Neutron flux and spectrum in the Dresden Felsenkeller underground facility studied by moderated He counters
arXiv:2006.02696 · doi:10.1103/PhysRevD.101.123027
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 He neutron counters are used for a detailed study of the ambient neutron background in tunnel IV of the Felsenkeller facility, underground below 45 meters 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 He 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 10 MeV 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 , , and cm s, 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.
10 figures, 4 tables; to be published in Phys. Rev. D
References in corpus (6)
- LUNA: Status and Prospects
- Muon-induced neutrons do not explain the DAMA data
- The muon intensity in the Felsenkeller shallow underground laboratory
- Measuring Muon-Induced Neutrons with Liquid Scintillation Detector at Soudan Mine
- A. Fluka Study of Underground Cosmogenic Neutron Production
- Muon-induced neutrons in lead and copper at shallow depth
Cited by in corpus (14)
- Horizons: Nuclear Astrophysics in the 2020s and Beyond
- The Status and Future of Direct Nuclear Reaction Measurements for Stellar Burning
- Exploring Stars in Underground Laboratories: Challenges and Solutions
- Solar fusion III: New data and theory for hydrogen-burning stars
- A new ultra low-level HPGe activity counting setup in the Felsenkeller shallow-underground laboratory
- The Felsenkeller shallow-underground laboratory for nuclear astrophysics
- Long-term evolution of the neutron rate at the Canfranc Underground Laboratory
- First results from the HENSA/ANAIS collaboration at the Canfranc Underground Laboratory
- Measurement of the neutron flux at the Canfranc Underground Laboratory with HENSA
- Design of a mobile neutron spectrometer for the Laboratori Nazionali del Gran Sasso (LNGS)
- Status and future directions for direct cross-section measurements of the 13C(a,n)16O reaction for astrophysics
- Underground nuclear astrophysics: Status and recent results from Felsenkeller laboratory
- Status of the HENSA collaboration at the Canfranc Underground Laboratory: results from two years of measurement of the neutron flux in hall B
- Measurement of the ambient neutron flux and spectral distribution at the Canfranc Underground Laboratory