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Colour Reconnection in WW events

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WW qqQQ events collected at LEP2. Colour Reconnection effect at LEP2 ... W decay vert. ~ 0.1 fm distance. hadronisation scale ~ 1 fm. large space-time overlap ... – PowerPoint PPT presentation

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Title: Colour Reconnection in WW events


1
Colour Reconnection in WW events
Jorgen DHondt University of Brussels - DELPHI
Collaboration
  • WW?qqQQ events collected at LEP2
  • Colour Reconnection effect at LEP2
  • Model dependent measurement(s)
  • Preliminary conclusions

XXXII International Symposium on Multiparticle
Dynamics
1/12
2
Colour Reconnection
Known example hadronic decay of B
mesons B ? J/Y X
BR.exp 1 BR.fullCR 3-5 BR.noCR 0.3-0.5
G.Gustafson, U.Petterson and P.Zerwas,
Phys.Lett. B209 (1988) 90
4 jet topology
e
e-
DELPHI detector at LEP2
Main interest
  • Probe the interaction of two fragmenting strings
  • Causes largest systematic error on W-mass

2/12
3
Colour Reconnection in WW
  • W decay vert. 0.1 fm distance
  • hadronisation scale 1 fm
  • ? large space-time overlap
  • suppressed in parton shower
  • due to group structure of QCD at least 2 gluons
    must be emitted
  • W width restrict the energy range of primary
    gluons from q1Q4 and q2Q3
  • (as2/MW) GW/Nc2
  • CR effect could occur in the confined region ???

asltlt1
as?1
T.Sjöstrand and V.A.Khoze, Z.Phys. C62 (1994)
Models to emulate the CR effect
3/12
4
Simulating the CR effect
CR implemented in existing fragmentation models
  • PYTHIA string reconfiguration if they overlap
    or cross in space-time
  • SK1 (lateral flux tube) via event string
    overlap O pCR 1-exp(-?O)
  • SK2 (vortex line with core) reconnection if
    cores cross
  • SK2 SK2 only if string length is reduced
  • ARIADNE rearrangement of colour dipoles to
    reduce the string length (mass)
  • AR2 only after soft gluon radiation (Eg lt GW)
  • AR3 allowed everywhere (also in pertubative
    phase)
  • HERWIG rearrangement of colour dipoles changing
    the size of the clusters

SK1 mW shift
  • Latest preliminary predictions for the W-mass
  • PYTHIA (SK1) 50 MeV/c2
  • ARIADNE (AR2) 70 MeV /c2
  • HERWIG 40 MeV/c2
  • Statistical uncertainty (LEP2) 30 MeV /c2

K 0.66
For each model one can study the effect on the
structure of the WW events with Monte Carlo
simulation and compare it with data.
PCR
4/12
5
Most sensitive observables
? design an observable sensitive to for example k
(SK1)
New!
Particle flow
W-mass measurements
CR is an important systematic uncertainty on mW
measured in WW ? qqqq events, but we designed
another mW estimator which does not have this
feature...
Design an observable to measure a
possible enhancement of particles in the
inter-W regions
simply count particles (background sensitive)
jet kinematics of the event (background
insensitive)
sensitivity 2.7 s (for full SK1)
sensitivity 4.3 s (for full SK1)
Eff. 12, Pur. 87
Eff. 90, Pur. 71
The correlation between both observables was
found to be negligibly small
...all results are preliminary
5/12
6
Achievements of LEP2
WW ? 4q selected (mW observable)
WW event up to 208.8 GeV
98
99
00
97
96
indirect
design limit
Up to 5000 WW?qqQQ events expected by DELPHI
background
sWW ? 18 pb
W-mass 6000 (used data 98-00)
background
Particle flow 720 (used data 97-00)
6/12
7
W-mass observables
Influence on W mass estimator (MeV/c2) for
different values of k (SK1)
DELPHI preliminary
mW is assumed to be unknown but it must be
invariant for different estimators mW(std)-mW(co
ne) from MC as function of k
MC prediction
Correlation between W mass estimators 83 ?
uncertainty on the difference is small
7/12
8
Data _at_189-209
?2
MC prediction SK1
2 sigma
1 sigma
centr.
k
MeV/c2
first time this is done with LEP data !!
Monte Carlo prediction if there is Colour
Reconnection
different behaviour
8/12
9
Particle flow observable
Project all charged particles Pi in the plane (
jet 1, jet 2)
Inside W and Between Ws
D
Rescale the angles to have an equal amount of
phase-space between the jets FJ,i ? FJ,i .
(1/FJK)
C
A
B
(
)
data at 189 GeV
( AC )
( AC )
1
d
Z ? qq(g)
dF
( BD )
Nev
( BD )
WW? qqln
no CR
A
B
C
D
SK1 100
SK1 100
0.2
0.8
9/12
10
Preliminary results
  • In the systematic error, were considered
  • Bose-Einstein effects (2)
  • Fragmentation modelling (1)
  • Background subtraction/modelling (0.5)
  • Generators/Tunings (0.3)

ltR189gt 0.900 ? 0.031 ? 0.021
Data _at_183-209
( extrapolated to 189 GeV )
R
Monte Carlo prediction
10/12
11
Combination SK1
no correlation assumed between the
two measurements (good approximation)
?2
68 CL for k 0.3 , 3.3 central value 1.3
68 CL for PCR 14 , 75 central value 44
11/12
12
Conclusion
  • Colour reconnection models are investigated in
    WW?qqQQ events
  • Two uncorrelated observables are designed
  • Integrating the particle flow between jets ( R )
  • Using the kinematics of the jets ( DmWstd,cone
    )
  • Preliminary results prefer a small amount of
    Colour Reconnection
  • (also the LEP combined measurement, cfr. talk
    of Nigel Watson)
  • The observables are not sensitive to the ARIADNE
    model !?

Therefore one cannot decrease the systematic
uncertainty on mW
  • Preliminary shift on the W-mass
  • PYTHIA (SK1) 50 MeV/c2
  • ARIADNE (AR2) 70 MeV/c2
  • HERWIG 40 MeV/c2
  • Statistical uncertainty (LEP2) 30 MeV/c2

More work needed on ARIADNE !!
12/12
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