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ChargedParticle Multiplicities in Neutrino Interactions

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Title: ChargedParticle Multiplicities in Neutrino Interactions


1
Charged-Particle Multiplicities in Neutrino
Interactions
  • Murat GULER, Umut KOSE
  • METU-Ankara
  • (for the CHORUS Collaboration)

2
Charged-Particle Multiplicities
  • The multiplicty of charged particles is an
    important global parameter reflecting the
    dynamics of the interaction.
  • The characteristics of charged-particle
    multiplicity distributions have been studied in
    detail in high energy hadronic collisions and in
    electron-positron annhilation.
  • Also, it has been studied in neutrino and
    anti-neutrino interactions on nucleons and light
    nuclei. In particular, Bubble Chamber experiments
  • However, data on neutrino interactions in nuclear
    emulsion are relatively scare. No data on
    anti-neutrino-nucleus interactions in nuclear
    emulsion.
  • Such data are useful in tuning interaction models
    in Monte Carlo event
  • generators.

3
The n beam
West Area Neutrino Facility at CERN SPS
  • Wide Band Beam
  • 4-years of operation (1994-1997)
  • 5.06 ? 1019 POTs
  • ltEnmgt 27 GeV

4
CHORUS detector
T5C
Nucl. Instr. Meth A 401 (1997) ,7
? -
Calorimeter
h-
  • Events are classified as
  • 0m sample
  • 1m sample
  • based on electronic detector
  • information


Muon spectrometer
Air core spectrometer
and emulsion tracker
Veto plane
5
Nuclear Emulsion Target
  • 60 years of RD.
  • The sub-micron spatial resolution of nuclear
    emulsion allows both investigation of the event
    topology and the mesurement of the angular
    distribution of the charged particles.
  • 770 kg nuclear emulsion was exposed to the
    neutrino beam in CHORUS.
  • Massive automatic scanning (pioneered by Nagoya
    Univ. group of CHORUS)

6
Automatic Scanning
Tracks reconstructed by a hardware video
processor frame to frame emulsion grains
coincidence
microscope stroke
7
Event Location
  • The location of the emulsion plate containing the
    interaction vertex
  • Tracks reconstructed by the electronic detectors
    are followed upstream into the emulsion stacks
  • A track is followed upstream in the target
    emulsion stack using track segments reconstructed
    in the most upstream 100µm of each plate.
  • If the track is not found in two subsequent
    plates the first plate with no track hit is
    defined as the plate containing the vertex.

1
2
3
8
Event Location
  • 150,000 n interactions have been located events
    with at least one reconstructed muon in the
    spectometer.
  • A sample of 1200 events was randomly selected
    to measure the parameters associated with
    charged-particle tracks at the (anti-) neutrino
    vertex.
  • We use the highest-mometum muons charge in
    the event to determine whether the interaction
    was induced fom neutrino or anti-neutrino.
  • n sample 627 events
  • n sample 581 events

9
Data Sample
  • To evaluate the genuine anti-neutrino events,
    contaminations which are mainly punch through
    hadrons and miss-identified µ- events must be
    evaluated.
  • In order to reduce this background a set of
    selection criteria imroving the realibity of the
    muon reconstruction were applied.
  • After contamination cleaning the number of
    anti-neutrino events becomes to be 529
  • Finally, we further require that square of the
    invariant mass of the hadronic system,W2, of
    (anti-) neutrino events is greater than 1 GeV2/c4
  • n sample 496 events
  • n sample 369 events

10
Analysis
  • Tracks are classified accordingly grain density
    as shower, grey and black.
  • Black prong glt1.4g0
  • Grey prong 1.4g0glt10g0
  • Shower prong g10g0 where go is grain density
    of higly relativistic a singly charged particle
    which equals 30 grains in 100mm for the CHORUS
    emulsion
  • The criteria used in old nuclear emulsion
    experiments is difficult to apply in the CHORUS
    analysis since the emulsion sheets were exposed
    prependicular to the beam direction.
  • In CHORUS, once the neutrino vertex had been
    located, the event was checked and measured
    extensively with a manual controlled microscope
    system.

11
Analysis
  • The black prongs are due to heavily ionizing
    particles have short path lengths and stop within
    one emulsion plate.
  • For the grey and shower prongs, the particle
    direction is measured. These particles are mainly
    pions with a small contamination of protons.
  • Ambiguity in classifying shower and grey prongs
    can be arise either due to the difficulty
    strickly applying the ionization criteria or due
    to variations in the quality of optics of the
    microscope.

Black prongs
12
Analysis
  • To overcome these limitations, we decided to
    classify these prongs by using the
    pseodo-rapidty variable
  • This has advantage of being independent of
    scanner and of the microscope optics, allowing us
    to compare in a straight manner the multiplicty
    measurements with theoretical models

The pseodo-rapidty distributions for the track
classified as shower and grey by the scanner
shower
grey
  • All prongs with ? 1 are classified as shower
    particles

13
Efficiency Estimation
Neutrino events
  • Reconstruction and detection efficiencies were
    evaluated making a detailed simulation of
    detector response using a program based on GEANT3
  • The simulated response of electronic detectors
    was processed through reconstruction program
    as that used for experimental data
  • The reconstrcution efficiency as function of W2
    and nch is given in tables
  • The samples are normalized in such a way that
    the efficiency at first bin is taken as 1.00

Anti-neutrino events
14
Multiplicty Distributions
  • The average number track multiplicity (nchns-1)
    in neutrino interactions.
  • ltnch(n A)gt 3.40.1
  • ltnh(n A)gt 4.70.2
  • In anti-neutrino inte-ractions
  • ltnch(n A)gt 2.80.1
  • ltnh(n A)gt 3.50.2

15
Multiplicity Distributions
  • The mean multiplicities are in good agreement
    with a linear depen- dence on lnW2

16
(QERES)-like events
  • For the first time a sample of (anti-) neutrino
    is large enough to study (QERES)-like topologies
  • Event is defined as being (QERES)-like
  • if the number of shower prongs is zero or one and
    the number of grey prongs zero or one for n-A
    interactions regardless of the number of black
    prongs.
  • In order to obtain (QERES)-like enriched sample
    in n-A interactions
  • the sum of shower and grey prongs is required to
    be zero or one regardless of the number of black
    tracks.
  • In order supress the background from DIS
    interactions we further require W2lt10 GeV2/c4 for
    both sample. After this selection the number
    (QERES)-like events is

17
(QERES)-like events
  • The number of background events that mimic
    (QERES)-like topology is obtained from the MC
    simulation to be
  • 83.4 (73.5)for n-A(n-A) interactions
  • The ratio of reconstruction and location
    efficiency of (QERES)-like events to that of all
    CC events is found to be
  • 1.22(1.13) for n-A(n-A) interactions
  • After applying efficiency and background
    corrections, the fraction of (QERES)-like events
    are found to be
  • (13.40.10.2) for n-A interactions
  • (26.31.43.9) for n-A interactions
  • The sub-sample of events with neither black or
    grey prongs is important for the understanding of
    nuclear mechanism involving hadrons in the
    nucleus. The fraction of this type of topology is
    measured as
  • (1.20.40.2) for n and (9.51.01.4) for n

18
Dispersion of track multiplicity
  • The linear dependence of Dch on nch would imply
    that multiplicity is independent of W2

19
KNO Scaling
  • One can observe that our data are not compatible
    with A0. Non-zero A is due to heavy nuclear
    targets in nuclear emulsion. In that case one
    introduce
  • Where a is the extrapolation point where the
    fitted dispersion line crosses average
    multiplicity line

The superimposed curve represent a fit to pp
data. The data approximately agree with KNO
scaling. The data points at different W2 lie
approximately on a single curve.
20
Conclusion
  • The multiplicity feature of (anti-) neutrino
    interactions in emulsion have been investigated.
  • The average number of shower and heavy prongs in
    (anti-) neutrino events are measured as
  • The dependence of the average multiplicity ltnchgt
    on lnW2 for n-A and n-A interactions is
    compatible with being linear with similar slope.
  • The dispersion Dch of the multiplicity
    distribution shows a linear dependence on the
    mean multiplicity ltnchgt.
  • The emulsion data is consistent with the KNO
    scaling as a function of
  • an appropriate multiplicity variable z.

ltnch(n A)gt 3.40.1 ltn h(n A)gt 4.70.2
ltnch( n A)gt 2.80.1 ltnh( n A)gt 3.50.2
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