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LENS-CAL I. Barabanov, V. Gurentsov, V. Kornoukhov Institute for Nuclear Research, Moscow and R. S. Raghavan, Virginia Tech LONU-LENS Blacksburg, Oct 15, 2006. Nuclear Matrix Element for Indium Neutrino Capture Reaction. The Capture Cross Section is
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LENS-CAL I. Barabanov, V. Gurentsov, V. Kornoukhov Institute for Nuclear Research, Moscow and R. S. Raghavan, Virginia Tech LONU-LENS Blacksburg, Oct 15, 2006
Nuclear Matrix Element for Indium Neutrino Capture Reaction The Capture Cross Section is σ = 1.632 x10-44 x [gA2 B(GT)] We pe F(ZW)] gA2 = 1.58 We Prompt Electron energy in mc2 units pe Electron momentum = √ (We2 – 1) F(Z=50, We) Fermi function B(GT) is reduced Gamow Teller Nuclear Matrix Element B(GT) must be calculated/ measured in Laboratory Theoretical Estimate made in RSR original PRL paper: Using nuclear systematics and shell model parameters of the The In (initial) and Sn (final) states: B(GT) ~ 0.16 :
Measurement: J. Rapaport et al, Phys.Rev. Letters 54, 2325 (1985) Performed via 115In(p,n) forward scattering at Indiana U Cyclotron σ (p,n) is proportional to B(GT) Forward (0o) neutron emission with. Ep= 120 MeV and 200 MeV B calibrated against B(F)= 3 for Analog state Result: B(GT) (neutrino state) = 0.17 (10%) B(GT) ~0 to states upto 4 MeV V. good agreement with rsr theory In-Sn neutrino state Neutrino state
Neutrino Source Calibration of B(GT) • In(p,n) reaction is strong interaction reaction which measures B(GT) via strong interactions. • Desirable to have direct weak interaction measurement of B(GT) • Direct measurement using a megCuri neutrino source. • LENS-CAL Source Technology & Expertise developed in Russia (SAGE detector calibration with 51Cr and 37 Ar Sources) LENS-CAL MegaCurie source made in Russia + Compact In loaded detector Operated probably in Baksan
Table I: Characteristics of neutrino Sources for LENS-CAL Neutrino Energy typically 700 keV
Source Energy ~700 keV OK for LENS-CAL First: No other excited state reached. LENS tag ensures excitation of specific state in daughter Sn. Usual problem in radiochem expts such Ga is not present here Second: Energy beyond In beta Endpoint. So double Coincidence enough Simplified tag analysis
Design Concepts for LENS-Cal Detector • Indium Density • Consider a neutrino source in the center of a spherical detector • The event yield Y is: • Y= σερ{ S /(4π r2 )} k 4π r2 dr = σε kρR(= radius of detector) • -k = the fraction of 4π enclosed by the detector array (k ≤1) • ε = the signal detection efficiency In foil thickness • Y varies as ρ the Indium Density. • Need design with high Indium density • In LS typically In is 8% -15% • Can this be increased? • In foil –Plastic Sandwich Stack Detector
Basic Idea of Sandwich Stack -- Use thin Indium foil sandwiched by thin plastic bar Thicknesses: Indium foil Signal electron emerge with high efficiency Plastic thickness > range of electron Optimized thicknesses: In foil 70-100 mg/cm2 Plastic: 300 mg/cm2 Good for Eν ~700 keV
In Sandwich Stack Expts Bell Labs 1979 Original Intent –pp neutrinos ! very thin In foil <10mg/cm2 plastic 160mg/cm2 ρ~60g/l Compared to Ar source: In foil 100mg and Plastic 300 mg ρ~330 g/l Sandwich stack design offers X2.2 higher Indium density Modules with Stacks 20x20x200cm Light attenuation OK Recent INR Monte Carlos Verify
LENS-CAL: Conceptual Design based on Sandwich Stack In Loading Side view Plan view 60 60 60 37Ar 37Ar Ar 37 360 Indium = 8 tons Plastic 25 tons. Indium 100mg/cm2 Plastic 300mg/cm2 Indium Density ρ= 0.33 g/cm3. Plastic Module 20x20x200 max Light guides/PMT’s
Preliminary Simulation Results 51Cr source with activity - 5 mCq Neutrino cross-section capture – 3.03x10-44 cm2 In thickness 0.1 g/cm2 Scintillator slab thickness 3 mm Threshold for neutrino electron – 450 keV Threshold of shower energy - 300 keV. Total In mass – 5 t Module cross section 5*5 cm2 10*10 cm2 15*15 cm2 Neutrino detection efficiency, % 31 26 22 Background (total) per day 1.5 2. 4.4 Number of neutrino events per 100 d 1515 1271 1075 Good Event Rate and Low intrinsic In Bgd.
New Physics from LENS Cal? • Look for Sterile Neutrino Oscillations in LENS-CAL • L. Mikaelyan et al, hep-ph/0310246; Jonathan Link • LSND Δm2 ~1eV2 ~104 x Δm122 of reactor νe ̃ • sin2 2θ ~0.1to 0.001 • Test at short baselines <10m available in LENS-CAL • Kamland 105 m x10-4 (0.7/3 MeV) ~ 2m in LENS-CAL • Look for event rate distribution vs. radius in LENS-CAL detector ! [i] LSND Collaboration, Phys. Rev.Lett. 79 (1998) 1774 [ii]KamLand Collaboration, Phys. Rev. Lett. 94 (2005) 081801
Conclusions Preliminary Analysis Shows Indium sandwich Stack Detectors with Technically feasible 51Cr sources are viable Further work for: other sources Source Strengths …. Revisit In LS modules lower density but higher efficiency