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Recently low-mass dark matter direct searches have been hindered by a low energy background, drastically reducing the physics reach of the experiments. In the CRESST-III experiment, this signal is characterised by a significant increase of…

In CRESST-III, 10 cryogenic detector modules optimized for low energy thresholds were operated for almost two years (May 2016 - February 2018). Together with this document we are publishing data from the best performing detector module…

The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased…

Many low-threshold experiments observe sharply rising event rates of yet unknown origins below a few hundred eV, and larger than expected from known backgrounds. Due to the significant impact of this excess on the dark matter or neutrino…

天体物理仪器与方法 · 物理学 2022-09-07 P. Adari , A. Aguilar-Arevalo , D. Amidei , G. Angloher , E. Armengaud , C. Augier , L. Balogh , S. Banik , D. Baxter , C. Beaufort , G. Beaulieu , V. Belov , Y. Ben Gal , G. Benato , A. Benoît , A. Bento , L. Bergé , A. Bertolini , R. Bhattacharyya , J. Billard , I. M. Bloch , A. Botti , R. Breier , G. Bres , J-. L. Bret , A. Broniatowski , A. Brossard , C. Bucci , R. Bunker , M. Cababie , M. Calvo , P. Camus , G. Cancelo , L. Canonica , F. Cappella , L. Cardani , J. -F. Caron , N. Casali , G. del Castello , A. Cazes , R. Cerulli , B. A. Cervantes Vergara , D. Chaize , M. Chapellier , L. Chaplinsky , F. Charlieux , M. Chaudhuri , A. E. Chavarria , G. Chemin , R. Chen , H. Chen , F. Chierchie , I. Colantoni , J. Colas , J. Cooley , J. -M. Coquillat , E. C. Corcoran , S. Crawford , M. Crisler , A. Cruciani , P. Cushman , A. D'Addabbo , J. C. D'Olivo , A. Dastgheibi-Fard , M. De Jésus , Y. Deng , J. B. Dent , E. L. Depaoli , K. Dering , S. Dharani , S. Di Lorenzo , A. Drlica-Wagner , L. Dumoulin , D. Durnford , B. Dutta , L. Einfalt , A. Erb , A. Erhart , R. Essig , J. Estrada , E. Etzion , O. Exshaw , F. Favela-Perez , F. v. Feilitzsch , G. Fernandez Moroni , N. Ferreiro Iachellini , S. Ferriol , S. Fichtinger , E. Figueroa-Feliciano , J. -B. Filippini , D. Filosofov , J. A. Formaggio , M. Friedl , S. Fuard , D. Fuchs , A. Fuss , R. Gaïor , A. Garai , C. Garrah , J. Gascon , G. Gerbier , M. Ghaith , V. M. Ghete , D. Gift , I. Giomataris , G. Giroux , A. Giuliani , P. Gorel , P. Gorla , C. Goupy , J. Goupy , C. Goy , M. Gros , P. Gros , Y. Guardincerri , C. Guerin , V. Guidi , O. Guillaudin , S. Gupta , E. Guy , P. Harrington , D. Hauff , S. T. Heine , S. A. Hertel , S. E. Holland , Z. Hong , E. W. Hoppe , T. W. Hossbach , J. -C. Ianigro , V. Iyer , A. Jastram , M. Ješkovský , Y. Jin , J. Jochum , J. P. Johnston , A. Juillard , D. Karaivanov , V. Kashyap , I. Katsioulas , S. Kazarcev , M. Kaznacheeva , F. Kelly , B. Kilminster , A. Kinast , L. Klinkenberg , H. Kluck , P. Knights , Y. Korn , H. Kraus , B. von Krosigk , A. Kubik , N. A. Kurinsky , J. Lamblin , A. Langenkämper , S. Langrock , T. Lasserre , H. Lattaud , P. Lautridou , I. Lawson , S. J. Lee , M. Lee , A. Letessier-Selvon , D. Lhuillier , M. Li , Y. -T. Lin , A. Lubashevskiy , R. Mahapatra , S. Maludze , M. Mancuso , I. Manthos , L. Marini , S. Marnieros , R. D. Martin , A. Matalon , J. Matthews , B. Mauri , D. W. Mayer , A. Mazzolari , E. Mazzucato , H. Meyer zu Theenhausen , E. Michielin , J. Minet , N. Mirabolfathi , K. v. Mirbach , D. Misiak , P. Mitra , J-. L. Mocellin , B. Mohanty , V. Mokina , J. -P. Mols , A. Monfardini , F. Mounier , S. Munagavalasa , J. -F. Muraz , X. -F. Navick , T. Neep , H. Neog , H. Neyrial , K. Nikolopoulos , A. Nilima , C. Nones , V. Novati , P. O'Brien , L. Oberauer , E. Olivieri , M. Olmi , A. Onillon , C. Oriol , A. Orly , J. L. Orrell , T. Ortmann , C. T. Overman , C. Pagliarone , V. Palušová , P. Pari , P. K. Patel , L. Pattavina , F. Petricca , A. Piers , H. D. Pinckney , M. -C. Piro , M. Platt , D. Poda , D. Ponomarev , W. Potzel , P. Povinec , F. Pröbst , P. Privitera , F. Pucci , K. Ramanathan , J. -S. Real , T. Redon , F. Reindl , R. Ren , A. Robert , J. Da Rocha , D. Rodrigues , R. Rogly , J. Rothe , N. Rowe , S. Rozov , I. Rozova , T. Saab , N. Saffold , T. Salagnac , J. Sander , V. Sanglard , D. Santos , Y. Sarkis , V. Savu , G. Savvidis , I. Savvidis , S. Schönert , K. Schäffner , N. Schermer , J. Schieck , B. Schmidt , D. Schmiedmayer , C. Schwertner , L. Scola , M. Settimo , Ye. Shevchik , V. Sibille , I. Sidelnik , A. Singal , R. Smida , M. Sofo Haro , T. Soldner , J. Stachurska , M. Stahlberg , L. Stefanazzi , L. Stodolsky , C. Strandhagen , R. Strauss , A. Stutz , R. Thomas , A. Thompson , J. Tiffenberg , C. Tomei , M. Traina , S. Uemura , I. Usherov , L. Vagneron , W. Van De Pontseele , F. A. Vazquez de Sola Fernandez , M. Vidal , M. Vignati , A. L. Virto , M. Vivier , T. Volansky , V. Wagner , F. Wagner , J. Walker , R. Ward , S. L. Watkins , A. Wex , M. Willers , M. J. Wilson , L. Winslow , E. Yakushev , T. -T. Yu , M. Zampaolo , A. Zaytsev , V. Zema , D. Zinatulina , A. Zolotarova

The CRESST-III experiment which is dedicated to low-mass dark matter search uses scintillating CaWO$_4$ crystals operated as cryogenic particle detectors. Background discrimination is achieved by exploiting the scintillating light signal of…

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,…

CRESST is a multi-stage experiment directly searching for dark matter (DM) using cryogenic $\mathrm{CaWO_4}$ crystals. Previous stages established leading limits for the spin-independent DM-nucleon cross section down to DM-particle masses…

The CRESST experiment seeks hypothetical WIMP particles that could account for the bulk of dark matter in the Universe. The detectors are cryogenic calorimeters in which WIMPs would scatter elastically on nuclei, releasing phonons. The…

Direct detection experiments have established the most stringent constraints on potential interactions between particle candidates for relic, thermal dark matter and Standard Model particles. To surpass current exclusion limits a new…

Recent experiments searching for sub-GeV/$c^2$ dark matter have observed event excesses close to their respective energy thresholds. Although specific to the individual technologies, the measured excess event rates have been consistently…

高能物理 - 实验 · 物理学 2022-10-12 SuperCDMS Collaboration , M. F. Albakry , I. Alkhatib , D. W. P. Amaral , T. Aralis , T. Aramaki , I. J. Arnquist , I. Ataee Langroudy , E. Azadbakht , S. Banik , C. Bathurst , D. A. Bauer , R. Bhattacharyya , P. L. Brink , R. Bunker , B. Cabrera , R. Calkins , R. A. Cameron , C. Cartaro , D. G. Cerdeño , Y. -Y. Chang , M. Chaudhuri , R. Chen , N. Chott , J. Cooley , H. Coombes , J. Corbett , P. Cushman , F. De Brienne , S. Dharani , M. L. di Vacri , M. D. Diamond , E. Fascione , E. Figueroa-Feliciano , C. W. Fink , K. Fouts , M. Fritts , G. Gerbier , R. Germond , M. Ghaith , S. R. Golwala , J. Hall , N. Hassan , B. A. Hines , M. I. Hollister , Z. Hong , E. W. Hoppe , L. Hsu , M. E. Huber , V. Iyer , A. Jastram , V. K. S. Kashyap , M. H. Kelsey , A. Kubik , N. A. Kurinsky , R. E. Lawrence , M. Lee , A. Li , J. Liu , Y. Liu , B. Loer , E. Lopez Asamar , P. Lukens , D. B. MacFarlane , R. Mahapatra , V. Mandic , N. Mast , A. J. Mayer , H. Meyer zu Theenhausen , É. Michaud , E. Michielin , N. Mirabolfathi , B. Mohanty , S. Nagorny , J. Nelson , H. Neog , V. Novati , J. L. Orrell , M. D. Osborne , S. M. Oser , W. A. Page , R. Partridge , D. S. Pedreros , R. Podviianiuk , F. Ponce , S. Poudel , A. Pradeep , M. Pyle , W. Rau , E. Reid , R. Ren , T. Reynolds , A. Roberts , A. E. Robinson , T. Saab , B. Sadoulet , I. Saikia , J. Sander , A. Sattari , B. Schmidt , R. W. Schnee , S. Scorza , B. Serfass , S. S. Poudel , D. J. Sincavage , C. Stanford , J. Street , H. Sun , F. K. Thasrawala , D. Toback , R. Underwood , S. Verma , A. N. Villano , B. von Krosigk , S. L. Watkins , O. Wen , Z. Williams , M. J. Wilson , J. Winchell , K. Wykoff , S. Yellin , B. A. Young , T. C. Yu , B. Zatschler , S. Zatschler , A. Zaytsev , E. Zhang , L. Zheng , S. Zuber

The search for dark matter, the missing mass of the Universe, is one of the most active fields of study within particle physics. The XENON1T experiment recently observed a 3.5$\sigma$ excess potentially consistent with dark matter, or with…

高能物理 - 实验 · 物理学 2021-01-13 M. Szydagis , C. Levy , G. M. Blockinger , A. Kamaha , N. Parveen , G. R. C. Rischbieter

We present a novel unifying interpretation of excess event rates observed in several dark matter direct-detection experiments that utilize single-electron threshold semiconductor detectors. Despite their different locations, exposures,…

高能物理 - 唯象学 · 物理学 2020-07-29 Noah Kurinsky , Daniel Baxter , Yonatan Kahn , Gordan Krnjaic

Two detector modules with lithium aluminate targets were operated in the CRESST underground setup between February and June 2021. The data collected in this period was used to set the currently strongest cross-section upper limits on the…

In the recent years, many low-threshold dark matter (DM) direct detection experiments have reported the observation of unexplained excesses of events at low energies. Exemplary for these, the experiment CRESST has detected unidentified…

高能物理 - 唯象学 · 物理学 2022-02-23 Riccardo Catena , Vanessa Zema

The CRESST experiment monitors 300g CaWO_4 crystals as targets for particle interactions in an ultra low background environment. In this paper, we analyze the background spectra that are recorded by three detectors over many weeks of data…

The CRESST experiment (Cryogenic Rare Event Search with Superconducting Thermometers) searches for dark matter via the phonon and light signals of elastic scattering processes in scintillating crystals. The discrimination between a possible…

The CRESST-II experiment uses cryogenic detectors to search for nuclear recoil events induced by the elastic scattering of dark matter particles in CaWO$_4$ crystals. Given the low energy threshold of our detectors in combination with light…

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