English
Related papers

Related papers: TREX-DM: a low background Micromegas-based TPC for…

200 papers

Two germanium detectors are currently operating in the Canfranc Underground Laboratory at 2450 m.w.e looking for WIMP dark matter. One is a 2 kg 76Ge IGEX detector (RG-2) which has an energy threshold of 4 keV and a low-energy background…

The main characteristics of a new concept of spherical gaseous detectors, with some details on its operation are first given. The very low energy threshold of such detector has led to investigations of its potential performance for dark…

Instrumentation and Methods for Astrophysics · Physics 2014-01-31 G. Gerbier , I. Giomataris , P. Magnier , A. Dastgheibi , M. Gros , D. Jourde , E. Bougamont , X. F. Navick , T. Papaevangelou , J. Galan , J. Derre , I. Savvidis , G. Tsiledakis

We explore paleo-detectors as an approach to the direct detection of Weakly Interacting Massive Particle (WIMP) dark matter radically different from conventional detectors. Instead of instrumenting a (large) target mass in a laboratory in…

Cosmology and Nongalactic Astrophysics · Physics 2019-02-28 Andrzej K. Drukier , Sebastian Baum , Katherine Freese , Maciej Górski , Patrick Stengel

We find that it is possible to increase sensitivity to low energy physics in a third or fourth DUNE-like module with careful controls over radiopurity and targeted modifications to a detector similar to the DUNE Far Detector design. In…

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

We present the results of a search for WIMPs from the commissioning run of the PandaX-II experiment located at the China Jinping underground Laboratory. A WIMP search data set with an exposure of 306$\times$19.1 kg-day was taken, while its…

Dark Matter (DM) is one of the most critical questions to be understood and answered in fundamental physics today. Plenty of astronomical and cosmological observations have already pinned down that DM exists in the Universe, the Milky Way,…

Instrumentation and Methods for Astrophysics · Physics 2022-09-13 Junhui Liao , Yuanning Gao , Zhuo Liang , Zebang Ouyang , Zhaohua Peng , Lifeng Zhang , Lei Zhang , Jian Zheng , Jiangfeng Zhou

There is a worldwide effort toward the development of a large TPC (Time Projection Chamber) devoted to directional Dark Matter detection. All current projects are being designed to fulfill a unique goal : identifying weakly interacting…

Cosmology and Nongalactic Astrophysics · Physics 2012-04-12 J. Billard , F. Mayet , D. Santos

A chamber for direct detection of WIMPs with masses < 10 GeV/c2 and solar axions is developed. The chamber is filled with a gas mixture of H2 +3ppm TMAE (1,5,10 bar), or D2 + 3ppm TMAE. These gas fillings make it possible to suppress an…

Instrumentation and Detectors · Physics 2016-03-21 B. M. Ovchinnikov , V. V. Parusov

Rare Objects SEarch with Bolometers UndergrounD) is an experiment which attempts to detect low mass Weak Interacting Massive Particles (WIMPs) through their elastic scattering off Al and O nuclei. It consists of three small sapphire…

We study the sensitivity of multi ton-scale time projection chambers using a liquid xenon target, e.g., the proposed DARWIN instrument, to spin-independent and spin-dependent WIMP-nucleon scattering interactions. Taking into account…

Instrumentation and Detectors · Physics 2015-10-14 Marc Schumann , Laura Baudis , Lukas Bütikofer , Alexander Kish , Marco Selvi

DARk matter WImp search with liquid xenoN (DARWIN) will be an experiment for the direct detection of dark matter using a multi-ton liquid xenon time projection chamber at its core. Its primary goal will be to explore the experimentally…

Instrumentation and Methods for Astrophysics · Physics 2016-12-02 J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , C. Amsler , E. Aprile , L. Arazi , F. Arneodo , P. Barrow , L. Baudis , M. L. Benabderrahmane , T. Berger , B. Beskers , A. Breskin , P. A. Breur , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Buetikofer , J. Calven , J. M. R. Cardoso , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , J. P. Cussonneau , M. P. Decowski , S. Diglio , G. Drexlin , E. Duchovni , E. Erdal , G. Eurin , A. Ferella , A. Fieguth , W. Fulgione , A. Gallo Rosso , P. Di Gangi , A. Di Giovanni , M. Galloway , M. Garbini , C. Geis , F. Glueck , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , V. Hannen , E. Hogenbirk , J. Howlett , D. Hilk , C. Hils , A. James , B. Kaminsky , S. Kazama , B. Kilminster , A. Kish , L. M. Krauss , H. Landsman , R. F. Lang , Q. Lin , F. L. Linde , S. Lindemann , M. Lindner , J. A. M. Lopes , T. Marrodan Undagoitia , J. Masbou , F. V. Massoli , D. Mayani , M. Messina , K. Micheneau , A. Molinario , K. D. Mora , E. Morteau , M. Murra , J. Naganoma , J. L. Newstead , K. Ni , U. Oberlack , P. Pakarha , B. Pelssers , P. de Perio , R. Persiani , F. Piastra , M. C. Piro , G. Plante , L. Rauch , S. Reichard , A. Rizzo , N. Rupp , J. M. F. Dos Santos , G. Sartorelli , M. Scheibelhut , S. Schindler , M. Schumann , J. Schreiner , L. Scotto Lavina , M. Selvi , P. Shagin , M. C. Silva , H. Simgen , P. Sissol , M. von Sivers , D. Thers , J. Thurn , A. Tiseni , R. Trotta , C. D. Tunnell , K. Valerius , M. A. Vargas , H. Wang , Y. Wei , C. Weinheimer , T. Wester , J. Wulf , Y. Zhang , T. Zhu , K. Zuber

Dark Matter particles are commonly assumed to be weakly interacting massive particles (WIMPs) with a mass in the GeV to TeV range. However, recent interest has shifted towards lighter WIMPs, which are more difficult to probe experimentally.…

Using information from a recent dark matter symposium at Marina del Rey and from various publications in 2012 and 2013, we discuss the most recent evidence and constraints on low mass WIMPs. There are now five separate experimental limits…

High Energy Physics - Experiment · Physics 2013-08-16 David Cline

The DAMIC experiment uses fully depleted, high resistivity CCDs to search for dark matter particles. With an energy threshold $\sim$50 eV$_{ee}$, and excellent energy and spatial resolutions, the DAMIC CCDs are well-suited to identify and…

Dual-phase time projection chambers (TPCs) filled with the liquid noble gas xenon (LXe) are currently the most sensitive detectors searching for interactions of WIMP dark matter in a laboratory-based experiment. This is achieved by…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Marc Schumann

The chamber for direct detection of WIMP with mass <0.5 Gev/c2 was developed. The chamber is filled with gas mixture Ne+10%H2 (0-1bar)+0,15ppm Ge(CH3)4. For events detection used GEM+pin-anodes , which provides the energy threshold about…

Instrumentation and Methods for Astrophysics · Physics 2015-12-04 B. M. Ovchinnikov , I. I. Tkachev , V. V. Parusov

We report first results from the Cryogenic Dark Matter Search (CDMS II) experiment running with its full complement of 30 cryogenic particle detectors at the Soudan Underground Laboratory. This report is based on the analysis of data…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

The XENON1T experiment at the Laboratori Nazionali del Gran Sasso (LNGS) is the first WIMP dark matter detector operating with a liquid xenon target mass above the ton-scale. Out of its 3.2t liquid xenon inventory, 2.0t constitute the…

Instrumentation and Methods for Astrophysics · Physics 2018-06-13 XENON Collaboration , E. Aprile , J. Aalbers , F. Agostini , M. Alfonsi , F. D. Amaro , M. Anthony , B. Antunes , F. Arneodo , M. Balata , P. Barrow , L. Baudis , B. Bauermeister , M. L. Benabderrahmane , T. Berger , A. Breskin , P. A. Breur , A. Brown , E. Brown , S. Bruenner , G. Bruno , R. Budnik , L. Bütikofer , J. Calvén , J. M. R. Cardoso , M. Cervantes , A. Chiarini , D. Cichon , D. Coderre , A. P. Colijn , J. Conrad , R. Corrieri , J. P. Cussonneau , M. P. Decowski , P. de Perio , P. Di Gangi , A. Di Giovanni , S. Diglio , J. -M. Disdier , M. Doets , E. Duchovni , G. Eurin , J. Fei , A. D. Ferella , A. Fieguth , D. Florin , D. Front , W. Fulgione , A. Gallo Rosso , M. Galloway , F. Gao , M. Garbini , C. Geis , K. -L. Giboni , L. W. Goetzke , L. Grandi , Z. Greene , C. Grignon , C. Hasterok , E. Hogenbirk , C. Huhmann , R. Itay , A. James , 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 , R. Maier , 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 , D. Orlandi , R. Othegraven , P. Pakarha , S. Parlati , 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 , S. Rosendahl , N. Rupp , J. M. F. dos Santos , R. Saldahna , G. Sartorelli , M. Scheibelhut , S. Schindler , J. Schreiner , M. Schumann , L. Scotto Lavina , M. Selvi , P. Shagin , E. Shockley , M. Silva , H. Simgen , M. v. Sivers , M. Stern , A. Stein , D. Tatananni , L. Tatananni , D. Thers , A. Tiseni , G. Trinchero , C. Tunnell , N. Upole , M. Vargas , O. Wack , R. Walet , H. Wang , Z. Wang , Y. Wei , C. Weinheimer , C. Wittweg , J. Wulf , J. Ye , Y. Zhang

This mini-review first introduces the motivations for Dark Matter Searches. The experimental aspect of the direct detection of Weakly Interactive Massive Particles (WIMPs) is described, detailing its principle and presenting some…

Astrophysics · Physics 2019-08-14 V. Sanglard
‹ Prev 1 4 5 6 7 8 10 Next ›