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Communication Dans Un Congrès Année : 2019

Ambient neutron background in the shallow-underground laboratory Felsenkeller

T. Hensel
  • Fonction : Auteur
M. Grieger
  • Fonction : Auteur
J. Agramunt
  • Fonction : Auteur
J.L. Taín
  • Fonction : Auteur
D. Bemmerer
  • Fonction : Auteur
S.E. Müller
T. Szücs
  • Fonction : Auteur
D. Degering
  • Fonction : Auteur
I. Dillmann
  • Fonction : Auteur
L.M. Fraile
  • Fonction : Auteur
M. Marta
  • Fonction : Auteur
K. Zuber
  • Fonction : Auteur

Résumé

One important component of the ambient background in underground laboratories are neutrons, which cover a wide energy range from thermal up to 100 MeV. After a few meters rock overburden, cosmic-ray neutrons are a negligible contribution underground and the remaining flux is due to neutron production by cosmic-ray muons and by (α,n) reactions from natural radioactivity in the rock. There are only a few measurements of the full spectral neutron flux available in the literature, a fact which hampers comparisons between laboratories and negatively affects the planning of future experiments. In an effort to overcome this issue a setup consisting of six moderated and one unmoderated 3He neutron counters that has been used at a depth of 850 m in the Canfranc underground laboratory, Spain [1], was utilized to study the neutron flux in the 48 m deep Dresden Felsenkeller underground laboratory, Germany. At Felsenkeller, an additional counter with a lead liner was used in order to address also the high-energy flux up to several hundreds of MeV.
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Dates et versions

hal-02165807 , version 1 (26-06-2019)

Identifiants

Citer

T. Hensel, M. Grieger, J. Agramunt, J.L. Taín, D. Bemmerer, et al.. Ambient neutron background in the shallow-underground laboratory Felsenkeller. 5th International Solar Neutrino Conference, Jun 2018, Dresden, Germany. pp.477-484, ⟨10.1142/9789811204296_0031⟩. ⟨hal-02165807⟩
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