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Neutrino DIS measurements in CHORUS

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Neutrino DIS measurements. in CHORUS. DIS2004. Strbske Pleso 14-4-2004. Alfredo G. Cocco ... CHORUS detector p/p = 0.035 p (GeV/c) 0.22 p/p = 10 15% (p 70 GeV/c) ... – PowerPoint PPT presentation

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Title: Neutrino DIS measurements in CHORUS


1
Neutrino DIS measurementsin CHORUS
DIS2004
Strbske Pleso 14-4-2004
Alfredo G. Cocco INFN Napoli
2
CHORUS detector
Air-core magnet
Active target
?p/p 0.035 p (GeV/c) ? 0.22
-nuclear emulsion target (770kg) -scintillating
fiber tracker
?
?p/p 10 15 (p lt 70 GeV/c)
muon spectrometer
27 GeV
Calorimeter
WB Neutrino beam
?E/E 32 /? E (hadrons) 14 /? E
(electrons) ?? h 60 mrad _at_ 10 GeV
nm nm ne ne 1.00
0.06 0.017 0.007
3
Neutrino targets
  • Emulsion (1 ?m precision ? decay topology)
    ET
  • 770 kg, 4 X0
  • 2x106 CC ? interactions, 1994-1997
  • Calorimeter
    CT
  • 112 ton, lead-scint.fiber, 5.2 ?
  • 1.5x107 CC ? interactions, 1994-1998
  • Special 4 targets
    4T
  • 100x4 kg, marble, plastic, Fe, Pb
  • 106 CC ? interactions, 1998

4
Non-oscillation physics in CHORUS
  • Charm
  • D0, ?c, QE charm production
  • cc CC/NC production
  • BR ? ?, fragmentation functions
  • anti-neutrino charm production
  • total charm production cross section
  • Structure functions
  • J/? NC production
  • Dimuons
  • Trimuons
  • Z/A dependence of CC cross-section

(ET) (CT) (CT) (CT) (CT) (4T)
5
Dimuons analysis
Dimuons
To extract ? mc ? ? ?
(fragmentation) ? B? (charm into ? decay
fraction)
6
Data selection
7
Data sample
Dimuons
? Data taken from 1995 to 1998 with a dedicated
trigger setup ?
6.6?106 triggers ? At least 2 reconstructed
muons ? 5?105
events
8
Selection criteria
Dimuons
? 5 ? Esh ? 200 GeV ? ngap1 ? 5
ngap2 ? 5 ? E?1 ? 5 GeV E?2 ? 5 GeV ? d12 ?
15 cm ? q2 ? 4 GeV2 ? ?Vy,z ? ? 120 cm
295 cm ? Vx ? 394 cm ? 20 ? E? ? 200 GeV
xbj ? 1.0 ybj ? 1.0
9
Final sample
Dimuons
2? selected N?? 2801 N?
13132 N? 1224 N 70 The leading
muon is that one with the highest PT (96
efficiency)
10
MCDIS generator
Dimuons
11
MCDIS
Dimuons
? A new complete event generator for neutrino CC
DIS has been implemented ? Based on Aivazis
helicity formalism ? Leading Order cross
section ? Strange quark parametrization (?,?) ?
Implements JETSET for hadronization ? Fermi
motion, radiative correction (Bardin) ? Full
control on each step via runcards
12
MCDISLeading Order cross section
Dimuons
Aivazis et al. (1994)
F helicity structure functions (mt mc VCKM
pdf(?)) ? Lorentz boost between lepton and
hardon configurations
13
MCDISLeading Order cross section
Dimuons
For charm neutrino production and neglecting
initial quark mass
Where ? in the limit of M2/Q2? 0 is the slow
rescaling variable
14
MCDISFragmentation function
Dimuons
Peterson parametrization
? 0.05
ZP(hc)/Pmax(hc)
z
15
MCDISTransverse momentum
Dimuons
? 1.1
N
PT
hc
W
PT2
16
MCDISParton Distribution Functions
Dimuons
? Used GRV94LO and CTEQ3L ? Strangeness
parametrization
? 1 for a flavour SU(3) symmetric sea
17
Data MC comparison
Dimuons
E? (GeV)
Esh (GeV)
data
MC
E?1 (GeV)
E?2 (GeV)
P?2 (GeV/c)
P?1 (GeV/c)
18
Data MC comparison
Dimuons
data
MC
y
x
z
Q2 (GeV2)
Vz(cm)
Vy(cm)
19
Data MC comparison
Dimuons
data
MC
d12(cm)
Vx(cm)
cos ?2
cos ?1
?12
Invariant mass (GeV)
20
Evaluation of Ncharm
21
Background
Dimuons
Background is due to ? and K decay into ? in CC
interactions This can be evaluated using same
sign dimuons in data and the ratio between
opposite and same sign events in CC MonteCarlo
Selection efficiencies and neutrino-antineutrino
cross contamination also to be taken into account
22
Background
Dimuons
MonteCarlo ? High statistics (106) fully
simulated CC interaction sample to
evaluate
23
Background
Dimuons
In order to subtract background using this
procedure it is crucial to verify that MC
reproduces the distributions of the same sign
dimuon events in the data
24
Same sign Data-MC comparison
Dimuons
data
MC
Esh (GeV)
E? (GeV)
E?2 (GeV)
E?1 (GeV)
P?2 (GeV/c)
P?1 (GeV/c)
25
induced opposite sign dimuon events
Dimuons
neutrino
antineutrino CDHS
9922 2123 CHORUS
10718 ? 288 420 ?
63 NOMAD 2714 ? 227
115 ? 40 CHARM II 3100
700 CCFR
5030 1060 NUTEV
5102 1458
26
4 parameters Maximum Likelihood fit
Dimuons
? Event by event (unbinned) likelihood function
in order to extract mc ? ? B? ? Probability
density given by MonteCarlo as a function of
the unknown parameters
27
ML fit result
Dimuons
? Correlation coefficients
? Systematic uncertainties
28
Dimuon analysis result(preliminary)
Dimuons
? mc 1.46 ? 0.15 (stat) ? 0.10 (syst) ?
? 0.56 ? 0.05 (stat) ? 0.045 (syst) ? ?
0.040 ? 0.003 (stat) ? 0.015 (syst) ? B?
0.098 ? 0.005(stat) ? 0.014 (syst)
29
Dimuon Analysis Summary
Dimuons
? Largest sample of neutrino induced dimuons to
date ? Results from LO analysis in agreement
with other experiments ? Slow Rescaling
model confirmed
30
Trimuon events in ?m CC interactions
  • CDHS and HPWF (1978) 100 m- m- m events
  • - origin
    largely unknown
  • CHORUS
  • 6x106 2m calorimeter triggers
  • observed 42 m- m- m, 3 m- m m (Pm gt 5
    GeV/c)
  • Detailed Monte-Carlo (LEPTO/JETSET/GEANT)
  • 4x106 events with full detector simulation
  • present knowledge of production rates and
  • m-decays of h, r,
    w, h, f
  • data-MC validation using 2m events (known
    origin)
  • data-MC comparison for 3m event sample

31
Trimuons
  • lt 90o
  • no int. bremsstrahlung

32
Trimuons
Conclusions MC predictions on 3? rate are in
agreement with measurements
33
Z/A dependence of ?m CC cross-section
Eur. Phys. J. C30 (2003) 159-167
  • for the first time 4 targets in the same
    experiment
  • were exposed
    simultaneously
  • positions rotated to avoid acceptance
    differences
  • ?m CC interactions in calorimeter used to
    monitor neutrino
  • flux and for relative
    normalisation of events
  • empty target period recorded for background
    subtraction
  • only muons used in event reconstruction
  • events are assigned to particular target by
  • extrapolating muon trajectory to the target
    plane

34
Relative total cross sections
Z/A
?(?n)/?(?p) 1.71
Predictions are based on GRV98LO PDF and
modifications according
to
A.Bodek-U.K.Yang model Predictions equalized to
measurements at marble point
35
Z/A
Comparison with previous experiments
Conclusions the result is in agreement with
previous experiments and with
predictions obtained by
parton model calculations
36
Many analyses are still in progress NEW
RESULTS WILL BE AVAILABLE WITHIN 2004
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