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Published byOctavia Wilson Modified over 9 years ago
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Neutrino Oscillations at Homestake from Chlorine to the Megadetector Ancient Origins of the Question ~1860 Darwin publishes “On The Origin of Species”- & Kelvin challenges the time scale – The Sun is less than 30 million years – Gravitational Energy BUT – Kelvin was wrong- The Physics is more interesting
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1946-Bruno Pontecorvo described a novel neutrino detector Neutrino + 37 Cl 37 Ar + e - ∟ 37 Cl + The Atomic Energy Commission classified the paper – This detector could be used to locate Nuclear vessels But the AEC was WRONG The Physics is more interesting e + 37 Cl 37 Ar + e - Reactors emit e
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1965-Ray Davis began construction of the Cl Detector to look for e from H He fusion in the Sun
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1985-The Cl detector observes 2.55 SNU (solar neutrino units) The Solar Model (Bahcall) predicts 8 SNU signal/prediction = 1/3 Conclusion: (a) the measurement is wrong, (b) the model is wrong or (c) both are wrong, The Conclusion is WRONG – The physics is more interesting
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Neutrinos Oscillate - 3 species Pontecorvo(1967) & MSW(1985) But, Solar Neutrino exps. are complicated – unknown source and unknown physics Remedy – Use a known source Reactors – KAMLAND - e Accelerators – Fermilab(& CERN, KEK)- μ
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Neutrino Oscillation Fundamentals 1) Unoscillated interaction rate ~ (Beam power) x (Detector Mass)/L 2 2) Detect & Measure: a) Energy distribution of after oscillation b) Energy distribution of e due to oscillation 3) Backgnd – e from decay of K + e + + e & e from decay of + e + + + e
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Fermilab Beam Power Options 1) Present – 0.7 Megawatts ( of protons) 2) SNuMI – 1.2 Megawatts 3) Project X – 2.0 Megawatts
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Oscillation Lengths For E = 1 GeV, L 23 = 494 km( disappearance) L 13 = 15,420km ( e appearance) Thus, e amplitude grows linearly with distance over any Earth based oscillation path. Signal/uncertainly is L independent since flux varies as 1/L 2 and uncertainly as (flux) ½. Since e from K + and + decays ~1% of flux, want beam path ~ 1/10 L 13 or ~ 1500 km. for signal/bkgnd ~ 10.
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Large Cavern for Long Base Line Experiment Concept (M. Laurenti) Finished Cavern Helical Drift
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Large Cavern for Long Base Line Experiment Concept (M. Laurenti) Finished Cavern Helical Drift
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Large Cavern for Long Base Line Experiment Concept (M. Laurenti) Finished Cavern Helical Drift
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Large Cavern for Long Base Line Experiment Concept Cross Section Helical Drift 4850L 5000L 53M I.D. 85M I.D.
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300 kTand 2 MW generates ~200000 cc evts/yr 300 kT Homestake detector and 2 MW generates ~200000 cc evts/yr
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Spectra with 300 kT detector and 2MW beam from FNAL Background issues examined by FNAL/BNL study. Background issues examined by FNAL/BNL study. NormalReversed sin²2θ ₁₃ = 0.04, 300kT, 1300 km, ~2MW @ 60 GeV 3yrs neutrinos and 3yrs antineutrinos and 3yrs antineutrinos sig~1214 sig~394 sig~564 sig~564 sig~627 Mark Dierckxsens(UChicago), Mary Bishai(BNL)
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Ultimate Reach Mark Dierckxsens(UChicago), Mary Bishai(BNL) Mass ordering θ ₁₃ CP Violation 60 GeV, 2MW, 3+3 yrs, 300kT stat+ 5%syst 0.003 0.007 0.007 50% coverage at 3 sigma
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Technical issues Measure 3-generation parameters without ambiguities. (CP measurement is approximately independent of θ 13 ). Need large detector independent of θ 13 value. 300 kT water Cherenkov detector @DUSEL Measurement of CP phase and Sin²2θ 13 at several points. All ambiguities and mass hierarchy are resolved.
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Developing Collaboration Proposal for an Experimental Program in Neutrino Physics and Proton Decay in the Homestake Laboratory This is the author list of hep-ex/0608023 August 2006
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Other Physics with the Megadetector 1) Nucleon decay ~ 10 35 years 2) Supernova prompt neutrinos – ~10 5 from SN in the Galaxy ~10 – 20 from Andromeda 3) Relic SN neutrinos 4) Solar neutrinos – sure & HOW 5) Atmospheric neutrinos – 6) Also, a great bkgnd shield for sensitive insert experiments
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Nucleon decay Large body of work by HyperK, and UNO. background levels for the positron+Pion mode 3.6/MTon-yr (normal) 0.15/MTon-yr (tight) Expected Sensitivity on K-nu mode is about ~8x10³³ yr Ref: Shiozawa (NNN05) 300kTX10yrs => 7X10³ ⁴ yrs
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HOPEFULLY THE NEW PHYSICS WILL BE MORE INTERESTING
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