Neutron flux and spectrum in the Dresden Felsenkeller underground facility studied by moderated He3 counters

M. Grieger, T. Hensel, J. Agramunt, D. Bemmerer, D. Degering, I. Dillmann, L. M. Fraile, D. Jordan, U. Köster, M. Marta, S. E. Müller, T. Szücs, J. L. Taín, and K. Zuber
Phys. Rev. D 101, 123027 – Published 24 June 2020

Abstract

Ambient neutrons may cause significant background for underground experiments. Therefore, it is necessary to investigate their flux and energy spectrum in order to devise a proper shielding. Here, two sets of altogether ten moderated He3 neutron counters are used for a detailed study of the ambient neutron background in tunnel IV of the Felsenkeller facility, underground below 45 m of rock in Dresden/Germany. One of the moderators is lined with lead and thus sensitive to neutrons of energies higher than 10 MeV. For each He3 counter moderator assembly, the energy-dependent neutron sensitivity was calculated with the FLUKA code. The count rates of the ten detectors were then fitted with the MAXED and GRAVEL packages. As a result, both the neutron energy spectrum from 109 to 300 MeV and the flux integrated over the same energy range were determined experimentally. The data show that at a given depth, both the flux and the spectrum vary significantly depending on local conditions. Energy-integrated fluxes of (0.61±0.05), (1.96±0.15), and (4.6±0.4)×104cm2s1, respectively, are measured for three sites within Felsenkeller tunnel IV which have similar muon flux but different shielding wall configurations. The integrated neutron flux data and the obtained spectra for the three sites are matched reasonably well by FLUKA Monte Carlo calculations that are based on the known muon flux and composition of the measurement room walls.

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  • Received 25 January 2019
  • Accepted 4 June 2020

DOI:https://doi.org/10.1103/PhysRevD.101.123027

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Particles & FieldsNuclear PhysicsGravitation, Cosmology & Astrophysics

Authors & Affiliations

M. Grieger1,2, T. Hensel1,2, J. Agramunt3, D. Bemmerer1,*, D. Degering4, I. Dillmann5, L. M. Fraile6, D. Jordan3, U. Köster7, M. Marta5, S. E. Müller1, T. Szücs1, J. L. Taín3, and K. Zuber2

  • 1Helmholtz-Zentrum Dresden-Rossendorf (HZDR), 01328 Dresden, Germany
  • 2Technische Universität Dresden, 01062 Dresden, Germany
  • 3Instituto de Física Corpuscular, CSIC and Universitat de Valencia, E-46980 Paterna, Spain
  • 4VKTA—Strahlenschutz, Analytik & Entsorgung Rossendorf, 01328 Dresden, Germany
  • 5GSI Helmholtzzentrum für Schwerionenforschung, 06159 Darmstadt, Germany
  • 6Grupo de Física Nuclear & IPARCOS, Universidad Complutense de Madrid, 28040 Madrid, Spain
  • 7Institut Laue-Langevin (ILL), 38042 Grenoble, France

  • *d.bemmerer@hzdr.de

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Vol. 101, Iss. 12 — 15 June 2020

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