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PowerPoint - MiniBooNE - Fermilab by dffhrtcv3


									(Status of ) The search for nm to ne
    oscillations at MiniBooNE
   Andrew Bazarko – Princeton University
               9 October 2003
    WIN03 – Weak Interactions and Neutrinos
           Lake Geneva, Wisconsin
MiniBooNE status snapshot

  MiniBooNE has been running for 1 year at Fermilab
         acquired 15% of goal 1021 protons on target
  At the moment (Sept – mid Nov) accelerator is shutdown
      important accelerator improvements are underway
                                      MiniBooNE’s first event:
                                      beam-induced muon
                                      (Labor Day weekend 2002)

 Overview of the experiment
     (preview of tomorrow’s tour)
 First neutrino events and analysis

                           nm beam from m+ decay at rest
LSND:                                 energy 20-53 MeV
                                           baseline 30 m
Evidence for                              L/E ~ 1 m/MeV

                                Dm2~0.2-10 eV2
    87.9+22.4+6.0 events
                               (Bugey is ne disappearance)
                   Too many     ’s?
3 light neutrino flavors

Solar (+KamLAND) neutrinos:
• mostly

Atmospheric (+K2K) neutrinos:
• mostly

      Where does LSND’s Dm ~0.2-10 eV

              fit in this picture??
  n Oscillation Scenarios:
With current results from solar, atmospheric, and LSND
n-oscillation searches (3 Dm2s), we have an interesting situation:

Only 3 active n:            3 active+1 sterile n:               CPT violation:

                                                       n mass
                             n mass
  n mass

                 OR...                         OR...                          OR...

 - not a good fit to data             - possible(?)                  - possible(?)

       Need to definitively check the LSND result.
Goal: test LSND with                             ?
5-s sensitivity over
whole allowed range
                                               8 Gev Booster

• higher statistics        target
• different signature
• different backgrounds
• different systematics
                               Main Injector

 BooNE: Fermilab Booster Neutrino Experiment
                           Y. Liu, I. Stancu Alabama
                           S. Koutsoliotas Bucknell
                           E. Hawker, R.A. Johnson, J.L. Raaf Cincinnati
First phase: “MiniBooNE”   T. Hart, E.D. Zimmerman Colorado
                           Aguilar-Arevalo, L.Bugel, J.M. Conrad,
                             J. Formaggio, J. Link, J. Monroe, D. Schmitz,
                             M.H. Shaevitz, M. Sorel, G.P. Zeller Columbia
• Single detector, nm ne   D. Smith Embry Riddle
                           L.Bartoszek, C. Bhat, S J. Brice, B.C. Brown,
      appearance             D.A. Finley, B.T. Fleming, R. Ford, F.G.Garcia,
                             P. Kasper, T. Kobilarcik, I. Kourbanis,
                             A. Malensek, W. Marsh, P. Martin, F. Mills,
                             C. Moore, P. J. Nienaber, E. Prebys,
• L/E=500 m/500 MeV =        A.D. Russell, P. Spentzouris, R. Stefanski,
                             T. Williams Fermilab
…..30 m/30 MeV (LSND)      D. C. Cox, A. Green, H.-O. Meyer, R. Tayloe
                           G.T. Garvey, C. Green, W.C. Louis, G.McGregor,
                             S.McKenney, G.B. Mills, V. Sandberg,
                             B. Sapp, R. Schirato, R. Van de Water,
                             D.H. White Los Alamos
                           R. Imlay, W. Metcalf, M. Sung, M.O. Wascko
                                  Louisiana State
                           J. Cao, Y. Liu, B.P. Roe Michigan
                           A.O. Bazarko, P.D. Meyers, R.B. Patterson,
                             F.C. Shoemaker, H.A.Tanaka Princeton

               magnetic horn   decay pipe abs 450 m dirt
                                             or            detector
                and target     25 or 50 m       be

8-GeV protons on Be target à
     p+, K+,…, focused by horn
           decay in 50-m pipe, mostly to nm
                   all but n absorbed in steel and dirt
                        n’s interact in 40-ft tank of mineral oil
                             charged particles produce light
                                    detected by phototube array

      Look for electrons produced by mostly-nm beam
     The Booster

 8 GeV proton accelerator
 supplies beam to all Fermilab
  It must now run at record intensity

MiniBooNE runs simultaneously
 with the collider program; goals:

                                                        MiniBooNE: negligible
                MiniBooNE               20
                                  5x10 p.o.t per year   impact on collider;
                                                        improvements to
                                 (1x1021 total)         Booster good
 Booster                                                for NuMI

                                     antiproton source
               Main Injector         TeVatron
                                     120 GeV fixed target
   Booster performance                   July 2002 - Sept 2003

We are pushing the
Booster hard
                                       MiniBooNE                 goal
Must limit radiation damage                                      intensity
and activation of Booster              startup
  increase protons
  but decrease beam loss

~steady improvements
   careful tuning
   understanding optics

need factor of 2-3 to reach
goal 1021 p.o.t. by early 2005   red: Booster output (protons/minute)
further improvements coming      blue: energy loss per proton
    collimator project (now)                          (W-min/proton)
    large-aperture RF cavities
    Target and magnetic horn
Increases neutrino intensity by 7x


170 kA in 140 msec pulses @ 5 Hz
                                                the horn
   Currently positive particles are being
   focused, selecting neutrinos
   the horn current can be reversed to select

 Prior to run, tested to
  11M pulses
 has performed flawlessly:
  40M pulses in situ
                                                the target
World’s longest-lived horn
Intrinsic ne in the beam
    p+àm+ nm                                Monte Carlo
            e + n en m

    K+àp0 e+ne

    KLàp- e+ne

important bkgd to osc search

Tackle this background with
 half-million nm interactions in detector
 HARP experiment (CERN)
 E910 (Brookhaven)
 “Little Muon Counter”
 25 m / 50 m decay length option
Little Muon Counter (LMC)
  } off-axis (7o) muon spectrometer
  } K decays produce higher-energy
    wide-angle muons than p decays
  } clean separation of muon parentage
  } scintillating fiber tracker      temporary LMC detector (scintillator paddles)
                                         commission data acquisition
                                         53 MHz beam RF structure seen
                    Monte Carlo

          m from p decay

                   m from K decay

  muon momentum at 7o (GeV)
The MiniBooNE detector
MiniBooNE detector
 pure mineral oil (Cherenkov:scint ~ 3:1)

 total volume:    800 tons (6 m radius)
 fiducial volume: 445 tons (5m radius)

 Phototube support structure
 provides opaque barrier between
 veto and main volumes

1280 20-cm PMTs in detector at 5.5 m radius
        10% photocathode coverage
         (330 new tubes, the rest from LSND)
240 PMTs in veto
 Pattern of hit tubes (with charge and time information)
 allows reconstruction of track location and direction
 and      separation of different event types.

 e.g. candidate events:             size = charge; red = early, blue = late

muon                      Michel electron           p0 g two photons
from nm interaction       from stopped m decay      from nm interaction
                          after nm interaction
                                            Understanding the detector

                                                      Laser flasks

                                            four Ludox-filled flasks
                                            fed by optical fiber from laser

 PMT charge and
 time response
                  397 nm laser
oil attenuation   (no scintillation!)
length            modeling other
                  sources of “late light”
                             Stopping muon calibration system

                             Scintillator tracker above the tank

Optically isolated scintillator cubes
 in tank:
   six 2-inch (5 cm) cubes
   one 3-inch cube

                        stopping muons with known path length
                        calibration sample
                           of muons up to 700 MeV
Michel electrons
 (electrons from the decay of stopped muons)
                                                  m candidate lifetime (ns)
   plentiful source from cosmics
      and beam-induced muons

  cosmic muon lifetime in oil
   measured: t = 2.15 ± 0.02 ms
   expected: t = 2.13 ms                             PRELIMINARY

            (8% m- capture)
                                               Michel electron energy (MeV)

  Energy scale and resolution                              15%
  at Michel endpoint (53 MeV)                              E resolution
                                                           at 53 MeV
               Michel electrons throughout
               detector (r<500 cm)
   Neutrino events

beam comes in spills @ up to 5 Hz
each spill lasts 1.6 msec

trigger on signal from Booster
read out for 19.2 msec; beam at [4.6, 6.2] msec

no high level analysis needed to see
neutrino events

backgrounds: cosmic muons
            decay electrons

simple cuts reduce non-beam
  backgrounds to ~10-3

160k neutrino candidates
   in 1.5 x 1020 protons on target
  The road to nm g ne appearance analysis

  Blind ne appearance analysis
      you can see all of the info on some events
      some of the info on all events
      you cannot see all of the info on all of the events

Early physics: other analyses before nm g ne appearance
  interesting in their own right
  relevant to other experiments
  necessary for nm g ne search
       vets data-MC agreement (optical properties, etc.)
        and reliability of reconstruction algorithms
       progress in understanding backgrounds
Early physics
 CC quasi-elastic             NC p0 production              NC elastic


 abundance ~40%              abundance ~7%               abundance ~15%
 simple topology             p0 g g g                    usually sub-C
 one muon-like ring           two rings                  dominated by
 proton rarely above C       E1, E2 from C intensities     scintillation

 select “sharp” events       reconstruct invariant       low Ntank (pmt hits)
 ~88% purity                  mass of two photons        high late light fraction

 kinematics:                 background to               understanding of
    E m, q m g E n , Q 2       ne appearance               scintillation
 relatively well-known s:     and                        sensitive to nucleon
  nm disappearance           limits on sterile n          strange spin component
CC nm quasi-elastic events                PRELIMINARY

 selection: topology                                    Evis
               ring sharpness
               on- vs. off-ring hits
                single m-like ring
                prompt vs. late light
 c variables combined                              PRELIMINARY
   in a Fisher discriminant

data and MC relatively normalized            cos qm
yellow band: Monte Carlo with current
uncertainties from • flux prediction
                   • sCCQE
                   • optical properties
                                                     sensitive to nm disappearance
               Neutrino energy
                    kinematic reconstruction:
                       assume nm n g m- p
                       use Em, qm to get En                              En

                             Monte Carlo
energy resolution


                               <10% for En>800 MeV
Preliminary nm disappearance sensitivity


uncertainty in flux
                       NTANK>200, NVETO<6, no decay electron
NC p0 production       perform two ring fit on all events
                       require ring energies E1, E2 > 40 MeV

                   fit mass peak to extract signal yield
                   including background shape from Monte Carlo

                                           note bkgd also peaking

   p0 production angle

 sensitive to production mechanism
 coherent is highly forward peaked

data and MC         PRELIMINARY

are relatively

MC shape
cross sections
                                     cos qp0
  p0 decay angle
                                                   cos qCM

  p0 momentum                    PRELIMINARY

CM frame          lab frame

  qCM = p/2        small g g
              a    opening                     p0 momentum
  cosqCM= 0        angle

  qCM = 0           photon                     PRELIMINARY
              a     energies
  cosqCM= 1         asymmetric
  NC elastic scattering                                               PRELIMINARY

Now select NTANK < 150
           NVETO< 6
  Background subtraction

                  PRELIMINARY                     PRELIMINARY           PRELIMINARY
 clear beam       beam with unrelated             normalized strobe           beam after
                  background                        data                      strobe
 excess                                                                       subtraction

 use random
 triggers to
 nm NC elastics

  Consider NTANK spectrum
   MC and data shapes agree
   qualitatively for NTANK>50
 Unknown component NTANK<30

data and MC relatively normalized for NTANK>50

                                       Late light selection:
                                      fit event vertex for NTANK>50
                                      calculate fraction of late hits
                                      select events with significant late light
ne appearance sensitivity
   preliminary estimates,
   backgrounds and signal

       1500 intrinsic ne

       500 m mis-ID
                               cover LSND allowed region at 5 s
       500 p0 mis-ID
                               updated estimates coming
       1000 LSND-based nm®ne   currently expect results in 2005
  steadily taking data
      currently at 15% of 1021 p.o.t

 beam is working well, but still need higher intensity
   improvements underway (shutdown) will be key

first sample of neutrino physics
    detector and reconstruction algorithms are working well

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