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Measurement of the ambient neutron flux and spectral distribution at the Canfranc Underground Laboratory

S. E. A. Orrigo, J. L. Tain, N. Mont-Geli, A. Tarifeño-Saldivia, L. M. Fraile, M. Grieger, A. Quero-Ballesteros, J. Agramunt, A. Algora, D. Bemmerer, F. Calviño, G. Cortés, A. De Blas, I. Dillmann, R. García, E. Nacher

Abstract

We report on the measurement of the ambient neutron flux and its energy distribution over a broad range of neutron energies, conducted in Hall A of the Canfranc Underground Laboratory using the High Efficiency Neutron Spectrometry Array (HENSA). In particular, we obtained a thermal neutron flux of $3.4(2) \times 10^{-6}$ cm$^{-2}$ s$^{-1}$ and a total energy-integrated flux of $14.8(2) \times 10^{-6}$ cm$^{-2}$ s$^{-1}$. This work represents the first long-term measurement of the total neutron flux, with full spectral characterization across a wide energy interval, performed in an underground laboratory to date. The results are relevant for rare-event search experiments located underground, ranging from nuclear astrophysics to astroparticle physics.

Measurement of the ambient neutron flux and spectral distribution at the Canfranc Underground Laboratory

Abstract

We report on the measurement of the ambient neutron flux and its energy distribution over a broad range of neutron energies, conducted in Hall A of the Canfranc Underground Laboratory using the High Efficiency Neutron Spectrometry Array (HENSA). In particular, we obtained a thermal neutron flux of cm s and a total energy-integrated flux of cm s. This work represents the first long-term measurement of the total neutron flux, with full spectral characterization across a wide energy interval, performed in an underground laboratory to date. The results are relevant for rare-event search experiments located underground, ranging from nuclear astrophysics to astroparticle physics.
Paper Structure (3 equations, 3 figures, 1 table)

This paper contains 3 equations, 3 figures, 1 table.

Figures (3)

  • Figure 1: HENSA response to neutrons simulated with GEANT4. Moderators and covering materials are indicated.
  • Figure 2: Energy spectrum of the ambient neutron flux in Hall A of LSC, obtained by deconvoluting the measured neutron rate Orr_2022 with the detector response shown in Fig. \ref{['Fig1']}, using two different algorithms Tain_2007: BAYES (red dashed line) and CHIMEM (blue solid line). The black dotted line represents the prior flux distribution Mon_2021, used as the initial solution in both iterative algorithms, with the value in the first energy bin fixed to our determined thermal flux value (see the text).
  • Figure 3: Reconstructed neutron counting rate using BAYES (red dashed line) and CHIMEM (blue solid line), compared with the data from Orr_2022 (black points).