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Search for sterile neutrinos in MINOS

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Title: Search for sterile neutrinos in MINOS


1
Search for sterile neutrinos in MINOS
  • Christopher Backhouse
  • University of Oxford
  • Fermilab Users Meeting
  • 4 June 2009

2
Search for sterile neutrinos in MINOS
  • Overview of the MINOS experiment
  • Sterile neutrinos
  • Event Selection
  • Prediction of FD spectrum from ND
  • Results from 3.181020 protons-on-target
  • 3-flavour expectation
  • 4-flavour model
  • ? decay model

Christopher Backhouse
2
3
Main Injector Neutrino Oscillation Search
  • 93 ?? beam from Fermilab Main Injector
  • Two detectors
  • Near Detector at Fermilab
  • Far Detector in Soudan mine 735km away
  • Measure flux at ND, compare to FD measurement

Near Detector
Far Detector
  • Functionally identical magnetized
    steel-scintillator tracking calorimeters
  • Fiducial masses
  • ND 27t
  • FD 3.8kt

See talk by G. Pawloski for more details
Christopher Backhouse
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4
3-Flavour Theory
Christopher Backhouse
4
5
Sterile Neutrinos
  • Z0 width (LEP) ? 3 light active neutrinos
  • Additional sterile ??
  • LSND suggests new large ?m2
  • Bugey, Karmen and MiniBooNE dont support this
    interpretation
  • Additional massive ? still interesting
  • Astrophysics dark matter, supernovae
  • Seesaw mechanism
  • Sterile neutrinos ? new physics!

Christopher Backhouse
5
6
Looking for Sterile Neutrinos in MINOS
  • NC interactions same for all flavours
  • Oscillations among active flavours dont affect
    NC spectrum
  • Sterile neutrinos wouldnt interact weakly at all
  • Sterile signal
  • Depletion of FD NC spectrum
  • Energy-dependent

Christopher Backhouse
6
7
Event Topologies
?µ CC Event
NC Event
  • Charged lepton track
  • Hadronic shower

June 4, 2009
Christopher Backhouse
7
Christopher Backhouse
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8
Pre-Selection Cuts
  • Beam and detector quality
  • Veto cosmics using timing and steepness
  • Event vertex not close to detector edge
  • Ensures containment of hadronic shower

Near Detector
Far Detector
Christopher Backhouse
8
9
ND Pre-Selection Cuts
  • High event rate in ND can cause poor event
    reconstruction
  • Split events
  • Incorrect vertex
  • Apply a series of cuts
  • Time and spatial separation
  • Total number of hit strips
  • Event steepness
  • Activity in edge region
  • Reduce poorly reconstructed background lt1GeV from
    34 to 8

9
Christopher Backhouse
10
ND NC Event Selection
  • Discard events gt60 planes
  • Discard events with a track gt5 planes longer than
    the shower
  • Same selection applied at FD
  • Variable distributions similar

Christopher Backhouse
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11
Neutral Current Selection
  • NC events selected with 90 efficiency and 60
    purity

Christopher Backhouse
11
12
Near Detector NC Spectrum
  • Good agreement between data and MC
  • Discrepancies smaller than systematic
    uncertainties

Christopher Backhouse
12
13
Far/Near Ratio Method
  • The F/N ratio method uses the ND data without
    relying on a specific parameterization
  • Correct each energy bin in the FD MC using the ND
    data/MC differences as a scale factor
  • Simple, robust to systematic errors
  • FD data spectrum blinded so prediction unbiased

Christopher Backhouse
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14
3-Flavour Analysis
  • Compare NC energy spectrum with expectation from
    standard 3-flavour oscillations
  • Pick the oscillation parameter values
  • Normal mass hierarchy
  • sin22?23 1
    (Super Kamiokande)
  • ?m232 2.43x10-3 eV2
    (MINOS CC result)
  • ?m221 7.59x10-5 eV2, ?12 35
    (KamLANDSNO)
  • ?13 0 or 12 from CHOOZ limit
  • ?3p/2 (maximum ne appearance)
  • Because CC ne are almost all selected as NC

Christopher Backhouse
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15
3-Flavour FD Energy Spectrum
Christopher Backhouse
15
16
R statistic
  • No ? disappearance ? R1

Christopher Backhouse
16
17
4-Flavour Analysis
  • Assume an additional sterile ? and an additional
    ?m2
  • Extend mixing matrix with extra angles and phases
  • Consider two mass scales
  • ?m241 gtgt ?m231
  • ?m241 ltlt ?m231
  • Simplify oscillation formulae

17
Christopher Backhouse
18
4-Flavour Analysis
  • Start with general matrix
  • UR34(?34) R24(?24,?2) R14(?14) R23(?23)
    R13(?13,?1)R12(?12)
  • 11 parameters
  • ?34, ?24, ?14, ?23, ?13, ?12
  • ?m223, ?m241, ?m221
  • ?1, ?2
  • Need to simplify

19
4-Flavour Analysis
  • ?34, ?24, ?23, ?13, ?14, ?12
  • ?m223, ?m241, ?m221
  • ?1, ?2
  • ?m221 ? 0
  • ?14 ? 0
  • ?2 ? 0
  • Pick mass scale
  • ? UR34(?34) R24(?24) R23(?23) R13(?13,?1)
  • ?13 and ?1 as before

20
4-Flavour Analysis
  • ?34 lt 38 (56 ?e) (90 C.L.) (Both models)
  • ?24 lt 10 (10.6 ?e) (90 C.L.) (?41 gtgt ?31)

21
Sterile fraction
  • Simple way to interpret result
  • What fraction of ?µ that disappear go to steriles?

fs lt 0.51 (0.55 ?e) (90 C.L.)
Christopher Backhouse
21
22
Future Sensitivity
Christopher Backhouse
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23
Neutrino Decay CC spectrum
  • Deficit in FD CC energy spectrum versus
    expectation
  • Decay disfavoured at 3.7s

Christopher Backhouse
23
24
Neutrino Decay NC spectrum
  • Decay would also deplete NC spectrum, improves
    limit
  • Mixed model
  • ? oscillations
  • One mass state decays

Pure decay disfavoured at 5.4s
Christopher Backhouse
24
25
Summary
  • Analysis of neutral current neutrino interactions
    from 3.18?1020 POT NuMI beam exposure
  • Consistent with no neutrino decay and no sterile
    neutrino admixture (R1.040.080.07-0.10(?e))
  • fs lt 51 (90 C.L. no ?e appearance)
  • Disfavour pure decay by 5.4s as alternative to
    oscillations
  • Mass-corrected ? lifetime gt 2.1x10-12 s/eV (90
    C.L.)
  • Statistically limited. More protons-on-target
    will continue to improve result

Christopher Backhouse
25
26
Acknowledgements
  • On behalf of the MINOS Collaboration, I would
    like to express our gratitude to the many
    Fermilab groups who provided technical expertise
    and support in the design, construction,
    installation and operation of the experiment
  • We also gratefully acknowledge financial support
    from DOE, STFC(UK), NSF and thank the University
    of Minnesota and the Minnesota DNR for hosting us

Christopher Backhouse
26
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27
------- Blank -------
14 October 2009
Christopher Backhouse
27
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Backup Slides
29
The MINOS Collaboration
140 scientists 28 institutions
Argonne Athens Benedictine Brookhaven
Caltech Cambridge Campinas Fermilab Harvard
Holy Cross IIT Indiana Minnesota-Twin
Cities Minnesota-Duluth Otterbein Oxford
Pittsburgh Rutherford Sao Paulo South
Carolina Stanford Sussex Texas
AM Texas-Austin Tufts UCL Warsaw William
Mary
Christopher Backhouse
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MINOS Physics Goals
  • Measure Dm2atm and sin22qatm via nm
    disappearance
  • Search for ne appearance (?13)
  • Compare n, n oscillations
  • Atmospheric ? and cosmic rays
  • Cross sections using ND
  • Search for or constrain exotic physics such as
    sterile n

Christopher Backhouse
30
31
NuMI Beam
  • 120GeV protons strike target
  • Pions and Kaons focussed
  • Decay into neutrinos (93 ?µ)
  • Rock absorbs everything else

Christopher Backhouse
31
32
Near Detector
  • Magnetized steel-scintillator tracking
    calorimeter
  • Alternate planes of steel and plastic
    scintillator strips
  • Read out by PMTs
  • 27t fiducial mass

Christopher Backhouse
32
33
Far Detector
  • Functionally equivalent to Near Detector
  • 3.8kt fiducial mass
  • 705m underground

Christopher Backhouse
33
34
Weak Interactions
  • Neutral current
  • No track
  • Unobserved energy
  • Hadronic shower
  • Charged current
  • Charged lepton track
  • Hadronic shower

June 4, 2009
Christopher Backhouse
34
Christopher Backhouse
34
35
Muon Neutrino Disappearance
  • Deficit in FD CC energy spectrum versus
    expectation

Christopher Backhouse
35
36
Muon Neutrino Disappearance
  • Worlds best measurement of ?m2

Christopher Backhouse
36
37
ND Event Pre-Selection Cuts
  • Beam quality and detector quality cuts
  • Event vertex reconstructed within the fiducial
    volume of the detector
  • Transverse vertex position gt 50 cm away from the
    edge of a partial plane or its outline on a full
    plane
  • 30 planes lt z lt 80 planes

Christopher Backhouse
37
38
FD Event Pre-Selection Cuts
  • Beam quality and detector quality cuts
  • Event vertex reconstructed within the fiducial
    volume of the detector
  • Transverse vertex position gt50 cm from the edge
    of the detector and gt45 cm from the center of the
    detector (avoid uninstrumented coil hole region)
  • z position gt25 cm from the front and gt1m from the
    back of each super-module

14 October 2009
Christopher Backhouse
38
39
FD NC Event Selection
  • Discard events gt60 planes
  • Discard events with a track gt5 planes longer than
    the shower

Christopher Backhouse
39
40
Systematic Errors
  • Normalization ?4
  • Livetime, Near/Far reconstruction efficiency,
    fiducial mass
  • Relative Hadronic Calibration ?3
  • Inter-detector calibration uncertainty
  • Absolute Hadronic Calibration ?11
  • Hadronic shower energy scale(?6)
  • Modeling of intranuclear rescattering(?10)
  • CC Contamination of NC-like sample ?15
  • ND Preselection
  • Evis lt 0.5GeV ?15.2
  • Evis lt 1.0GeV ?2.9

Christopher Backhouse
40
41
Blind Analysis
  • Hide unknown fraction of FD events using unknown
    function of energy
  • Decide analysis details using Monte Carlo and ND
    data
  • Use open FD dataset for data quality checks
  • Open the box
  • Dont change any details of the analysis after
    this point
  • Ensures result unbiased

Christopher Backhouse
41
42
4-Flavor Contours
Christopher Backhouse
42
43
4-Flavor Contours Sensitivity
Christopher Backhouse
43
44
Decay Sensitivity
45
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