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相关论文: Prototyping an Active Neutron Veto for SuperCDMS

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Neutrons are a particularly dangerous background for direct WIMP dark matter searches; their nuclear recoils with the target nucleus are often indistinguishable from nuclear recoils produced by WIMP-nuclear collisions. In this study, we…

仪器与探测器 · 物理学 2016-04-06 Shawn Westerdale , Emily Shields , Frank Calaprice

We present a conceptual design for an active neutron veto, based on boron-loaded liquid scintillator, for use in direct-detection dark matter experiments. The simulated efficiency of a 1 meter thick veto, after including the effects of…

核实验 · 物理学 2011-06-13 Alex Wright , Pablo Mosteiro , Ben Loer , Frank Calaprice

Scintillator doped with a high neutron-capture cross-section material can be used to detect neutrons via their resulting gamma rays. Examples of such detectors using liquid scintillator have been successfully used in high-energy physics…

仪器与探测器 · 物理学 2019-01-01 D. M. Poehlmann , D. Barker , H. Chagani , P. Cushman , G. Heuermann , A. Medved , H. E. Rogers , R. Schmitz

A direct WIMP (Weakly Interacting Massive Particle) detector with a neutron veto system is designed to better reject neutrons. Two experimental configurations are studied in the present paper: one is for an Xe detector enclosed in a…

天体物理仪器与方法 · 物理学 2015-05-19 Ye Xu , XiangPan Ji , ZeLong Liu , DanNing Di , HaoKai Sun , Yu Lei

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…

仪器与探测器 · 物理学 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

The NUCLEUS experiment aims to measure coherent elastic neutrino nucleus scattering of reactor anti-neutrinos using cryogenic calorimeters. Operating at an overburden of 3 m.w.e., muon-induced backgrounds are expected to be one of the…

A good particle candidate for Cold Dark Matter (CDM) is the supersymmetric neutralino or more generally a weakly interacting massive particle (WIMP). The expected interaction rate of WIMPs with the detector medium in the direct detection…

天体物理仪器与方法 · 物理学 2010-02-17 V. Kozlov

Radiogenic neutrons emitted by detector materials are one of the most challenging backgrounds for the direct search of dark matter in the form of weakly interacting massive particles (WIMPs). To mitigate this background, the XENONnT…

仪器与探测器 · 物理学 2025-11-10 XENON Collaboration , E. Aprile , J. Aalbers , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , D. Antón Martin , F. Arneodo , L. Baudis , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , K. Boese , A. Brown , G. Bruno , R. Budnik , C. Cai , C. Capelli , J. M. R. Cardoso , A. P. Cimental Chávez , A. P. Colijn , J. Conrad , J. J. Cuenca-García , V. D'Andrea , L. C. Daniel Garcia , M. P. Decowski , A. Deisting , C. Di Donato , P. Di Gangi , S. Diglio , K. Eitel , S. el Morabit , A. Elykov , A. D. Ferella , C. Ferrari , H. Fischer , T. Flehmke , M. Flierman , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , M. Galloway , F. Gao , S. Ghosh , R. Giacomobono , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , P. Gyorgy , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , Y. Kaminaga , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , D. Koke , A. Kopec , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , Y. -T. Lin , S. Lindemann , M. Lindner , K. Liu , M. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , T. Luce , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , E. Masson , S. Mastroianni , A. Melchiorre , J. Merz , M. Messina , A. Michael , K. Miuchi , A. Molinario , S. Moriyama , K. Morá , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , Y. Pan , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , G. Plante , T. R. Pollmann , L. Principe , J. Qi , J. Qin , D. Ramírez García , M. Rajado , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , J. Shi , M. Silva , H. Simgen , C. Szyszka , A. Takeda , Y. Takeuchi , P. -L. Tan , D. Thers , F. Toschi , G. Trinchero , C. D. Tunnell , F. Tönnies , K. Valerius , S. Vecchi , S. Vetter , F. I. Villazon Solar , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong

Silicon photo-multipliers (SiPMs) are state-of-the-art sensors capable of detecting a single photoelectron under cryogenic conditions, with potentially lower radioactivity than widely used photomultiplier tubes. The DarkSide-20k experiment,…

仪器与探测器 · 物理学 2026-04-06 20k collaboration

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…

天体物理仪器与方法 · 物理学 2015-06-18 Ye Xu , Xiangpan Ji , Haolin Li , Yulong Feng

COSINUS is a dark matter (DM) direct search experiment that uses sodium iodide (NaI) crystals as cryogenic calorimeters. Thanks to the low nuclear recoil energy threshold and event-by-event discrimination capability, COSINUS will address…

In the case of underground experiments for neutrino physics or rare event searches, the background caused by cosmic muons contributes significantly and therefore must be identified and rejected. We proposed and optimized a new detector…

仪器与探测器 · 物理学 2017-04-05 Y. P. Zhang , J. L. Xu , H. Q. Lu , P. Zhang , C. C. Zhang , C. G. Yang

The design, optimisation and construction of an anti-coincidence veto detector to complement the ZEPLIN-III direct dark matter search instrument is described. One tonne of plastic scintillator is arranged into 52 bars individually read out…

The elastic nuclear recoil signal, being under intense scrutiny by multiple underground experiments, can be interpreted either as coming from the interaction of nuclei with WIMP dark matter or from the scattering of new species of…

高能物理 - 唯象学 · 物理学 2014-03-26 Maxim Pospelov , Josef Pradler

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…

天体物理仪器与方法 · 物理学 2019-10-11 Ye Xu , Jieqin Lan , Yin Bai , Weiwei Gao

Dark Matter experiments searching for Weakly interacting massive particles (WIMPs) primarily use nuclear recoils (NRs) in their attempt to detect WIMPs. Migdal-induced electronic recoils (ERs) provide additional sensitivity to light Dark…

高能物理 - 唯象学 · 物理学 2022-12-22 J. R. Angevaare , G. Bertone , A. P. Colijn , M. P. Decowski , B. J. Kavanagh

This paper describes the design of the active muon veto subsystem for the MiniCLEAN dark matter direct detection experiment at SNOLAB in Sudbury, Ontario, Canada. The water-filled veto is instrumented with 48 PMTs which are read out by…

仪器与探测器 · 物理学 2015-12-09 Robert Abruzzio , Benjamin Buck , Stephen Jaditz , James Kelsey , Jocelyn Monroe , Kimberyl Palladino

The ZEPLIN-III experiment is operating in its second phase at the Boulby Underground Laboratory in search of dark matter WIMPs. The major upgrades to the instrument over its first science run include lower background photomultiplier tubes…

DarkSide-50 is a detector for dark matter candidates in the form of weakly interacting massive particles (WIMPs). It utilizes a liquid argon time projection chamber (LAr TPC) for the inner main detector. The TPC is surrounded by a liquid…

仪器与探测器 · 物理学 2017-02-06 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 , 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 , 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 , A. Pocar , S. Pordes , D. A. Pugachev , H. Qian , K. Randle , G. Ranucci , A. Razeto , B. Reinhold , A. L. Renshaw , Q. Riffard , 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 , R. 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

SuperCDMS SNOLAB will be a next-generation experiment aimed at directly detecting low-mass (< 10 GeV/c$^2$) particles that may constitute dark matter by using cryogenic detectors of two types (HV and iZIP) and two target materials…

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