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In the field of neutron scattering science, a large variety of instruments require detectors for thermal and cold neutrons. Helium-3 has been one of the main actors in thermal and cold neutron detection for many years. Nowadays neutron…

Instrumentation and Detectors · Physics 2020-07-21 Francesco Piscitelli , Giacomo Mauri , Alessio Laloni , Richard Hall-Wilton

In the future several Spallation Source facilities will be available worldwide. Spallation Sources produce large amount of neutrinos from decay-at-rest muons and thus can be well adapted to accommodate state-of-the-art neutrino experiments.…

High Energy Physics - Phenomenology · Physics 2010-12-02 R. Lazauskas , C. Volpe

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

The observation of neutrinoless double-beta decay would resolve the Majorana nature of the neutrino and could provide information on the absolute scale of the neutrino mass. The initial phase of the Majorana experiment, known as the…

We present the first measurements of the muon-induced neutron flux at the Boulby Underground Laboratory. The experiment was carried out with an 0.73 tonne liquid scintillator that also served as an anticoincidence system for the ZEPLIN-II…

The atmospheric muon and neutrino flux have been simulated using the same approach which successfully accounted for the recent secondary proton, electron and positron flux measurements in orbit by the AMS experiment. For the muon flux, a…

Astrophysics · Physics 2014-10-13 Yong Liu , L. Derome , M. Buenerd

The measurement of environmental neutrons is particularly important in the search for new physics, such as dark matter particles, because neutrons constitute an often-irreducible background source. The measurement of the neutron energy…

Instrumentation and Detectors · Physics 2023-01-13 T. Shiraishi , S. Akamatsu , T. Naka , T. Asada , G. De Lellis , V. Tioukov , G. Rosa , R. Kobayashi , N. Ambrosio , A. Alexandrov , O. Sato

It is known that neutron background is a big problem for low-background experiments in underground Laboratories. Our global net of en-detectors sensitive to thermal neutrons includes the detectors running both on the surface and at…

The Sanford Underground Research Facility (SURF) has been operating since 2007 supporting underground research in rare-process physics, as well as offering research opportunities in other disciplines. SURF laboratory facilities include a…

High Energy Physics - Experiment · Physics 2022-09-27 Jaret Heise

High-energy cosmic-ray muons reaching deep underground laboratories can cause events in detectors that mimic signals expected from dark matter particles, neutrinos, or rare decays. Knowledge of the muon flux and energy spectrum is important…

High Energy Physics - Experiment · Physics 2026-02-20 D. S. Akerib , A. K. Al Musalhi , F. Alder , B. J. Almquist , C. S. Amarasinghe , A. Ames , T. J. Anderson , N. Angelides , H. M. Araújo , J. E. Armstrong , M. Arthurs , A. Baker , S. Balashov , J. Bang , J. W. Bargemann , E. E. Barillier , K. Beattie , A. Bhatti , T. P. Biesiadzinski , H. J. Birch , E. Bishop , G. M. Blockinger , C. A. J. Brew , P. Brás , S. Burdin , M. C. Carmona-Benitez , M. Carter , A. Chawla , H. Chen , Y. T. Chin , N. I. Chott , S. Contreras , M. V. Converse , R. Coronel , A. Cottle , G. Cox , D. Curran , C. E. Dahl , I. Darlington , S. Dave , A. David , J. Delgaudio , S. Dey , L. de Viveiros , L. Di Felice , C. Ding , J. E. Y. Dobson , E. Druszkiewicz , S. Dubey , C. L. Dunbar , S. R. Eriksen , N. M. Fearon , N. Fieldhouse , S. Fiorucci , H. Flaecher , E. D. Fraser , T. M. A. Fruth , P. W. Gaemers , R. J. Gaitskell , A. Geffre , J. Genovesi , C. Ghag , J. Ghamsari , A. Ghosh , R. Gibbons , S. Gokhale , J. Green , M. G. D. van der Grinten , J. J. Haiston , C. R. Hall , T. Hall , R. H. Hampp , S. J. Haselschwardt , M. A. Hernandez , S. A. Hertel , G. J. Homenides , M. Horn , D. Q. Huang , D. Hunt , R. S. James , E. Jacquet , K. Jenkins , A. C. Kaboth , A. C. Kamaha , M. K. Kannichankandy , D. Khaitan , A. Khazov , J. Kim , Y. D. Kim , D. Kodroff , E. V. Korolkova , H. Kraus , S. Kravitz , L. Kreczko , V. A. Kudryavtsev , C. Lawes , D. S. Leonard , K. T. Lesko , C. Levy , J. Lin , A. Lindote , W. H. Lippincott , J. Long , M. I. Lopes , W. Lorenzon , C. Lu , S. Luitz , V. Mahajan , P. A. Majewski , A. Manalaysay , R. L. Mannino , R. J. Matheson , C. Maupin , M. E. McCarthy , D. N. McKinsey , J. McLaughlin , J. B. Mclaughlin , R. McMonigle , B. Mitra , E. Mizrachi , M. E. Monzani , K. Morå , E. Morrison , B. J. Mount , M. Murdy , A. St. J. Murphy , H. N. Nelson , F. Neves , A. Nguyen , C. L. O'Brien , F. H. O'Shea , I. Olcina , K. C. Oliver-Mallory , J. Orpwood , K. Y. Oyulmaz , K. J. Palladino , N. J. Pannifer , N. Parveen , S. J. Patton , B. Penning , G. Pereira , E. Perry , T. Pershing , A. Piepke , S. S. Poudel , Y. Qie , J. Reichenbacher , C. A. Rhyne , G. R. C. Rischbieter , E. Ritchey , H. S. Riyat , R. Rosero , N. J. Rowe , T. Rushton , D. Rynders , S. Saltão , D. Santone , I. Sargeant , A. B. M. R. Sazzad , R. W. Schnee , G. Sehr , B. Shafer , S. Shaw , W. Sherman , K. Shi , T. Shutt , C. Silva , G. Sinev , J. Siniscalco , A. M. Slivar , R. Smith , V. N. Solovov , P. Sorensen , J. Soria , T. Stenhouse , T. J. Sumner , A. Swain , M. Szydagis , D. R. Tiedt , M. Timalsina , D. R. Tovey , J. Tranter , M. Trask , K. Trengove , M. Tripathi , A. Usón , A. C. Vaitkus , O. Valentino , V. Velan , A. Wang , J. J. Wang , Y. Wang , L. Weeldreyer , T. J. Whitis , K. Wild , M. Williams , J. Winnicki , L. Wolf , F. L. H. Wolfs , S. Woodford , D. Woodward , C. J. Wright , Q. Xia , J. Xu , Y. Xu , M. Yeh , D. Yeum , J. Young , W. Zha , H. Zhang , T. Zhang , Y. Zhou

Cosmic muon induced neutrons are a major source of background for low countrate experiments like neutrino oscillation or dark matter searches. Especially at shallow sites these neutrons are the limiting factor for the ultimate sensitivity…

High Energy Physics - Experiment · Physics 2017-08-23 J. Wolf

We report the limits on the diffuse supernova neutrino background (DSNB) flux and the fundamental DSNB parameters measured from the first science run of the LUX-ZEPLIN (LZ) experiment, a dual-phase xenon detector located at the Sanford…

High Energy Physics - Experiment · Physics 2025-01-20 Qing Xia

In the search for a monochromatic peak as the signature of neutrinoless double beta decay an excellent energy resolution and an ultra-low background around the $Q$-value of the decay are essential. The LEGEND-200 experiment performs such a…

Instrumentation and Detectors · Physics 2023-02-02 L. Baudis , G. Benato , E. M. Bond , P. -J. Chiu , S. R. Elliott , R. Massarczyk , S. Meijer , Y. Müller

Neutrino-electron scattering can be used to probe neutrino electromagnetic properties at low-threshold underground detectors with good angular and recoil electron energy resolution. We propose to do this using a number of artificial…

High Energy Physics - Phenomenology · Physics 2007-05-23 O. G. Miranda , J. Segura , V. B. Semikoz , J. W. F. Valle

Precise in-situ measurements of the neutron flux in underground laboratories is crucial for direct dark matter searches, as neutron induced backgrounds can mimic the typical dark matter signal. The development of a novel neutron…

Instrumentation and Detectors · Physics 2022-12-21 I. Giomataris , S. Green , I. Katsioulas , P. Knights , I. Manthos , J. Matthews , T. Neep , K. Nikolopoulos , T. Papaevangelou , B. Phoenix , J. Sanders , R. Ward

An extremely low-background environment is a crucial requirement for any neutrinoless double beta decay experiment. Neutrons are very difficult to stop, because they can pass through the shields and activate nuclei in the detector, even…

Instrumentation and Detectors · Physics 2023-07-25 Qianming Wang , Zeyu Huang , Pengchong Hu , Emilio Ciuffoli

The IceCube Neutrino Observatory at the South Pole has measured astrophysical neutrinos using through-going and starting events in the TeV to PeV energy range. The origin of these astrophysical neutrinos is still largely unresolved, and…

High Energy Astrophysical Phenomena · Physics 2023-02-01 Barbara Skrzypek , Marco Chianese , Carlos Argüelles Delgado

A fast neutron spectrometer consisting of segmented plastic scintillator and He-3 proportional counters was constructed for the measurement of neutrons in the energy range 1 MeV to 200 MeV. We discuss its design, principles of operation,…

Instrumentation and Detectors · Physics 2014-11-24 T. J. Langford , C. D. Bass , E. J. Beise , H. Breuer , D. K. Erwin , C. R. Heimbach , J. S. Nico

Environmental neutrons are a source of background for rare event searches in underground laboratories. Since the majority of the neutron background comes from the cavern walls due to the intrinsic radioactivity of concrete and rock, the…

Instrumentation and Detectors · Physics 2025-12-11 Francesco Pompa , Klaus Eitel , Alfredo Davide Ferella , Felix Kratzmeier , Melih Solmaz , Kathrin Valerius

The 3He-based neutron detectors are no longer the default solution for neutron scattering applications. Both the inability of fulfilling the requirements in performance, needed for the new instruments, and the shortage of 3He, drove a…

Instrumentation and Detectors · Physics 2020-03-13 Giacomo Mauri , Francesco Messi , Kalliopi Kanaki , Richard Hall-Wilton , Francesco Piscitelli