Full-text resources of PSJD and other databases are now available in the new Library of Science.
Visit https://bibliotekanauki.pl

PL EN


Preferences help
enabled [disable] Abstract
Number of results
2018 | 133 | 4 | 923-927

Article title

Low Background CdWO₄ Scintillation Detector

Content

Title variants

Languages of publication

EN

Abstracts

EN
Low background scintillation setup has been developed that exhibits 3 orders of magnitude lower counting rate of a large volume (2.1 kg) CdWO₄ detector in the energy region 0.5-2.6 MeV, and one order of magnitude above 3 MeV. The background reduction was achieved by application of radiopure passive shield, active plastic-scintillation muon veto placed above the setup and pulse-shape discrimination. Construction of additional plastic scintillation counters is in progress to reduce the residual cosmic muons background. The setup can be applied to develop radiopure scintillators, measure radioactive contamination of materials, carry out small scale low counting experiments.

Keywords

EN

Year

Volume

133

Issue

4

Pages

923-927

Physical description

Dates

published
2018-04

Contributors

  • Institute for Nuclear Research NAS Ukraine, pr. Nauki 47, Kyiv, 03028, Ukraine
author
  • Institute for Nuclear Research NAS Ukraine, pr. Nauki 47, Kyiv, 03028, Ukraine
  • CSNSM, Univ. Paris-Sud, CNRS/IN2P3, Univ. Paris-Saclay, Batiments 104 et 108, 91405 Orsay Campus, France
author
  • Institute for Nuclear Research NAS Ukraine, pr. Nauki 47, Kyiv, 03028, Ukraine
  • Institute for Nuclear Research NAS Ukraine, pr. Nauki 47, Kyiv, 03028, Ukraine
author
  • Institute for Nuclear Research NAS Ukraine, pr. Nauki 47, Kyiv, 03028, Ukraine

References

  • [1] R.L. Brodzinski, J.H. Reeves, F.T. Avignone III, H.S. Miley, J. Radioanal. Nucl. Chem. 124, 513 (1988) , doi: 10.1007/BF02041340
  • [2] G. Heusser, Ann. Rev. Nucl. Part. Sci. 45, 543 (1995) , doi: 10.1146/annurev.ns.45.120195.002551
  • [3] F.A. Danevich, A.Sh. Georgadze, V.V. Kobychev, B.N. Kropivyansky, A.S. Nikolaiko, O.A. Ponkratenko, V.I. Tretyak, S.Yu. Zdesenko, Yu.G. Zdesenko, Phys. Rev. C 68, 035501 (2003) , doi: 10.1103/PhysRevC.68.035501
  • [4] P. Belli, R. Bernabei, V.B. Brudanin, F. Capella, V. Caracciolo, R. Cerulli, D.M. Chernyak, F.A. Danevich, S. d'Angelo, A. Di Marco, A. Incicchitti, M. Laubenstein, V.M. Mokina, D.V. Poda, O.G. Polischuk, V.I. Tretyak, I.A. Tupitsyna, Phys. Rev. C 93, 045502 (2016) , doi: 10.1103/PhysRevC.93.045502
  • [5] S. Umehara, T. Kishimoto, I. Ogawa, R. Hazama, H. Miyawaki, S. Yoshida, K. Matsuoka, K. Kishimoto, A. Katsuki, H. Sakai, D. Yokoyama, K. Mukaida, S. Tomii, Y. Tatewaki, T. Kobayashi, A. Yanagisawa, Phys. Rev. C 78, 058501 (2008) , doi: 10.1103/PhysRevC.78.058501
  • [6] R. Bernabei, P. Belli, F. Capella, R. Cerulli, C.J. Dai, A. d'Angelo, H.L. He, A. Incicchitti, H.H. Kuang, X.H. Ma, F. Montecchia, F. Nozzoli, D. Prosperi, X.D. Sheng, R.G. Wang, Z.P. Ye, Eur. Phys. J. C 67, 39 (2010) , doi: 10.1140/epjc/s10052-010-1303-9
  • [7] S.C. Kim, H. Bhang, J.H. Choi, W.G. Kang, B.H. Kim, H.J. Kim, K.W. Kim, S.K. Kim, Y.D. Kim, J. Lee, J.H. Lee, J.K. Lee, M.J. Lee, S.J. Lee, J. Li, J. Li, X.R. Li, Y.J. Li, S.S. Myung, S.L. Olsen, S. Ryu, I.S. Seong, J.H. So, Q. Yue, Phys. Rev. Lett. 108, 181301 (2012) , doi: 10.1103/PhysRevLett.108.181301
  • [8] P. Belli, R. Bernabei, N. Bukilic, F. Capella, R. Cerulli, C.J. Dai, F.A. Danevich, J.R. de Läter, A. Incicchitti, V.V. Kobychev, S.S. Nagorny, S. Nisi, F. Nozzoli, D.V. Poda, D. Prosperi, V.I. Tretyak, S.S. Yurchenko, Phys. Rev. C 76, 064603 (2007) , doi: 10.1103/PhysRevC.76.064603
  • [9] F.A. Danevich, A.Sh. Georgadze, V.V. Kobychev, S.S. Nagorny, A.S. Nikolaiko, O.A. Ponkratenko, V.I. Tretyak, S.Yu. Zdesenko, Yu.G. Zdesenko, Phys. Rev. C 67, 014310 (2003) , doi: 10.1103/PhysRevC.67.014310
  • [10] C. Arnaboldi, J.W. Beeman, O. Cremonesi, L. Gironi, M. Pavan, G. Pessina, S. Pirro, E. Previtali, Astropart. Phys. 34, 143 (2010) , doi: 10.1016/j.astropartphys.2010.06.009
  • [11] J.W. Beeman, F.A. Danevich, V.Ya. Degoda, E.N. Galashov, A. Giuliani, V.V. Kobychev, M. Mancuso, S. Marnieros, C. Nones, E. Olivieri, G. Pessina, C. Rusconi, V.N. Shlegel, V.I. Tretyak, Ya.V. Vasiliev, Phys. Lett. B 710, 318 (2012) , doi: 10.1016/j.physletb.2012.03.009
  • [12] H. Bhang et al., J. Phys. Conf. Ser. 375, 042023 (2012) , doi: 10.1088/1742-6596/375/4/042023
  • [13] J.W. Beeman, F. Bellini, L. Cardani, N. Casali, I. Dafinei, S. Di Domizio, F. Ferroni, L. Gironi, A. Giuliani, S. Nagorny, F. Orio, L. Pattavina, G. Pessina, G. Piperno, S. Pirro, E. Previtali, C. Rusconi, C. Tomei, M. Vignati, JINST 8, P05021 (2013) , doi: 10.1088/1748-0221/8/05/P05021
  • [14] D.R. Artusa et al., Eur. Phys. J. C 74, 3096 (2014) , doi: 10.1140/epjc/s10052-014-3096-8
  • [15] T.B. Bekker, N. Coron, F.A. Danevich, V.Ya. Degoda, A. Giuliani, V.D. Grigorieva, N.V. Ivannikova, M. Mancuso, P. de Marcillac, I.M. Moroz, C. Nones, E. Olivieri, G. Pessina, D.V. Poda, V.N. Shlegel, V.I. Tretyak, M. Velazquez, Astropart. Phys. 72, 38 (2016) , doi: 10.1016/j.astropartphys.2015.06.002
  • [16] G. Angloher et al., Eur. Phys. J. C 72, 1971 (2012) , doi: 10.1140/epjc/s10052-012-1971-8
  • [17] G. Wang et al., arXiv: 1504.03599, [physics.ins-det] (2015) http://arXiv.org/abs/1504.03599
  • [18] D.V. Poda, et al., Rad. Measur. 56, 66 (2013) , doi: 10.1016/j.radmeas.2013.02.017
  • [19] T. Fazzini, P.G. Bizzeti, P.R. Maurenzig, C. Stramaccioni, F.A. Danevich, V.V. Kobychev, V.I. Tretyak, Yu.G. Zdesenko, Nucl. Instrum. Methods Phys. Res. A 410, 213 (1998) , doi: 10.1016/S0168-9002(98)00179-X
  • [20] E.N. Galashov, V.A. Gusev, V.N. Shlegel, Ya.V. Vasiliev, Crystallogr. Rep. 54, 689 (2009) , doi: 10.1134/S1063774509040245
  • [21] P. Belli et al., Nucl. Instrum. Methods Phys. Res. A 615, 301 (2010) , doi: 10.1016/j.nima.2010.01.081
  • [22] A.A. Pavlyuk, Ya.V. Vasiliev, L.Yu. Kharchenko, F.A. Kuznetsov, in: Proc. APSAM-92, Asia Pacific Society for Advanced Materials, Shanghai, 1992, Institute of Materials Research, Tohoku University, Sendai 1993, p. 164
  • [23] V.I. Tretyak, Astropart. Phys. 33, 40 (2010) , doi: 10.1016/j.astropartphys.2009.11.002
  • [24] M. Bektasoglu, H. Arslan, Pramana J. Phys. 80, 837 (2013) , doi: 10.1007/s12043-013-0519-2

Document Type

Publication order reference

Identifiers

YADDA identifier

bwmeta1.element.bwnjournal-article-appv133n4p38kz
JavaScript is turned off in your web browser. Turn it on to take full advantage of this site, then refresh the page.