark matter particles. I describe the future of this field of research, focussing on the question of what can be achieved in the next decade. I will present the…

Instrumentation and Methods for Astrophysics · Physics 2012-12-04 Laura Baudis

Latest results of the direct dark matter search with the EDELWEISS-II experiment

The EDELWEISS-II experiment uses cryogenic heat-and-ionization Germanium detectors in order to detect the rare interactions from WIMP dark matter particles of local halo. New-generation detec- tors with an interleaved electrode geometry…

Cosmology and Nongalactic Astrophysics · Physics 2010-12-13 Gilles Gerbier , for EDELWEISS collaboration

Dark Matter Evidence, Particle Physics Candidates and Detection Methods

The problem of the dark matter in the universe is reviewed. A short history of the subject is given, and several of the most obvious particle candidates for dark matter are identified. Particular focus is given to weakly interacting,…

High Energy Astrophysical Phenomena · Physics 2012-06-15 Lars Bergström

New class of biological detectors for WIMPs

Weakly Interacting Massive Particles (WIMPs) may constitute a large fraction of the matter in the Universe. There are excess events in the data of DAMA/LIBRA, CoGeNT, CRESST-II, and recently CDMS-Si, which could be consistent with WIMP…

Instrumentation and Methods for Astrophysics · Physics 2015-07-03 Andrzej K. Drukier , Charles Cantor , Mark Chonofsky , George M. Church , Robert L. Fagaly , Katherine Freese , Alejandro Lopez , Takeshi Sano , Christopher Savage , Wesley P. Wong

The Direct and Indirect Detection of Weakly Interacting Dark Matter Particles

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

Astrophysics · Physics 2007-05-23 F. Halzen

Constraints on ultraheavy dark matter from the CDEX-10 experiment at the China Jinping Underground Laboratory

We report a search for ultraheavy dark matter (UHDM) with the CDEX-10 experiment at the China Jinping Underground Laboratory. Using a Monte Carlo framework that incorporates Earth shielding effects, we simulated UHDM propagation and energy…

High Energy Physics - Experiment · Physics 2026-03-31 Y. F. Wang , L. T. Yang , Q. Yue , K. J. Kang , Y. J. Li , H. P. An , Greeshma C. , J. P. Chang , H. Chen , Y. H. Chen , J. P. Cheng , J. Y. Cui , W. H. Dai , Z. Deng , Y. X. Dong , C. H. Fang , H. Gong , Q. J. Guo , T. Guo , X. Y. Guo , L. He , J. R. He , H. X. Huang , T. C. Huang , S. Karmakar , Y. S. Lan , H. B. Li , H. Y. Li , J. M. Li , J. Li , M. C. Li , Q. Y. Li , R. M. J. Li , X. Q. Li , Y. L. Li , Y. F. Liang , B. Liao , F. K. Lin , S. T. Lin , J. X. Liu , R. Z. Liu , S. K. Liu , Y. D. Liu , Y. Liu , Y. Y. Liu , H. Ma , Y. C. Mao , A. Mureed , H. Pan , N. C. Qi , J. Ren , X. C. Ruan , M. B. Shen , H. Y. Shi , M. K. Singh , T. X. Sun , W. L. Sun , C. J. Tang , Y. Tian , H. F. Wan , G. F. Wang , J. Z. Wang , L. Wang , Q. Wang , Q. Wang , Y. X. Wang , H. T. Wong , Y. C. Wu , H. Y. Xing , K. Z. Xiong , R. Xu , Y. Xu , T. Xue , Y. L. Yan , N. Yi , C. X. Yu , H. J. Yu , X. Yu , M. Zeng , Z. Zeng , F. S. Zhang , P. Zhang , P. Zhang , Z. Y. Zhang , M. G. Zhao , J. F. Zhou , Z. Y. Zhou , J. J. Zhu