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Development of large mass detectors for low-energy neutrinos and dark matter may allow supernova detection via neutrino-nucleus elastic scattering. An elastic-scattering detector could observe a few, or more, events per ton for a galactic…

Astrophysics · Physics 2009-11-07 C. J. Horowitz , K. J. Coakley , D. N. McKinsey

This project is focused on the development of a novel strategy for the precise measurement of beta decay energy spectra. The exact determination of beta spectra has wide implications in the particle and nuclear physics fields: from sterile…

The SNO+ experiment collected data as a low-threshold water Cherenkov detector from September 2017 to July 2019. Measurements of the 2.2-MeV $\gamma$ produced by neutron capture on hydrogen have been made using an Am-Be calibration source,…

Instrumentation and Detectors · Physics 2020-07-15 The SNO+ Collaboration , : , M. R. Anderson , S. Andringa , M. Askins , D. J. Auty , N. Barros , F. Barão , R. Bayes , E. W. Beier , A. Bialek , S. D. Biller , E. Blucher , R. Bonventre , M. Boulay , E. Caden , E. J. Callaghan , J. Caravaca , D. Chauhan , M. Chen , O. Chkvorets , B. Cleveland , M. A. Cox , M. M. Depatie , J. Dittmer , F. Di Lodovico , A. D. Earle , E. Falk , N. Fatemighomi , V. Fischer , E. Fletcher , R. Ford , K. Frankiewicz , K. Gilje , D. Gooding , C. Grant , J. Grove , A. L. Hallin , D. Hallman , S. Hans , J. Hartnell , P. Harvey , W. J. Heintzelman , R. L. Helmer , D. Horne , B. Hreljac , J. Hu , A. S. M. Hussain , A. S. Inácio , C. J. Jillings , T. Kaptanoglu , P. Khaghani , J. R. Klein , R. Knapik , L. L. Kormos , B. Krar , C. Kraus , C. B. Krauss , T. Kroupova , I. Lam , B. J. Land , A. LaTorre , I. Lawson , L. Lebanowski , E. J. Leming , A. Li , J. Lidgard , B. Liggins , Y. H. Lin , Y. Liu , V. Lozza , M. Luo , S. Maguire , A. Maio , S. Manecki , J. Maneira , R. D. Martin , E. Marzec , A. Mastbaum , N. McCauley , A. B. McDonald , P. Mekarski , M. Meyer , C. Mills , I. Morton-Blake , S. Nae , M. Nirkko , L. J. Nolan , H. M. O'Keeffe , G. D. Orebi Gann , M. J. Parnell , J. Paton , S. J. M. Peeters , T. Pershing , L. Pickard , G. Prior , A. Reichold , S. Riccetto , R. Richardson , M. Rigan , J. Rose , R. Rosero , P. M. Rost , J. Rumleskie , I. Semenec , F. Shaker , M. K. Sharma , K. Singh , P. Skensved , M. Smiley , M. I. Stringer , R. Svoboda , B. Tam , L. Tian , J. Tseng , E. Turner , R. Van Berg , J. G. C. Veinot , C. J. Virtue , E. Vázquez-Jáuregui , S. C. Walton , J. Wang , M. Ward , J. J. Weigand , J. R. Wilson , P. Woosaree , A. Wright , J. P. Yanez , M. Yeh , T. Zhang , Y. Zhang , K. Zuber , A. Zummo

During this experiment we were testing the hypothesis that standing waves in a phospholipid membrane stack indeed lead to a detectable signal in coherent grazing-incidence small-angle neutron scattering, GISANS. These modes were identified…

The IceCube Neutrino Observatory at the South Pole has measured the diffuse astrophysical neutrino flux up to ~PeV energies and is starting to identify first point source candidates. The next generation facility, IceCube-Gen2, aims at…

High Energy Astrophysical Phenomena · Physics 2021-07-20 Steffen Hallmann , Brian Clark , Christian Glaser , Daniel Smith

The atmospheric neutrino flux represents a continuous source that can be exploited to infer properties about Cosmic Rays and neutrino oscillation physics. The JUNO observatory, a 20 kt liquid scintillator currently under construction in…

High Energy Physics - Experiment · Physics 2020-12-08 G. Settanta , S. M. Mari , C. Martellini , P. Montini

The large next generation liquid-scintillator detector LENA (Low Energy Neutrino Astronomy) offers an excellent opportunity for neutrino oscillometry. The characteristic spatial pattern of very low monoenergetic neutrino disappearance from…

Space missions offer unique opportunities for studying ultra-high-energy (UHE) cosmic rays and neutrinos by leveraging secondary emissions generated by extensive air showers (EAS) resulting from their interactions with the atmosphere or…

Instrumentation and Methods for Astrophysics · Physics 2025-09-18 Tobias Heibges , Claire Guépin , Luke Kupari , Hannah Wistrand , Randy Lahm , Johannes Eser , Mary Hall Reno , Tonia M. Venters , Lawrence Wiencke

The T-REX neutron time-of-flight spectrometer at the European Spallation Source will use Multi-Grid Technology, which relies on thin B4C coatings on the Al blades of the grids to detect scattered thermal neutrons. Following a Monte Carlo…

Instrumentation and Detectors · Physics 2025-11-06 A. Backis , C. -C. Lai , M. Aouane , P. P. Deen , K. G. Fissum , J. R. M. Annand , K. Livingston , D. Raspino

A lead scintillator sandwich sampling calorimeter has been installed in the HERA tunnel 105.6 m from the central ZEUS detector in the proton beam direction. It is designed to measure the energy and scattering angle of neutrons produced in…

The design of a neutron source capable of producing 24 and 70 keV neutron beams with narrow energy spread is presented. The source exploits near-threshold kinematics of the $^{7}$Li(p,n)$^{7}$Be reaction while taking advantage of the…

Instrumentation and Detectors · Physics 2014-05-22 T. H. Joshi , S. Sangiorgio , V. Mozin , E. B. Norman , P. Sorensen , M. Foxe , G. Bench , A. Bernstein

We report here first extensive measurements of the temperature dependence of phonon density of states of BaFe2As2, the parent compound of the newly discovered FeAs-based superconductors, using inelastic neutron scattering. The experiments…

Superconductivity · Physics 2008-09-17 R. Mittal , Y. Su , S. Rols , T. Chatterji , S. L. Chaplot , H. Schober , M. Rotter , D. Johrendt , Th. Brueckel

The interaction between the ejecta of supernovae (SNe) of Type IIn and a dense circumstellar medium (CSM) can efficiently generate thermal UV/optical radiation and lead to the emission of neutrinos in the $1$-$10^{3}$~TeV range. We…

High Energy Astrophysical Phenomena · Physics 2023-08-02 Tetyana Pitik , Irene Tamborra , Massimiliano Lincetto , Anna Franckowiak

The first lead neutron slowing-down spectrometer (LSDS) from a pulsed source in elastic scattering on lead nuclei has been constructed in the laboratory of the atomic nucleus of the Physics Institute of the Russian Academy of Sciences LPI.…

In the domain of Fermi energy, the hot nucleus temperature can be determined by using the energy spectra of evaporated light charged particles. But this method of measurement is not without difficulties both theoretical and experimental.…

After the first measurement of the coherent elastic neutrino nucleus scattering (CENNS) by the COHERENT Collaboration, it is expected that new experiments will confirm the observation. Such measurements will allow to put stronger…

High Energy Physics - Phenomenology · Physics 2018-08-01 B. C. Cañas , E. A. Garcés , O. G. Miranda , A. Parada

The next generation of very-short-baseline reactor experiments will require compact detectors operating at surface level and close to a nuclear reactor. This paper presents a new detector concept based on a composite solid scintillator…

A time-of-flight spectrometer of neutrons in the energy range (0.05 -- 2.5)$\mu$eV is described. This spectrometer has been tested my measuring the total and differential neutron cross sections for a number of materials: Al, Cu, $^{6}$LiF,…

Nuclear Experiment · Physics 2011-02-15 Yu. N. Pokotilovski , M. I. Novopoltsev , P. Geltenbort , Th. Brenner

At a spallation neutron source, the wavelength of a neutron is generally determined by its time-of-flight (TOF) from the source to the detector. The achievable precision is ultimately limited by the non-zero emission time-width of the…

Instrumentation and Detectors · Physics 2007-05-23 A. A. Parizzi , W. -T. Lee , G. P. Felcher , F. Klose