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The Future of Neutrino Physics

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The Future of Neutrino Physics. SUPA Particle Physics Theme Launch. 12 October 2005 ... Magnetised iron calorimeter? Liquid argon TPC? Totally active scintillator? ... – PowerPoint PPT presentation

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Title: The Future of Neutrino Physics


1
The Future of Neutrino Physics
SUPA Particle Physics Theme Launch 12 October
2005 Paul Soler University of Glasgow
2
Contents
1. Present knowledge 1.1 Global fits 1.2 Unknown
facts 2. CP violation and q13 2.1 Super-beams 2.2
Neutrino factory concept 2.3 Physics reach of a
neutrino factory 2.4 Beta beams? 3.
Non-oscillation physics 4. Double beta decay 5.
UK activities in Neutrino Factories 5.1 Targets,
proton drivers 5.2 Hadron production yields 5.3
MICE
3
1. Present knowledge
Neutrino oscillations discovered. Mixing
described by
For 3-flavour eigenstates U is Maki-Nakagawa-Sakat
a (MNS)
6 parameters 3 mixing angles - ?23,?12 and
?13 CP-violation angle - d
2 mass differences - ?m223 and ?m212
Transition probability
4
1.1 Global fits
  • Consistent picture emerging
  • Information from atmospheric neutrinos, solar
    neutrinos, KamLand and reactor experiments used
    to extract parameters
  • Global fit provides q23, q12, Dm122 and Dm232

5
1.2 Unkown facts
  • q13 not known
  • CP violation phase d not known.
  • Absolute neutrino mass scale not known
  • Are neutrinos Majorana (ie. its own antiparticle)
    or Dirac
  • Are there sterile neutrinos?
  • Mass hierarchy not known

6

2. CP Violation and q13
  • First need to determine q13 using neutrino
    super-beams
  • Do nm?ne oscillations and fit sin2q13 to
  • Off-axis beams with 1-4 MW proton intensity
  • Japanese T2K (Tokai to SuperK, 250 km) or
  • MINOS off-axis (700 km)

Off-axis narrower energy band
7

2.2 Neutrino factory concept
  • Neutrino factory can provide sufficient neutrino
    luminosity to perform CP violation experiments at
    very long baseline 3000-7000 km.
  • Conceptual design neutrinos produced from muon
    decay in storage ring. Rate calculable by
    kinematics of decay (Michel spectrum)

8
2.3 Physics reach of a neutrino factory
  • Far detector (3000-7000 km) can search for
    wrong-sign muons in appearance mode,
    disappearance of right-sign leptons, either e
    or m and possible appearance of t.
  • Detectors
  • Magnetised iron calorimeter?
  • Liquid argon TPC?
  • Totally active scintillator?
  • Water Cherenkov, other?
  • Can detect sign of Dm232 due to matter effects
    and determine CP violating phase d if it is large
    enough.

9

2.3 Physics reach of a neutrino factory
  • Determine q13 and CP phase d simultaneously need
    1021 muons/year
  • Optimal CP phase sensitivity 6000 km but
  • can obtain gt5s sensitivity for 1000-8000 km

10

2.4 Beta beams?
  • Beta beam beta decay of accelerated radioactive
    nuclei
  • (P. Zucchelli, Phys. Lett. B, 532 (2002),
    166-172.)
  • He-6 for neutrino production g 150
  • Ne-18 for antineutrino production g 60
  • Large Cherenkov detector at 150 km to perform
    oscillation searches.
    Measure CP violation and q13 with less
    background, since no need for charge selection.

d vs q13 sensitivity
11

3. Non-oscillation physics
  • High precision n-p and n-n deep inelastic
    scattering
  • PDFs, nuclear shadowing
  • ?S from xF3 - ??S0.003
  • Vcd and Vcs, D0/ D0 mixing
  • sin2?W - ?sin2?W 0.0001
  • Polarised structure functions
  • Beyond the SM searches
  • n cross-sections for oscillations
  • Other physics
  • High muon flux flavour violating decays,
    muonium, muonic atoms, m-spin rotation,
    electroweak parameters
  • High proton flux nuclear physics (heavy and
    exotic nuclei), nuclear astrophysics, atomic
    physics, medicine, materials,

12
4. Double beta decay
  • Double beta decay 35 possible beta emitters
    (even-even nuclei). Very rare (half-life more
    than 1020 years) since second order process.
  • Beta decay kinematically forbidden and double
    beta kinematically allowed
  • Neutrinoless double beta Majorana character of
    neutrino
  • UK involvement in NEMO, Cobra

Aim 100 meV sensitivity
13
5. UK activities in Neutrino factory RD
  • UK Neutrino Factory Consortium Daresbury,
    Glasgow, Imperial College, Liverpool, Oxford,
    RAL, Sheffield, Warwick
  • Many technological challenges for neutrino
    factory! Cost 2 bn
  • Very high intensity proton drivers (4MW proton
    beams)
  • Targets need to withstand shock-waves from
    protons and very rapid heating mercury jets,
    rotating band or cooled metal beads

14
5.2 Hadron Production Yields
  • Need hadron production yields from protons on
    targets to optimize neutrino factory energies
  • HARP at CERN 2-15 GeV
  • Preliminary results on Al target
  • Useful for K2K expt.

15
5.3 Muon Ionization Cooling Experiment (MICE)

Muon Ionization Cooling Experiment at RAL
demonstrates ionization cooling for neutrino
factory and muon collider
Squeezing of transverse emittance by ionization
and acceleration
MICE Phase I approved!!
Transverse emittance
16
Outlook
  • The Neutrino Factory is the ultimate tool for the
    study of neutrinos
  • UK has established internationally recognised,
    broadly-based NuFact RD activity to demonstrate
    key technologies (not only MICE but also proton
    driver, targetry, neutrino detection etc.)
  • SUPA partners already contributing to neutrino
    factory RD
  • Glasgow, Edinburgh members of MICE MICE beamline
    simulation and diagnostics, measurement of
    emittance.
  • Glasgow member of HARP hadron yields.
  • Faraday partnership RF RD with Strathclyde
    University (Alan Phelps)
  • Scoping study for World Design Study III
  • Initiation of International Scoping Study to
    define parameters of neutrino factory physics,
    machine and detectors.
  • Launched at NUFACT05 one year to define scope
    for World Design Study III based at RAL (design
    studies I II based at BNL and Fermilab).
  • Aim produce robust proposal to EU FP7 for WDS
    (Mar 07)
  • Main Glasgow involvement define detectors for
    neutrino factories
  • SUSSP61 theme on Neutrinos, 8-23 August 2006, St
    Andrews.
  • Many world leading figures in neutrino
    physics invited.
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