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Related papers: Neutron Background Studies for the CRESST Dark Mat…

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A direct WIMP (Weakly Interacting Massive Particle) detector with a neutron veto system is designed to better reject neutrons. An experimental configuration is studied in the present paper: a WIMP detectors with CsI(Na) target is placed…

Instrumentation and Methods for Astrophysics · Physics 2015-06-18 Ye Xu , Xiangpan Ji , Haolin Li , Yulong Feng

Nuclear recoil events produced by neutron scatters form one of the most important classes of background in WIMP direct detection experiments, as they may produce nuclear recoils that look exactly like WIMP interactions. In DarkSide-50, we…

Instrumentation and Detectors · Physics 2017-02-06 The DarkSide Collaboration , P. Agnes , L. Agostino , I. F. M. Albuquerque , T. Alexander , A. K. Alton , K. Arisaka , H. O. Back , B. Baldin , K. Biery , G. Bonfini , M. Bossa , B. Bottino , A. Brigatti , J. Brodsky , F. Budano , S. Bussino , M. Cadeddu , L. Cadonati , M. Cadoni , F. Calaprice , N. Canci , A. Candela , H. Cao , M. Cariello , M. Carlini , S. Catalanotti , P. Cavalcante , A. Chepurnov , A. G. Cocco , G. Covone , L. Crippa , D. D'Angelo , M. D'Incecco , S. Davini , S. De Cecco , M. De Deo , M. De Vincenzi , A. Derbin , A. Devoto , F. Di Eusanio , G. Di Pietro , E. Edkins , A. Empl , A. Fan , G. Fiorillo , K. Fomenko , G. Foster , D. Franco , F. Gabriele , C. Galbiati , C. Giganti , A. M. Goretti , F. Granato , L. Grandi , M. Gromov , M. Guan , Y. Guardincerri , B. R. Hackett , K. R. Herner , E. V. Hungerford , Aldo Ianni , Andrea Ianni , I. James , T. Johnson , C. Jollet , K. Keeter , C. L. Kendziora , V. Kobychev , G. Koh , D. Korablev , G. Korga , A. Kubankin , X. Li , M. Lissia , P. Lombardi , S. Luitz , Y. Ma , I. N. Machulin , A. Mandarano , S. M. Mari , J. Maricic , L. Marini , C. J. Martoff , A. Meregaglia , P. D. Meyers , T. Miletic , R. Milincic , D. Montanari , A. Monte , M. Montuschi , M. E. Monzani , P. Mosteiro , B. J. Mount , V. N. Muratova , P. Musico , J. Napolitano , A. Nelson , S. Odrowski , M. Orsini , F. Ortica , L. Pagani , M. Pallavicini , E. Pantic , S. Parmeggiano , K. Pelczar , N. Pelliccia , S. Perasso , A. Pocar , S. Pordes , D. A. Pugachev , H. Qian , K. Randle , G. Ranucci , A. Razeto , B. Reinhold , A. L. Renshaw , A. Romani , B. Rossi , N. Rossi , S. D. Rountree , D. Sablone , P. Saggese , R. Saldanha , W. Sands , S. Sangiorgio , C. Savarese , E. Segreto , D. A. Semenov , E. Shields , P. N. Singh , M. D. Skorokhvatov , O. Smirnov , A. Sotnikov , C. Stanford , Y. Suvorov , R. Tartaglia , J. Tatarowicz , G. Testera , A. Tonazzo , P. Trinchese , E. V. Unzhakov , A. Vishneva , B. Vogelaar , M. Wada , S. Walker , H. Wang , Y. Wang , A. W. Watson , S. Westerdale , J. Wilhelmi , M. M. Wojcik , X. Xiang , J. Xu , C. Yang , J. Yoo , S. Zavatarelli , A. Zec , W. Zhong , C. Zhu , G. Zuzel

We present first significant limits on WIMP dark matter by the phonon-light technique, where combined phonon and light signals from a scintillating cryogenic detector are used. Data from early 2004 with two 300 g CRESST-II prototype…

We reconsider the discovery limit of multi-ton direct detection dark matter experiments in the light of recent measurements of the coherent elastic neutrino-nucleus scattering process. Assuming the cross section to be a parameter entirely…

High Energy Physics - Phenomenology · Physics 2022-01-28 D. Aristizabal Sierra , V. De Romeri , L. J. Flores , D. K. Papoulias

We reexamine the model-independent data analysis methods for extracting properties of Weakly Interacting Massive Particles (WIMPs) by using data (measured recoil energies) from direct Dark Matter detection experiments directly and, as a…

High Energy Astrophysical Phenomena · Physics 2010-11-10 Chung-Lin Shan

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…

The future Ricochet experiment aims at searching for new physics in the electroweak sector by providing a high precision measurement of the Coherent Elastic Neutrino-Nucleus Scattering (CENNS) process down to the sub-100 eV nuclear recoil…

The experiment CRESST-II aims at the detection of dark matter with scintillating CaWO$_4$ crystals operated as cryogenic detectors. Recent results on spin-independent WIMP-nucleon scattering from the CRESST-II Phase 2 allowed to probe a new…

Future multi-tonne Direct Detection experiments will be sensitive to solar neutrino induced nuclear recoils which form an irreducible background to light Dark Matter searches. Indeed for masses around 6 GeV the spectra of neutrinos and Dark…

High Energy Physics - Phenomenology · Physics 2015-03-10 Jonathan H. Davis

Recently the CRESST collaboration has published the long anticipated results of their direct Dark Matter (DM) detection experiment with a CaWO_4 target. The number of observed events exceeds known backgrounds at more than 4 sigma…

High Energy Physics - Phenomenology · Physics 2015-05-30 Joachim Kopp , Thomas Schwetz , Jure Zupan

Recent developments of the nuclear emulsion technology led to the production of films with nanometric silver halide grains suitable to track low energy nuclear recoils with submicrometric length. This improvement opens the way to a…

A direct WIMP (Weakly Interacting Massive Particle) detector with a neutron veto system is designed to better reject neutrons. An experimental configuration is studied in the present paper: 984 Ge modules are placed inside a reactor…

Instrumentation and Methods for Astrophysics · Physics 2019-10-11 Ye Xu , Jieqin Lan , Yin Bai , Weiwei Gao

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…

Background induced by neutrons in deep underground laboratories is a critical issue for all experiments looking for rare events, such as dark matter interactions or neutrinoless 2-beta decay. Neutrons can be produced either by natural…

Astrophysics · Physics 2009-06-23 V. A. Kudryavtsev , L. Pandola , V. Tomasello

We revisit the expected sensitivity of large-scale xenon detectors to Weakly Interacting Massive Particles (WIMPs). Assuming current primary noise sources can be mitigated, we find that with the present discrimination power between nuclear…

High Energy Physics - Phenomenology · Physics 2024-10-04 Itay M. Bloch , Salvatore Bottaro , Diego Redigolo , Ludovico Vittorio

Ultra-low-background experiments address some of the most important open questions in particle physics, cosmology and astrophysics: the nature of dark matter, whether the neutrino is its own antiparticle, and does the proton decay. These…

Instrumentation and Detectors · Physics 2018-03-14 J. Cooley , K. J. Palladino , H. Qiu , M. Selvi , S. Scorza , C. Zhang

Dark matter is poorly constrained by direct detection experiments at masses below 1 MeV. This is an important target for the next generation of experiments, and several methods have been proposed to probe this mass range. One class of such…

High Energy Physics - Phenomenology · Physics 2020-07-31 Benjamin V. Lehmann , Stefano Profumo