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Book Detection of Supernova Neutrinos at Spallation Neutron Sources Supported by National Natural Science Foundation of China  11205185  11175020  11275025  11575023

Download or read book Detection of Supernova Neutrinos at Spallation Neutron Sources Supported by National Natural Science Foundation of China 11205185 11175020 11275025 11575023 written by and published by . This book was released on 2016 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Abstract: After considering supernova shock effects, Mikheyev-Smirnov-Wolfenstein effects, neutrino collective effects, and Earth matter effects, the detection of supernova neutrinos at the China Spallation Neutron Source is studied and the expected numbers of different flavor supernova neutrinos observed through various reaction channels are calculated with the neutrino energy spectra described by the Fermi-Dirac distribution and the "beta fit" distribution respectively. Furthermore, the numerical calculation method of supernova neutrino detection on Earth is applied to some other spallation neutron sources, and the total expected numbers of supernova neutrinos observed through different reactions channels are given.

Book Study of Accelerator Neutrino Detection at a Spallation Source  Supported by National Natural Science Foundation of China  11205185  11175020

Download or read book Study of Accelerator Neutrino Detection at a Spallation Source Supported by National Natural Science Foundation of China 11205185 11175020 written by and published by . This book was released on 2016 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: Abstract: We study the detection of accelerator neutrinos produced at the China Spallation Neutron Source (CSNS). Using the code FLUKA, we have simulated the production of neutrinos in a proton beam on a tungsten target and obtained the yield efficiency, numerical flux, and average energy of different flavors of neutrinos. Furthermore, detection of these accelerator neutrinos is investigated in two reaction channels: neutrino-electron reactions and neutrino-carbon reactions. The expected numbers of different flavors of neutrinos have also been calculated.

Book A Large Neutrino Detector Facility at the Spallation Neutron Source at Oak Ridge National Laboratory

Download or read book A Large Neutrino Detector Facility at the Spallation Neutron Source at Oak Ridge National Laboratory written by and published by . This book was released on 2001 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: The ORLaND (Oak Ridge Large Neutrino Detector) collaboration proposes to construct a large neutrino detector in an underground experimental hall adjacent to the first target station of the Spallation Neutron Source (SNS) at the Oak Ridge National Laboratory. The main mission of a large (2000 ton) Scintillation-Cherenkov detector is to measure[bar[nu]][sub[mu]][r-arrow][bar[nu]][sub e] neutrino oscillation parameters more accurately than they can be determined in other experiments, or significantly extending the covered parameter space below (sin'20[le] 10[sup[minus]4]). In addition to the neutrino oscillation measurements, ORLaND would be capable of making precise measurements of sin[sup 2][theta][sub W], search for the magnetic moment of the muon neutrino, and investigate the anomaly in the KARMEN time spectrum, which has been attributed to a new neutral particle. With the same facility an extensive program of measurements of neutrino nucleus cross sections is also planned to support nuclear astrophysics.

Book The COHERENT Experiment at the Spallation Neutron Source

Download or read book The COHERENT Experiment at the Spallation Neutron Source written by and published by . This book was released on 2015 with total page 21 pages. Available in PDF, EPUB and Kindle. Book excerpt: The COHERENT collaboration's primary objective is to measure coherent elastic neutrino- nucleus scattering (CEvNS) using the unique, high-quality source of tens-of-MeV neutrinos provided by the Spallation Neutron Source (SNS) at Oak Ridge National Laboratory (ORNL). In spite of its large cross section, the CEvNS process has never been observed, due to tiny energies of the resulting nuclear recoils which are out of reach for standard neutrino detectors. The measurement of CEvNS has now become feasible, thanks to the development of ultra-sensitive technology for rare decay and weakly-interacting massive particle (dark matter) searches. The CEvNS cross section is cleanly predicted in the standard model; hence its measurement provides a standard model test. It is relevant for supernova physics and supernova-neutrino detection, and enables validation of dark-matter detector background and detector-response models. In the long term, precision measurement of CEvNS will address questions of nuclear structure. COHERENT will deploy multiple detector technologies in a phased approach: a 14-kg CsI[Na] scintillating crystal, 15 kg of p-type point-contact germanium detectors, and 100 kg of liquid xenon in a two-phase time projection chamber. Following an extensive background measurement campaign, a location in the SNS basement has proven to be neutron-quiet and suitable for deployment of the COHERENT detector suite. The simultaneous deployment of the three COHERENT detector subsystems will test the N=2 dependence of the cross section and ensure an unambiguous discovery of CEvNS. This document describes concisely the COHERENT physics motivations, sensitivity and plans for measurements at the SNS to be accomplished on a four-year timescale.

Book Supernova Neutrinos

Download or read book Supernova Neutrinos written by and published by . This book was released on 2003 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt: We propose that neutrino-proton elastic scattering, [nu]+ p[yields][nu]+ p, can be used for the detection of supernova neutrinos. Though the proton recoil kinetic energy spectrum is soft, with T[sub p][approx-equal] 2E[sub[nu]][sup 2]/M[sub p], and the scintillation light output from slow, heavily ionizing protons is quenched, the yield above a realistic threshold is nearly as large as that from[bar[nu]][sub e]+ p[yields] e[sup+]+ n. In addition, the measured proton spectrum is related to the incident neutrino spectrum, which solves a long-standing problem of how to separately measure the total energy release and temperature of[nu][sub[mu]], [nu][sub[tau]], [bar[nu]][sub[mu]], and[bar[nu]][sub[tau]]. The ability to detect this signal would give detectors like KamLAND and Borexino a crucial and unique role in the quest to detect supernova neutrinos.

Book Neutron Counter for Supernova Neutrino Detection

Download or read book Neutron Counter for Supernova Neutrino Detection written by John C. Andress and published by . This book was released on 1998 with total page 90 pages. Available in PDF, EPUB and Kindle. Book excerpt: