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The CRESST experiment, located at Laboratori Nazionali del Gran Sasso in Italy, searches for dark matter particles via their elastic scattering off nuclei in a target material. The CRESST target consists of scintillating CaWO$_4$ crystals,…

The Cryogenic Dark Matter Search experiment (CDMS) employs low-temperature Ge and Si detectors to detect WIMPs via their elastic scattering interaction with the target nuclei. The current analysis of 397.8 kg-days Ge exposure resulted in…

天体物理学 · 物理学 2019-08-13 T. Bruch

The new detection concept applied for the direct WIMP search experiment CRESST II, which enables a clear discrimination between electron recoils and nuclear recoils, will leave neutrons as the main background. This background will soon…

高能物理 - 实验 · 物理学 2007-05-23 H. Wulandari , J. Jochum , W. Rau , F. von Feilitzsch

We present first competitive results on WIMP dark matter using the phonon-light-detection technique. A particularly strong limit for WIMPs with coherent scattering results from selecting a region of the phonon-light plane corresponding to…

The purpose of this document is to describe the upgrade of the CRESST dark matter search at LNGS. The proposed strategy will allow to explore a region of the parameter space for spin-independent WIMP-nucleon elastic scattering corresponding…

CRESST is a direct dark matter search experiment, aiming for an observation of nuclear recoils induced by the interaction of dark matter particles with cryogenic scintillating calcium tungstate crystals. Instead of confining ourselves to…

The EDELWEISS-II experiment uses cryogenic heat-and-ionization detectors in order to detect the rare interactions from possible WIMP dark matter particles on Germanium nuclei. Recently, new-generation detectors with an interleaved electrode…

宇宙学与河外天体物理 · 物理学 2019-08-13 E. Armengaud

The EDELWEISS-II collaboration has performed a direct search for WIMP dark matter with an array of ten 400 g heat-and-ionization cryogenic detectors equipped with interleaved electrodes for the rejection of near-surface events. Six months…

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…

宇宙学与河外天体物理 · 物理学 2010-12-13 Gilles Gerbier , for EDELWEISS collaboration

The SIMPLE project uses superheated C2ClF5 liquid detectors to search for particle dark matter candidates. We report the results of the first stage exposure (14.1 kgd) of its latest two-stage, Phase II run, with 15 superheated droplet…

宇宙学与河外天体物理 · 物理学 2011-01-11 TA Girard , T. A. Morlat , M. Felizardo , A. C. Fernandes , A. R. Ramos , J. G. Marques

Cryogenic calorimetric experiments to search for neutrinoless double-beta decay ($0\nu\beta\beta$) are highly competitive, scalable and versatile in isotope. The largest planned detector array, CUPID, is comprised of about 1500 individual…

The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

The CRESST-II collaboration have announced evidence for the direct detection of dark matter in 730 kg-days exposure of a CaWO$_4$ target. We examine these new results, along with DAMA and CoGeNT data, in the context of the mirror dark…

高能物理 - 唯象学 · 物理学 2015-06-04 R. Foot

The CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) and the EURECA (European Underground Rare Event Calorimeter Array) experiments are direct dark matter search experiments where cryogenic detectors are used to detect…

高能物理 - 唯象学 · 物理学 2008-12-18 S. Roth , C. Ciemniak , C. Coppi , F. v. Feilitzsch , A. Guetlein , C. Isaila , J. -C. Lanfranchi , S. Pfister , W. Potzel , W. Westphal

Most experiments that search for direct interactions of WIMP dark matter with a target can distinguish the dominant electronrecoil background from the nuclear recoil signal, based on some discrimination parameter. An acceptance region is…

天体物理仪器与方法 · 物理学 2009-11-06 Rafael F. Lang

The CUPID Collaboration is designing a tonne-scale, background-free detector to search for double beta decay with sufficient sensitivity to fully explore the parameter space corresponding to the inverted neutrino mass hierarchy scenario.…

仪器与探测器 · 物理学 2020-11-30 A. Armatol , E. Armengaud , W. Armstrong , C. Augier , F. T. Avignone , O. Azzolini , A. Barabash , G. Bari , A. Barresi , D. Baudin , F. Bellini , G. Benato , M. Beretta , L. Bergè , M. Biassoni , J. Billard , V. Boldrini , A. Branca , C. Brofferio , C. Bucci , J. Camilleri , S. Capelli , L. Cappelli , L. Cardani , P. Carniti , N. Casali , A. Cazes , E. Celi , C. Chang , M. Chapellier , A. Charrier , D. Chiesa , M. Clemenza , I. Colantoni , F. Collamati , S. Copello , F. Cova , O. Cremonesi , R. J. Creswick , A. Cruciani , A. D'Addabbo , G. D'Imperio , I. Dafinei , F. A. Danevich , M. de Combarieu , M. De Jesus , P. de Marcillac , S. Dell'Oro , S. Di Domizio , V. Dompé , A. Drobizhev , L. Dumoulin , G. Fantini , M. Fasoli , M. Faverzani , E. Ferri , F. Ferri , F. Ferroni , E. Figueroa-Feliciano , J. Formaggio , A. Franceschi , C. Fu , S. Fu , B. K. Fujikawa , J. Gascon , A. Giachero , L. Gironi , A. Giuliani , P. Gorla , C. Gotti , P. Gras , M. Gros , T. D. Gutierrez , K. Han , E. V. Hansen , K. M. Heeger , D. L. Helis , H. Z. Huang , R. G. Huang , L. Imbert , J. Johnston , A. Juillard , G. Karapetrov , G. Keppel , H. Khalife , V. V. Kobychev , Yu. G. Kolomensky , S. Konovalov , Y. Liu , P. Loaiza , L. Ma , M. Madhukuttan , F. Mancarella , R. Mariam , L. Marini , S. Marnieros , M. Martinez , R. H. Maruyama , B. Mauri , D. Mayer , Y. Mei , S. Milana , D. Misiak , T. Napolitano , M. Nastasi , X. F. Navick , J. Nikkel , R. Nipoti , S. Nisi , C. Nones , E. B. Norman , V. Novosad , I. Nutini , T. O'Donnell , E. Olivieri , C. Oriol , J. L. Ouellet , S. Pagan , C. Pagliarone , L. Pagnanini , P. Pari , L. Pattavina , B. Paul , M. Pavan , H. Peng , G. Pessina , V. Pettinacci , C. Pira , S. Pirro , D. V. Poda , T. Polakovic , O. G. Polischuk , S. Pozzi , E. Previtali , A. Puiu , A. Ressa , R. Rizzoli , C. Rosenfeld , C. Rusconi , V. Sanglard , J. A. Scarpaci , B. Schmidt , V. Sharma , V. Shlegel , V. Singh , M. Sisti , D. Speller , P. T. Surukuchi , L. Taffarello , O. Tellier , C. Tomei , V. I. Tretyak , A. Tsymbaliuk , A. Vedda , M. Velazquez , K. J. Vetter , S. L. Wagaarachchi , G. Wang , L. Wang , B. Welliver , J. Wilson , K. Wilson , L. A. Winslow , M. Xue , L. Yan , J. Yang , V. Yefremenko , V. Yumatov , M. M. Zarytskyy , J. Zhang , A. Zolotarova , S. Zucchelli

The usual assumption in direct dark matter searches is to only consider the spin-dependent or spin-independent scattering of dark matter particles. However, especially in models with light dark matter particles…