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Related papers: SNO+ Commissioning Status

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The current status of neutrino oscillation searches with reactors and accelerators is reviewed. An outlook, especially on future long baseline neutrino oscillation projects, is given.

High Energy Physics - Phenomenology · Physics 2016-10-26 K. Zuber

Noble liquid detectors have become an attractive option for exploring physics beyond the standard model. Current experiments are using these detectors to search for dark matter interactions, neutrinoless double beta decay, and other…

Instrumentation and Detectors · Physics 2019-10-15 Philip L. R. Weigel , Erin V. Hansen , Michelle J. Dolinski

In the course of the high-frequency upgrade of GEO 600, its optical configuration was extended by a squeezed-light laser [1]. Recently, a non-classically enhanced measurement sensitivity of GEO 600 was reported [2]. In this paper, a…

It was recently shown that standard sub-GeV dark matter candidates can be effectively probed by large neutrino observatories via annual modulation of the total photomultiplier hit rate. That work focused on the production of light by the…

High Energy Physics - Phenomenology · Physics 2025-12-17 Lillian Santos-Olmsted , Rebecca K. Leane , Carlos Blanco , John F. Beacom

The SNO+ experiment is a large multi-purpose neutrino detector, currently filled with liquid scintillator. For the first time in a single experiment, SNO+ is able to measure the neutrino oscillation parameters $\theta_{12}$ and $\Delta…

High Energy Physics - Experiment · Physics 2024-03-29 Daniel Cookman

Although formal proposals have not yet been made, the UNO and Hyper-Kamiokande projects are being developed to follow-up the tremendously successful program at Super-Kamiokande using a detector that is 20-50 times larger. The potential of…

Astrophysics · Physics 2009-11-10 Maury Goodman

The large depth of the SNO+ experiment (2070 m, 6010 m.w.e.) means that only a few muons per day pass through the detector. However, their high energy causes muon induced backgrounds which can affect multiple physics analyses.…

Instrumentation and Detectors · Physics 2024-04-08 Jasmine Simms

The SNO+ liquid scintillator experiment is under construction in the SNOLAB facility in Canada. The success of this experiment relies upon accurate characterization of the liquid scintillator, linear alkylbenzene (LAB). In this paper,…

Instrumentation and Detectors · Physics 2011-06-16 H. M. O'Keeffe , E. O'Sullivan , M. C. Chen

We report on the status of the Fermilab accelerator complex, including recent performance, upgrades in progress, and plans for the future. Beam delivery to the neutrino experiments surpassed our goals for the past year. The Proton…

Accelerator Physics · Physics 2016-12-30 M. E. Convery

The light yield of a water-based Cherenkov detector can be significantly improved by adding a wavelength shifter. Wavelength shifter (WLS) molecules absorb ultraviolet photons and re-emit them at longer wavelengths where typical…

Instrumentation and Detectors · Physics 2008-11-26 Xiongxin Dai , Etienne Rollin , Alain Bellerive , Cliff Hargrove , David Sinclair , Cathy Mifflin , Feng Zhang

We summarize the current status of accelerator based neutrino crosssection measurements. We focus on the experimental challenges while also presenting the motivation for these measurements. Selected results are highlighted after a quick…

High Energy Physics - Experiment · Physics 2018-04-11 M. F. Carneiro

The direction of individual $^8$B solar neutrinos has been reconstructed using the SNO+ liquid scintillator detector. Prompt, directional Cherenkov light was separated from the slower, isotropic scintillation light using time information,…

High Energy Physics - Experiment · Physics 2024-04-11 A. Allega , M. R. Anderson , S. Andringa , J. Antunes , M. Askins , D. J. Auty , A. Bacon , J. Baker , N. Barros , F. Barão , R. Bayes , E. W. Beier , T. S. Bezerra , A. Bialek , S. D. Biller , E. Blucher , E. Caden , E. J. Callaghan , M. Chen , S. Cheng , B. Cleveland , D. Cookman , J. Corning , M. A. Cox , R. Dehghani , J. Deloye , M. M. Depatie , F. Di Lodovico , J. Dittmer , K. H. Dixon , E. Falk , N. Fatemighomi , R. Ford , A. Gaur , O. I. Ganzálaz-Reina , D. Gooding , C. Grant , J. Grove , S. Hall , A. L. Hallin , W. J. Heintzelman , R. L. Helmer , C. Hewitt , B. Hreljac , V. Howard , J. Hu , R. Hunt-Stokes , S. M. A. Hussain , A. S. Inácio , C. J. Jillings , S. Kaluzienski , T. Kaptanoglu , P. Khaghani , H. Khan , J. R. Klein , L. L. Kormos , B. Krar , C. Kraus , C. B. Krauss , T. Kroupová , C. Lake , L. Lebanowski , J. Lee , C. Lefebvra , Y. H. Lin , V. Lozza , M. Luo , A. Maio , S. Manecki , J. Maneira , R. D. Martin , N. McCauley , A. B. McDonald , C. Mills , G. Milton , I. Morton-Blake , M. Mubasher , A. Molina Colina , D. Morris , S. Naugle , L. J. Nolan , H. M. O'Keeffe , G. D. Orebi Gann , J. Page , K. Paleshi , W. Parker , J. Paton , S. J. M. Peeters , L. Pickard , P. Ravi , A. Reichold , S. Riccetto , M. Rigan , J. Rose , R. Rosero , J. Rumleskie , I. Semenec , P. Skensvard , M. Smiley , J. Smith , R. Svoboda , B. Tam , J. Tseng , S. Valder , E. Vázquez-Jáuregui , C. J. Virtue , J. Wang , M. Ward , J. R. Wilson , J. D. Wilson , A. Wright , J. P. Yanez , S. Yang , M. Yeh , Z. Ye , S. Yu , Y. Zhang , K. Zuber , A. Zummo

The Sudbury Neutrino Observatory (SNO) measures both the flux of the electron-type neutrinos and the total flux of all active flavours of neutrinos originating from the Sun. A model-independent test of neutrino flavour transformation was…

High Energy Physics - Experiment · Physics 2019-08-14 A. W. P. Poon

The SOUL systems at the Large Bincoular Telescope can be seen such as precursor for the ELT SCAO systems, combining together key technologies such as EMCCD, Pyramid WFS and adaptive telescopes. After the first light of the first upgraded…

In this note, we compile results of various simulation studies for the upgrade of the Belle detector. Based on these studies, we propose a set of optimum or appropriate parameters of the detector.

SNO+ is a multipurpose liquid-scintillator neutrino detector located 2 km underground at SNOLAB, Canada. Three large nuclear reactors at baselines of 240-350 km allow a precise measurement of the neutrino oscillation parameter $\Delta…

High Energy Physics - Experiment · Physics 2026-04-08 William Parker

With the completion of the first cubic-kilometer class neutrino telescopes, IceCube, the race for the discovery of the first cosmic high-energy neutrino sources enters into a new phase. The usage of neutrinos as cosmic messengers has the…

High Energy Astrophysical Phenomena · Physics 2011-11-01 Alexander Kappes

I describe the current status of the solar neutrino problem, summarizing the arguments that its resolution will require new particle physics. The phenomenon of matter-enhanced neutrino oscillations is reviewed. I consider the implications…

Nuclear Theory · Physics 2007-05-23 W. C. Haxton

The current status of neutrino oscillation searches with reactors and accelerators is reviewed. An outlook, especially on future long baseline neutrino oscillation projects, is given.

High Energy Physics - Phenomenology · Physics 2007-05-23 K. Zuber

The optical properties of the Sudbury Neutrino Observatory (SNO) heavy water Cherenkov neutrino detector are measured in situ using a light diffusing sphere ("laserball"). This diffuser is connected to a pulsed nitrogen/dye laser via…