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Related papers: Post-Acceleration Study for Neutrino Super-beam at…

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The nuSTORM facility has been designed to deliver beams of electron neutrinos and muon neutrinos (and their anti-particles) from the decay of a stored muon beam with a central momentum of 3.8 GeV/c and a momentum acceptance of 10%. The…

Accelerator Physics · Physics 2017-03-20 D. Adey , S. K. Agarwalla , C. M. Ankenbrandt , R. Asfandiyarov , J. J. Back , G. Barker , E. Baussan , R. Bayes , S. Bhadra , V. Blackmore , A. Blondel , S. A. Bogacz , C. Booth , S. B. Boyd , A. Bravar , S. J. Brice , A. D. Bross , F. Cadoux , H. Cease , A. Cervera , J. Cobb , D. Colling , P. Coloma , L. Coney , A. Dobbs , J. Dobson , A. Donini , P. Dornan , M. Dracos , F. Dufour , R. Edgecock , J. Evans , M. Geelhoed , M. A. George , T. Ghosh , J. J. Gomez-Cadenas , A. de Gouvea , A. Haesler , G. Hanson , P. F. Harrison , M. Hartz , P. Hernandez , J. A. Hernando Morata , P. Hodgson , P. Huber , A. Izmaylov , Y. Karadzhov , T. Kobilarcik , J. Kopp , L. Kormos , A. Korzenev , Y. Kuno , A. Kurup , P. Kyberd , J. B. Lagrange , A. Laing , A. Liu , J. M. Link , K. Long , K. Mahn , C. Mariani , C. Martin , J. Martin , N. McCauley , K. T. McDonald , O. Mena , S. R. Mishra , N. Mokhov , J. Morfin , Y. Mori , W. Murray , D. Neuffer , R. Nichol , E. Noah , M. A. Palmer , S. Parke , S. Pascoli , J. Pasternak , M. Popovic , P. Ratoff , M. Ravonel , M. Rayner , S. Ricciardi , C. Rogers , P. Rubinov , E. Santos , A. Sato , T. Sen , E. Scantamburlo , J. K. Sedgbeer , D. R. Smith , P. J. Smith , J. T. Sobczyk , L. Soby , F. J. P. Soler , S. Soldner-Rembold , M. Sorel , P. Snopok , P. Stamoulis , L. Stanco , S. Striganov , H. A. Tanaka , I. J. Taylor , C. Touramanis , C. D. Tunnell , Y. Uchida , N. Vassilopoulos , M. O. Wascko , A. Weber , M. J. Wilking , E. Wildner , W. Winter , U. K. Yang

The Japan Proton Accelerator Research Complex (J-PARC) currently delivers a 1 MW, 3 GeV proton beam to the Materials and Life Science Experimental Facility (MLF). Power is expected to increase to 1.3 MW, driven by the needs of…

This report is intended to describe first, the principal physics reasons for an ambitious experimental program in neutrino physics and proton decay based on construction of a series of massive water Cherenkov detectors located deep…

The nuSTORM facility has been designed to deliver beams of electron and muon neutrinos from the decay of a stored muon beam with a central momentum of 3.8 GeV/c and a momentum spread of 10%. The facility is unique in that it will: serve the…

Accelerator Physics · Physics 2013-05-08 D. Adey , S. K. Agarwalla , C. M. Ankenbrandt , R. Asfandiyarov , J. J. Back , G. Barker , E. Baussan , R. Bayes , S. Bhadra , V. Blackmore , A. Blondel , S. A. Bogacz , C. Booth , S. B. Boyd , A. Bravar , S. J. Brice , A. D. Bross , F. Cadoux , H. Cease , A. Cervera , J. Cobb , D. Colling , L. Coney , A. Dobbs , J. Dobson , A. Donini , P. J. Dornan , M. Dracos , F. Dufour , R. Edgecock , J. Evans , M. A. George , T. Ghosh , A. deGouvea , J. J. Gomez-Cadenas , A. Haesler , G. Hanson , M. Geelhoed , P. F. Harrison , M. Hartz , P. Hernandez , J. A. Hernando-Morata , P. J. Hodgson , P. Huber , A. Izmaylov , Y. Karadhzov , T. Kobilarcik , J. Kopp , L. Kormos , A. Korzenev , A. Kurup , Y. Kuno , P. Kyberd , J. P. Lagrange , A. M. Laing , J. Link , A. Liu , K. R. Long , N. McCauley , K. T. McDonald , K. Mahn , C. Martin , J. Martin , O. Mena , S. R. Mishra , N. Mokhov , J. Morfin , Y. Mori , W. Murray , D. Neuffer , R. Nichol , E. Noah , M. A. Palmer , S. Parke , S. Pascoli , J. Pasternak , M. Popovic , P. Ratoff , M. Ravonel , M. Rayner , S. Ricciardi , C. Rogers , P. Rubinov , E. Santos , A. Sato , E. Scantamburlo , J. K. Sedgbeer , D. R. Smith , P. J. Smith , J. T. Sobczyk , S. Soldner-Rembold , F. J. P. Soler , M. Sorel , A. Stahl , L. Stanco , P. Stamoulis , S. Striganov , H. Tanaka , I. J. Taylor , C. Touramanis , C. D. Tunnel , Y. Uchida , N. Vassilopoulos , M. O. Wascko , A. Weber , E. Wildner , M. J. Wilking , W. Winter , U. K. Yang

Elegant experiments are being carried out, or are in preparation, to improve the precision with which the solar and atmospheric neutrino-oscillation parameters are known, and to attempt to make a first measurement of the small mixing angle…

Instrumentation and Detectors · Physics 2010-01-05 K. Long

Coherent elastic neutrino-nucleus scattering (CE$\nu$NS) offers a unique way to study neutrino properties and to search for new physics beyond the Standard Model. Nuclear reactors are promising sources to explore this process at low…

The potential of muon beams for high energy physics applications is described along with the challenges of producing high quality muon beams. Two proposed approaches for delivering high intensity muon beams, a proton driver source and a…

Accelerator Physics · Physics 2019-09-26 Manuela Boscolo , Jean Pierre Delahaye , Mark Palmer

For the China Spallation Neutron Source (CSNS), a combination of the H- stripping and phase space painting method is used to accumulate a high intensity beam in the Rapid Cycling Synchrotron (RCS). In this paper, firstly, the injection…

Accelerator Physics · Physics 2015-10-19 Ming-Yang Huang , Sheng Wang , Nan Huang , Jing Qiu , Shou-Yan Xu , Liang-Sheng Huang

In order to update the beam power from 100 kW to 250 kW in China spallation neutron source (CSNS) Phase II, one of the important measures is to replace the 80 meters long beam transport line between the present 80 MeV linac injector and the…

Accelerator Physics · Physics 2015-07-14 LI Zhi-Hui , FU Shi-Nian

The Long Baseline Neutrino Experiment (LBNE) will utilize a beamline facility located at Fermilab to carry out a compelling research program in neutrino physics. The facility will aim a wide band beam of neutrinos toward a detector placed…

Accelerator Physics · Physics 2015-02-06 V. Papadimitriou , R. Andrews , J. Hylen , T. Kobilarcik , A. Marchionni , C. D. Moore , P. Schlabach , S. Tariq

The GEM-based neutron detector has flourished in the past decade. However almost all the GEM-based neutron detectors work in the flow-gas mode, and the long-term performances of the detectors may be unstable due to the dynamic changes of…

The Spallation Neutron Source (SNS) at Oak Ridge National Laboratory provides an intense, high-quality source of neutrinos from pion decay at rest. This source was recently used for the first measurements of coherent elastic…

High Energy Physics - Experiment · Physics 2021-11-16 P. S. Barbeau , Yu. Efremenko , K. Scholberg

Accelerator driven system (ADS) subcritical nuclear reactors are under development around the world. They will be intense sources of free, 30-50 MeV antimuon decay at rest antimuon neutrinos. These ADS reactor neutrinos can provide a robust…

High Energy Physics - Phenomenology · Physics 2017-04-27 Emilio Ciuffoli , Jarah Evslin , Fengyi Zhao

the main physics goal for Back-n white neutron facility at China Spallation Neutron Source (CSNS) is to measure nuclear data. The energy of neutrons is one of the most important parameters for measuring nuclear data. Method of time of…

Jinping Neutrino Experiment (Jinping) is proposed to significantly improve measurements on solar neutrinos and geoneutrinos in China Jinping Laboratory - a lab with a number of unparalleled features, thickest overburden, lowest reactor…

The European Spallation Source, currently under construction in Lund, Sweden, is a multidisciplinary international laboratory. Once completed to full specifications, it will operate the world's most powerful pulsed neutron source. Supported…

Supernovae (SNe) with strong interactions with circumstellar material (CSM) are promising candidate sources of high-energy neutrinos and gamma rays, and have been suggested as an important contributor to Galactic cosmic rays beyond 1 PeV.…

High Energy Astrophysical Phenomena · Physics 2019-03-27 Kohta Murase , Anna Franckowiak , Keiichi Maeda , Raffaella Margutti , John F. Beacom

The small energy exchange via nucleon recoils in neutrino-nucleon scattering is now supposed to be one of the important factors for successful explosion of core-collapse supernovae (CCSNe) as they can change neutrino spectra through…

High Energy Astrophysical Phenomena · Physics 2020-07-08 Chinami Kato , Hiroki Nagakura , Yusuke Hori , Shoichi Yamada

The sources of the astrophysical neutrino flux discovered by IceCube are for the most part unresolved. Extragalactic core-collapse supernovae (CCSNe) have been suggested as candidate multi-messenger sources. In interaction-powered…

High Energy Astrophysical Phenomena · Physics 2023-08-03 Massimiliano Lincetto

There are recent considerations to increase the photomultiplier density in the IceCube detector array beyond that of DeepCore, which will lead to a lower detection threshold and a huge fiducial mass for the neutrino detection. This…

High Energy Physics - Phenomenology · Physics 2015-05-30 Jian Tang , Walter Winter