Searching for Muon to Electron Conversion Below the 1016 Level

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Searching for Muon to Electron Conversion Below the 1016 Level

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Searching for Muon to Electron Conversion Below the 10-16 Level. Michael Hebert ... Project start awaits Congressional action; RSVP (MECO KOPIO) is not in the ... –

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Title: Searching for Muon to Electron Conversion Below the 1016 Level


1
Searching for Muon to Electron Conversion Below
the 10-16 Level
  • Michael Hebert
  • UC Irvine
  • PANIC02
  • Osaka, Sept. 29 Oct. 4, 2002

2
MECO Collaboration
Eleven Institutions worldwide at present.
Substantial growth expected following
formal project start
  • Institute for Nuclear Research, Moscow
  • V. M. Lobashev, V. Matushka,
  • New York University
  • R. M. Djilkibaev, A. Mincer,
    P. Nemethy, J. Sculli, A.N. Toropin
  • Osaka University
  • M. Aoki, Y. Kuno, A. Sato
  • University of Pennsylvania
  • W. Wales
  • Syracuse University
  • R. Holmes, P. Souder
  • College of William and Mary
  • M. Eckhause, J. Kane, R. Welsh
  • Boston University
  • J. Miller, B. L. Roberts, O. Rind
  • Brookhaven National Laboratory
  • K. Brown, M. Brennan, G. Greene,
  • L. Jia, W. Marciano, W. Morse,
    Y. Semertzidis, P. Yamin
  • University of California, Irvine
  • M. Hebert, T. J. Liu, W. Molzon, J.
    Popp, V. Tumakov
  • University of Houston
  • E. V. Hungerford, K. A. Lan, L.
    S. Pinsky, J. Wilson
  • University of Massachusetts, Amherst
  • K. Kumar

3
Charged Lepton Flavor Violation
  • Lepton Flavor is NOT conserved in the neutral
    sector as shown by recent neutrino mixing results
  • Lepton Flavor Violation (LFV) in the charged
    sector should occur via n mixing, but far
    below the experimentally accessible range,
    meaning that any observed signal necessarily
    requires new physics
  • Fortunately a wide variety of proposed extensions
    to the Standard Model predict observable LFV
    processes in charged lepton sector

4
One Example
  • SU(5) SUSY- GUT predicts a signal only a few
    orders of magnitude below the current
    experimental limit
  • SO(10) prediction is enhanced by

Courtesy Hisano
MECO single event sensitivity
5
History of Charged LFV Searches
1
  • Goal A four order of magnitude leap in
    sensitivity to the 2 ? 10 17 level for a
    single event
  • Effective mass reach is enormous, e.g. for
    leptoquark exchange

?-N ? e- N ? ? e ? ? ? e e e- K0??
? e- K?? ??e-
10-4
10-8
Sensitivity to Lepton Flavor Violation
10-12
MECO Goal
10-16
1940 1950 1960 1970 1980 1990
2000 2010
Year
6
Muon to Electron Conversion
  • Low energy muons are stopped in Ti foils, forming
    muonic atoms
  • Three possible fates for the muon
  • Nuclear capture
  • Three body decay in orbit
  • Coherent LFV decay
  • Signal is a single mono-energetic electron
  • Single particle signal avoids accidental
    backgrounds at high rate
  • Rate is normalized to the kinematically similar
    weak capture process

7
MECO Features
  • 1000fold increase in muon beam intensity (from
    MELC at MMF)
  • High Z target for improved pion production
  • Axially-graded 5 T solenoidal field to maximize
    pion capture
  • Muon transport in a curved solenoid
    suppressing
    neutrals, positives,
    and high
    momentum negatives
    (new for
    MECO)
  • Pulsed beam to eliminate prompt
    backgrounds
    (A. Baertscher et al.)
  • Beam pulse duration ltlt muon lifetime
  • Pulse separation muon lifetime
  • Extinction between pulses lt 10-9
  • High rate capability and improved acceptance
    electron detectors
  • Axially-graded 2 T solenoidal field for improved
    acceptance (from MELC)
  • Spectrometer with axial components and good
    resolution (new for MECO)

8
Potential Backgrounds
  • Muon Decay in Orbit
  • The dominant background
  • Steeply falling spectrum near endpoint, e.g.
  • Sets required energy resolution
  • Nbkgd 0.25 for Rme 2 ? 10-17 ? DEe 900 keV
    (FWHM)
  • Radiative Muon Capture also eliminated by
    energy resolution
  • Radiative Pion Capture requires beam extinction
    lt 10-9
  • Muon decay in flight e- scattering
    negligible with pulsed beam
  • Beam e- scattering in stopping target
    eliminated by pulsed beam
  • Antiproton induced e- requires thin stopping
    window
  • Cosmic ray induced e- requires active and
    passive shielding

9
The MECO Apparatus
Superconducting Detector Solenoid contains
conversion electron detectors
Superconducting Production Solenoid captures muons
Superconducting Transport Solenoid selects low
momentum m-
10
Production Region
  • Axially graded 5 T solenoid captures pions and
    muons, transporting them toward the stopping
    target
  • Cu and W heat and radiation shield protects
    superconducting coils from effects of 50kW
    primary proton beam

Superconducting coils
2.5 T
Proton Beam
Production Target
Heat Radiation Shield
5 T
11
Transport Solenoid
  • Curved solenoid eliminates
    line-of-sight transport of photons
    and neutrons
  • Curvature drift and collimators sign and momentum
    select beam
  • dB/ds lt 0 in the straight sections to avoid long
    transit time trajectories

2.1 T
Collimators
2.5 T
Curvature Drift
12
Detector Region
  • Axially-graded field near stopping target to
    increase acceptance and reduce cosmic ray
    background
  • Uniform field in spectrometer region to simplify
    momentum analysis
  • Electron detectors downstream of target to reduce
    rates from g and neutrons

Electron Calorimeter
Straw Tracking Detector
Stopping Target Foils
1 T
1 T
2 T
13
Electron Spectrometer Performance
Side View
Axial View
Background with Detector Response
Conversion electron produced in the stopping
target, detected in the Tracker, and triggered in
the Calorimeter
900 keV FWMH
  • 900 keV resolution dominated by
  • Energy loss in muon stopping target (640 keV
    FWHM)
  • Tracker intrinsic resolution (350
    keV FWHM)

Full GEANT Simulation Signal
14
MECO Sensitivity Background
  • Expected Sensitivity
  • Expected Background

15
Current Status
  • Scientific approval
  • Approved by BNL and by the NSF through level of
    the Director
  • Approved (with KOPIO) by the NSB as an MREFC
    Project (RSVP)
  • Endorsed by the recent HEPAP Subpanel on
    long-range planning
  • Technical and management reviews
  • Positively reviewed by many NSF and Laboratory
    appointed panels
  • Magnet system design positively reviewed by
    external expert committees appointed by MECO
    leadership
  • Funding
  • Currently operating on 2.1M RD funds from the
    NSF
  • Project start awaits Congressional action RSVP
    (MECO KOPIO) is not in the FY03 budget
    efforts in Congress to improve NSF MREFC funding
  • Construction schedule
  • Construction schedule driven by superconducting
    solenoids estimate from the Conceptual Design
    Study is 41 months from signing of contract until
    magnets are installed and operational

16
Outlook
  • The physics potential for MECO is extremely
    robust. Numerous extensions of the Standard
    Model predict an observable m?e signal if we are
    able to achieve the predicted four order of
    magnitude increase in sensitivity
  • We expect to make this leap forward using several
    advances in the muon conversion state of the art
  • 1000fold increase in rate of the m- stops
  • Muon beam line that minimizes contamination while
    maximizing yield
  • Improved detector acceptance, high rate
    capability, and good resolution
  • We expect to move into the detailed design and
    construction phase very soon, meaning now is the
    perfect time for people to get involved!

More information visit http//meco.ps.uci.edu
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