Standard

High dynamic range measurement of CdWO4 afterglow. / Postupaev, V. V.

в: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Том 923, 11.04.2019, стр. 147-156.

Результаты исследований: Научные публикации в периодических изданияхстатьяРецензирование

Harvard

Postupaev, VV 2019, 'High dynamic range measurement of CdWO4 afterglow', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, Том. 923, стр. 147-156. https://doi.org/10.1016/j.nima.2019.01.090

APA

Postupaev, V. V. (2019). High dynamic range measurement of CdWO4 afterglow. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 923, 147-156. https://doi.org/10.1016/j.nima.2019.01.090

Vancouver

Postupaev VV. High dynamic range measurement of CdWO4 afterglow. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2019 апр. 11;923:147-156. doi: 10.1016/j.nima.2019.01.090

Author

Postupaev, V. V. / High dynamic range measurement of CdWO4 afterglow. в: Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 2019 ; Том 923. стр. 147-156.

BibTeX

@article{26d23f0c7a534b72a85a70e831065e38,
title = "High dynamic range measurement of CdWO4 afterglow",
abstract = "The notable feature of cadmium tungstate (CWO) is quite long (∼14.5μs) decay time of its brightest scintillation component. In this paper, the technique and results of high dynamic range measurements of CWO afterglow are discussed. Samples were irradiated by bremsstrahlung of a ∼0.5 MeV, 6μs electron beam. The afterglow tail of the scintillation curve was measured down to the relative amplitude <10−5. At such intensities, a parasitic fluorescence of a photomultiplier essentially contributes to the total signal. The CWO light emission dynamics is determined by known scintillation components to at least 10−5 level. Constraints on the existence of a possible slower fluorescence component are discussed.",
keywords = "Afterglow, Cadmium tungstate, CdWO, Scintillator, SYSTEM, DETECTORS, SCINTILLATORS, CdWO4, CRYSTAL",
author = "Postupaev, {V. V.}",
note = "Publisher Copyright: {\textcopyright} 2019 Elsevier B.V.",
year = "2019",
month = apr,
day = "11",
doi = "10.1016/j.nima.2019.01.090",
language = "English",
volume = "923",
pages = "147--156",
journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",
issn = "0168-9002",
publisher = "Elsevier Science B.V.",

}

RIS

TY - JOUR

T1 - High dynamic range measurement of CdWO4 afterglow

AU - Postupaev, V. V.

N1 - Publisher Copyright: © 2019 Elsevier B.V.

PY - 2019/4/11

Y1 - 2019/4/11

N2 - The notable feature of cadmium tungstate (CWO) is quite long (∼14.5μs) decay time of its brightest scintillation component. In this paper, the technique and results of high dynamic range measurements of CWO afterglow are discussed. Samples were irradiated by bremsstrahlung of a ∼0.5 MeV, 6μs electron beam. The afterglow tail of the scintillation curve was measured down to the relative amplitude <10−5. At such intensities, a parasitic fluorescence of a photomultiplier essentially contributes to the total signal. The CWO light emission dynamics is determined by known scintillation components to at least 10−5 level. Constraints on the existence of a possible slower fluorescence component are discussed.

AB - The notable feature of cadmium tungstate (CWO) is quite long (∼14.5μs) decay time of its brightest scintillation component. In this paper, the technique and results of high dynamic range measurements of CWO afterglow are discussed. Samples were irradiated by bremsstrahlung of a ∼0.5 MeV, 6μs electron beam. The afterglow tail of the scintillation curve was measured down to the relative amplitude <10−5. At such intensities, a parasitic fluorescence of a photomultiplier essentially contributes to the total signal. The CWO light emission dynamics is determined by known scintillation components to at least 10−5 level. Constraints on the existence of a possible slower fluorescence component are discussed.

KW - Afterglow

KW - Cadmium tungstate

KW - CdWO

KW - Scintillator

KW - SYSTEM

KW - DETECTORS

KW - SCINTILLATORS

KW - CdWO4

KW - CRYSTAL

UR - http://www.scopus.com/inward/record.url?scp=85073151434&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2019.01.090

DO - 10.1016/j.nima.2019.01.090

M3 - Article

AN - SCOPUS:85073151434

VL - 923

SP - 147

EP - 156

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

SN - 0168-9002

ER -

ID: 21861366