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Ricochet

Search for the Coherent Elastic Nuclear Scattering of Neutrinos from a reactor

 Reactor hall, H7 position, 8.8 m from the reactor core

ILL site  
Start position8m from the reactor coreneutrino flux (1.2 1012 ν/cm2/s)
Available space3 m wide x 6 m long x 3.5 m highbelow 15 m water equivalent (m.w.e.) against cosmic radiations
Backgroundswell characterizedwell-shielded against irradiation from the reactor and neighboring instruments (IN20 and D19)
Cryostat and shielding  
Hexa-Dry 200 Ultra-quiet cryostat
CryoConcept company), France
Dry cryogen-free
Ultra-quiet technology
cold stages at 50K, 4K, 1K, 100 mK and 10 mK
 10 mK stageholds the detector
 1 K stageholds cold shielding & cold-front end electronics
Vibrations  
must be suppressed > 50 Hzinsulation of inner frame from the floorpassive with visco-elastic materials
Height40 mm 
Backgrounds  
cosmogenic and radiogenicCRY (cosmic rays) and MCNP modelsGeant4 simulations
Expected 350 Hz muon-veto trigger ratedead-time between 20-30% 
Detector  
CryoCubearray of 27 (3×3×3) high purity germanium crystal detectorsencapsulated in a radio-pure infrared-tight copper box
Particle identification threshold100eV 

INSTRUMENT DESCRIPTION

Ricochet is deployed at the ILL-H7 site in the reactor hall.

The H7 site starts at about 8 m from the ILL reactor core that provides a nominal nuclear power of 58.3 MW, leading to a neutrino flux at the Ricochet detectors 8.8 m from the reactor core of about 1.2×1012 cm−2s−1. The reactor is operated in cycles of typically 50 days’ duration with reactor-off periods sufficiently long to measure reactor-independent backgrounds, such as internal radioactivity or cosmogenic induced backgrounds, with high statistics. The available space is about 3 m wide, 6 m long and 3.5 m high. It is located below a water channel providing about 15 m water equivalent (m.w.e.) against cosmic radiations. It is not fed by a neutron beam and is well-shielded against irradiation from the reactor and neighboring instruments (IN20 and D19).