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LENS Low Energy Neutrino Spectroscopy

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LENS - Low Energy Neutrino Spectroscopy. Thomas Bowles. Los Alamos ... C. Buck, W. Hampel, F. Hartmann, J. Kiko, D. Motta, T. Kirsten, S. Schoenert, H.Simgen ... – PowerPoint PPT presentation

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Title: LENS Low Energy Neutrino Spectroscopy


1
LENS - Low Energy Neutrino Spectroscopy
  • Thomas Bowles
  • Los Alamos National Laboratory /
  • University of Washington
  • TAUP 03
  • University of Washington
  • September 6, 2003

Nuclear Physics
2
LENS Collaboration
  • College de France, Paris
  • A. de Belefon, T. Beau, H. de Kerret, D. Kryn, M.
    Obolensky, D. Vignaud
  • Dapnia, CEA/Saclay
  • J. Bouchez, P. Bourgeois, C. Cavata, R. Chipaux,
    M. Cribier, G. Fioni, T.Lassere,
  • J. Mallet, J.P. Meyer, C. Veyssiere, H. Zaccone
  • Max Planck Inst. fur Kernphysik, Heidelberg
  • C. Buck, W. Hampel, F. Hartmann, J. Kiko, D.
    Motta,
  • T. Kirsten, S. Schoenert, H.Simgen
  • LNGS, Gran Sasso
  • M. Balata, V. Berezinsky, A. Bettini, C.
    Cattadori, N. Ferrari
  • RCNP, Univ. Osaka M. Fujiwara
  • Institute of Nuclear Research RAS
  • I.R. Barabanov, V.I. Beresnev, L.B. Bezrukov,
    V.I. Gurentsov, V.N. Kornoukhov,
  • N.P. Nesterova, O.G. Ryazhskaya, E.A. Yanovitch,
    G. T. Zatsepin
  • Inst. of Physical Chemistry RAS
  • N. A. Danilov, V. M. Gelis , G. V. Korpusov, G.
    V. Kostikova, Yu. S. Krylov
  • Inst. of Chemical Technology V. V. Yakshin
  • Inst. for Theoretical Exptl. Physics B.
    Kochurov, V. Konev
  • Bell Laboratories R. S. Raghavan

Nuclear Physics
3
LENS Physics Goals
  • p-p flux is the standard candle for solar
    neutrinos
  • Measure the ne flux of p-p and 7Be to a few
    accuracy
  • Measure the ne flux of CNO to 10
  • Search for sterile neutrino component at few
    level
  • (requires a measurement of p-p NC)
  • Search for CPT violation at few level
  • (combined with KamLAND results)
  • Push towards improved accuracy on q12
  • (requires 1-2 accuracy)
  • Requires detector with
  • low threshold (100 keV)
  • p-p count rates (1000 cts/yr)
  • high S/B ( 10/1)
  • calibration of reaction cross section to few
    accuracy
  • (multi-MCi 51Cr source calibration)

Nuclear Physics
4
LENS - CC Reaction Signature
115In count rate 95 p-p events/yr/ton
Signature is inverse b correlated spatially and
temporally with (e/g)2 and g3
115In b decay rate is 250 kHz/ton!
Nuclear Physics
5
LENS Detector Design
Nuclear Physics
6
LENS RD Issues
Nuclear Physics
7
Light Yield as a function of In loading
New Indium-carbhydroxide LS formulation (August
02 LNGS-INR)
Optical Properties In-LS 4 g/l BPO 15 mg /l
bisMSB
LY 100 is for pure Pseudocumene 5 g/l BPO
INFN / INR
Gran Sasso National Laboratory
8
Comparison of pure PC and InLS
InLS (BPO 5 g/l) In 85 g/l PC (BPO
5g/l) LY 67 _at_ In 80 g/l
Pure PC (green) and InLS (red) (new
LNGS-INR formulation)
INFN / INR
Gran Sasso National Laboratory
9
In Acac scintillator (45g/l Indium)
Performances in 5cm x 5cm x 100cm prototype
cell 137Cs source at center
Compton back-scattering-peak (deposited energy
477keV)
  • En. Res. (1?) 11.6
  • Space Res. (1?) 7cm
  • Light at center 200 pe/MeV
  • Effective Att. Length 128cm

10
Status - Scintillator RD
Nuclear Physics
11
LENS Low-Level Background Facility at Gran Sasso
Nuclear Physics
12
First background results from LENS prototype
detector at LLBF
LENS-LLBF Inner Array
Integral bkg rate 2.1x10-3 c/s/kg (single hits,
50 keV threshold)
14C/12C 10-17 in PXE (measured in 2 liter cell!)
13
Status - Detector RD
Nuclear Physics
14
LENS Future Plans
  • Early 2004
  • Complete scintillator and detector RD
  • Complete background measurements in LLBF
  • Finalize design for full-scale detector
  • Appears likely that In-LENS will be technically
    feasible
  • Potentially measure p-p to 3-4, 7Be to
    4-5, CNO to 10

But the price you pay is Achieving S/B gt 3
requires e (p-p) 25) In loading likely to
be limited to 4-5 Total scintillator volume
driven into kiloton range Fine segmentation
required leads to gt 45,000 PMTs Total cost
is likely to be 70M
  • LENS collaboration to decide on proposal in
    spring 2004

Nuclear Physics
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