Gilles Gerbier for EDELWEISS collab.

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Presentation transcript:

Gilles Gerbier for EDELWEISS collab. Neutron studies within Edelweiss - Lyon/Saclay groups - Update IDM 2004 Gilles Gerbier for EDELWEISS collab. -Edelweiss data : neutron evts ? -Comparison GEANT321 FLUKA -Benchmarks for comparison - neutron primary production

Edelweiss data background E>30 keV, Q<0.5 11 12 5

Incomplete charge collection events Total : E>30 kEV Q>0.5 = 28 evts, last 42 kg.d Upperband : 11 In recoil zone : 5 Lower band : 12 If homogeneous filling of incomplete charge collection evts : expect about 25 % (recoil zone surface/total) of total in recoil zone ie : 7 Observed 5 => no evidence for significant other contribution (neutron)

Neutrons 1 double recoil interaction seen 1 Coincidence recoil recoil evt in bolo1 – bolo2 90 % CL interval (poisson) : 0.051-4.73 evts Probability of double evt ~ 10 % => Expected single at 90 % CL ~ 0.5 - 47 evts !!! Expected rate from rock neutrons Rate of neutron > 1 MeV in LSM is 1.6 10-6 n/cm²/s Propagation with GEANT3/MCNP gave following compatible expectations : Rate > 10 keV = 0.05 evts/kg/d Rate > 30 keV = 0.014 evts/kg/d => expected in 62 kg.d : 3 evts with E >10 keV : 1 evt>30keV

“Recommendations” from Third TECNOmSIQ meeting, Paris 24/01/03

Correction in photonuclear cross section in GEANT321 – Martine Stern IPNL X section integrated from n = 10 MeV Cut 10 meV Cut 140 meV Initial X section n GeV However : no photo production of neutron in secondary shower !!! But try to compare…

Fluka – Vitaly K. Geant 3 – Martine S.

Study of features of primary interaction : energy/mult. in scintillator 100 000 muons crossing 240 cm of scintillator <=> 200 g/cm²

Study of features of primary interaction : energy/mult. in lead 100 000 muons crossing 18 cm of lead

Summary Primary production in scintillator 20 GeV Analyt calc 0.7 10-5 n/mu/g/cm² Mean multiplicity (>= 1) Mean energy 20 GeV Analyt calc 0.7 10-5 0.87 2.1 65 MeV 300 GeV 1.6 10-5 1.8 2.2 117 MeV Delorme et al 1995 Primary production in lead n/mu/g/cm² Mean multiplicity (>= 1) Mean energy 20 GeV 10 10-5 13 14 MeV 300 GeV 20 10-5 16 24 MeV

What next ? Go to GEANT4 ? Get reliability in Production, including other, p, g : FLUKA/GEANT4/exp Propagation + simulation in detector : GEANT4/ MCNP Reestimate neutron rate, recoil rate, E spectra multiplicity for EDW 2 From muons in shield From muons in rock