231 research outputs found

    Fabrication and characterization of a lithium-glass-based composite neutron detector

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    A novel composite, scintillating material intended for neutron detection and composed of small (1.5 mm) cubes of KG2-type lithium glass embedded in a matrix of scintillating plastic has been developed in the form of a 2.2 in.-diameter, 3.1 in.-tall cylindrical prototype loaded with (5.82±0.02)%\left( 5.82 \pm 0.02 \right)\% lithium glass by mass. The response of the material when exposed to 252{}^{252}Cf fission neutrons and various γ\gamma-ray sources has been studied; using the charge-integration method for pulse shape discrimination, good separation between neutron and γ\gamma-ray events is observed and intrinsic efficiencies of (1.15±0.16)×10−2\left( 1.15 \pm 0.16 \right)\times 10^{-2} and (2.28±0.21)×10−4\left( 2.28 \pm 0.21 \right)\times 10^{-4} for 252{}^{252}Cf fission neutrons and 60{}^{60}Co γ\gamma rays are obtained; an upper limit for the sensitivity to 137{}^{137}Cs γ\gamma rays is determined to be <3.70×10−8< 3.70 \times 10^{-8}. The neutron/γ\gamma discrimination capabilities are improved in circumstances when a neutron capture signal in the lithium glass can be detected in coincidence with a preceding elastic scattering event in the plastic scintillator; with this coincidence requirement, the intrinsic efficiency of the prototype detector for 60{}^{60}Co γ\gamma rays is (2.42±0.61)×10−6\left( 2.42 \pm 0.61 \right)\times 10^{-6} while its intrinsic efficiency for unmoderated 252{}^{252}Cf fission neutrons is (4.31±0.59)×10−3\left( 4.31 \pm 0.59 \right)\times 10^{-3}. Through use of subregion-integration ratios in addition to the coincidence requirement, the efficiency for γ\gamma rays from 60{}^{60}Co is reduced to (7.15±4.10)×10−7\left( 7.15 \pm 4.10 \right) \times 10^{-7} while the 252{}^{252}Cf fission neutron efficiency becomes (2.78±0.38)×10−3\left( 2.78 \pm 0.38 \right) \times 10^{-3}.Comment: Final results, figures, and text; published in Nuclear Instruments and Methods in Physics Research Section

    Development of a lithium-glass based composite neutron detector for He replacement

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    Comment on "Evidence for Neutrinoless Double Beta Decay"

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    We comment on the recent claim for the experimental observation of neutrinoless double-beta decay. We discuss several limitations in the analysis provided in that paper and conclude that there is no basis for the presented claim.Comment: A comment written to Modern Physics Letters A. 4 pages, no figures. Updated version, accepted for publicatio

    Project 8 Phase III Design Concept

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    We present a working concept for Phase III of the Project 8 experiment, aiming to achieve a neutrino mass sensitivity of 2 eV2~\mathrm{eV} (90 %90~\% C.L.) using a large volume of molecular tritium and a phased antenna array. The detection system is discussed in detail.Comment: 3 pages, 3 figures, Proceedings of Neutrino 2016, XXVII International Conference on Neutrino Physics and Astrophysics, 4-9 July 2016, London, U

    Results from the Project 8 phase-1 cyclotron radiation emission spectroscopy detector

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    The Project 8 collaboration seeks to measure the absolute neutrino mass scale by means of precision spectroscopy of the beta decay of tritium. Our technique, cyclotron radiation emission spectroscopy, measures the frequency of the radiation emitted by electrons produced by decays in an ambient magnetic field. Because the cyclotron frequency is inversely proportional to the electron's Lorentz factor, this is also a measurement of the electron's energy. In order to demonstrate the viability of this technique, we have assembled and successfully operated a prototype system, which uses a rectangular waveguide to collect the cyclotron radiation from internal conversion electrons emitted from a gaseous 83m^{83m}Kr source. Here we present the main design aspects of the first phase prototype, which was operated during parts of 2014 and 2015. We will also discuss the procedures used to analyze these data, along with the features which have been observed and the performance achieved to date.Comment: 3 pages; 2 figures; Proceedings of Neutrino 2016, XXVII International Conference on Neutrino Physics and Astrophysics, 4-9 July 2016, London, U
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