Characterization of a 109Cd γ-Ray Source for the Two-Phase Argon Detector
- Authors: Bondar A.E.1,2, Buzulutskov A.F.1,2, Dolgov A.D.2, Legkodymov A.A.1, Nosov V.V.1,2, Oleynikov V.P.1,2, Porosev V.V.1,2, Shemyakina E.O.1,2, Sokolov A.V.1,2
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Affiliations:
- Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences
- Novosibirsk State University
- Issue: Vol 62, No 6 (2019)
- Pages: 746-749
- Section: Nuclear Experimental Technique
- URL: https://ogarev-online.ru/0020-4412/article/view/160945
- DOI: https://doi.org/10.1134/S0020441219050142
- ID: 160945
Cite item
Abstract
A two-phase argon detector is being developed in our laboratory for dark matter search and low-energy neutrino experiments. A 109Cd γ-ray source was used to calibrate the energy scale of the detector. In this paper, a detailed emission spectrum of the 109Cd source was measured using a YAP:Ce based scintillation detector and high-purity germanium detector. It was shown that the 109Cd source equipped with a tungsten substrate and a copper filter can provide a complete set of γ-ray lines in the range from 8 to 90 keV for energy calibration of two-phase detectors. These measurements allowed us to successfully quantify the shape of the amplitude spectrum observed when the two-phase detector was irradiated by the 109Cd source.
About the authors
A. E. Bondar
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
A. F. Buzulutskov
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
A. D. Dolgov
Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090
A. A. Legkodymov
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090
V. V. Nosov
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
V. P. Oleynikov
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Author for correspondence.
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
V. V. Porosev
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
E. O. Shemyakina
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
A. V. Sokolov
Institute of Nuclear Physics, Siberian Branch, Russian Academy of Sciences; Novosibirsk State University
Email: V.P.Oleynikov@inp.nsk.su
Russian Federation, Novosibirsk, 630090; Novosibirsk, 630090
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