APS 5-MAY-2009 G. Gutierrez, Fermilab Edward A. Bouchet Award Talk “ The top quark mass, a brief...
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Transcript of APS 5-MAY-2009 G. Gutierrez, Fermilab Edward A. Bouchet Award Talk “ The top quark mass, a brief...
APS 5-MAY-2009 G. Gutierrez, Fermilab
Edward A. Bouchet Award Talk“The top quark mass, a brief history and present status”
Gaston GutierrezFermilab
This talk is dedicated to the memory of Clicerio
Avilez.
APS 5-MAY-2009 G. Gutierrez, Fermilab
• Concepts of maximum likelihood.
• A brief history of the top quark mass measured by calculating a probability density distribution for every event.
• The current status of the top mass measurements.
• Other application of M.E.M.
• Conclusion.
Outline of the talk
APS 5-MAY-2009 G. Gutierrez, Fermilab
If for an event characterized by a set of measurements one can calculate the probability density function:
then given N events the optimal estimation of the set of parameters is obtained by maximizing
General Maximum Likelihood technique
)|( xP
x
N
iixPL
1
)|()(
1)|(with dxxP
APS 5-MAY-2009 G. Gutierrez, Fermilab
In general we have to sun over all states that can lead to the set of measurements
the sum is over probabilities (amplitudes) if the states do not (do) interfere. For a perfect detector we have
with
Probability calculation
states
ss xPcxP )|()|(
x
)(
)|()|(
xd
dxxP ss
space phase factorflux
|| 2
M
d
APS 5-MAY-2009 G. Gutierrez, Fermilab
Probability calculation for real detectors
)|,()|()(
)|,()|()()|(
xyWydxAdx
xyWydxAxP
s
ss
Detector acceptance(e.g. cuts, trigger, …)
partonicintegral partonic
variables
mapping between partonicand measured variables
measuredvariables
parameters
Integral over measuredVariable (normalization)
APS 5-MAY-2009 G. Gutierrez, Fermilab
Why apply the previous method to the top mass?
• The top mass is an important SM parameter.
• Together with the W mass it constrains the Higgs mass
• Top is a very isolated state, which makes for a cleaner calculation of the pdf.
• No matter which method we use we all need to model the relation between the top mass and the detector measurements.
APS 5-MAY-2009 G. Gutierrez, Fermilab
Kunitaka Kondo
J. Phys. Soc. Japan, 57, 4126 (1988)
J. Phys. Soc. Japan, 60, 836 (1991)
J. Phys. Soc. Japan, 62, 1177 (1993)
APS 5-MAY-2009 G. Gutierrez, Fermilab
R.H. Dalitz and Gary R. Goldstein
Phys. Rev. D45, 1541 (1992)
Proc. Roy. Soc. Lond. A455, 2803 (1999)
J. Mod. Phys. A9, 635 (1994)
Phys. Lett. B287, 225 (1992)
Phys. Rev. D47, 967 (1993) (with K. Sliwa)
APS 5-MAY-2009 G. Gutierrez, Fermilab
D0 experiment
Nature 429,638 (2004)
First complete measurement, including: 1) all detector effects (e.g. reconstruction efficiencies, cuts, trigger, …), 2) correct normalization, 3) background probabilities, 4) MC tests of linearity, 5) pull calculations and 6) estimation of systematic effects.
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run I: Top probability for data events
Left plot show -ln(Ptt) as a function of
Mt for 10-9<Pbkg <10-8 (red arrows in
lower figure).
x=-ln(PB)
x=18.5
x=20.4
x=20.0x=19.4
x=19.2
x=20.5
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run I: Top probability for data events
Left plots show -ln(Ptt) as a function of
Mt for 9.7x10-13 <Pbkg < 9.0x10-12 (red
arrows in lower figure).
x=-ln(PB)x=27.7x=27.2
x=26.7x=26.6
x=25.9
x=25.7
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run I: MC linearity after background selection
Test of linearity of response with MC samples containing large numbers of events.
The number of events in the plot are given before the background cut
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run I: Top mass measurement
Mt= 180.1 3.6 GeV (stat)
This new technique improves the statistical error on Mt from 5.6 GeV [PRD 58 52001,
(1998)] to 3.6 GeV. This is equivalent to a factor of 2.4 in the number of events. The number of extracted signal events is: (11±3)/(0.71 x 0.70 x 0.87)=25 ±7
(a 0.5 GeV shift has been applied, from MC studies)
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run I: W mass check
80.9 ± 2.6 GeV
(GeV) BMWM (GeV) BM
WM
The likelihood minimizes at = 79.4 GeV, with an error of 2.2 GeV. Studies at Mtop= 175 GeV show that there is a systematic shift in MW of 1.5 GeV and an under estimation of the error of 20%. Therefore
BMWM
GeV 6.29.80 WM
APS 5-MAY-2009 G. Gutierrez, Fermilab
Top and W decay
Wlq
νq’-bar
p = 40 GeV/cThe decay to jets is 3 times more likely than to e and μ
tb W
p ~ 70 GeV/cTop decays to W+b essentially 100 % of the time
Mt = 172 GeV/c2
MW = 80 GeV/c2
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run II: Top mass at D0
There were many improvements in the probability calculations. But the main gain has been to: 1) include a Jet Energy Scale (JES) parameter in the minimization and 2) use a prior from the γ+jet energy calibration.
lepton+jets most recently published result (1 fb-1)
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run II: Top mass at D0
lepton+jets most recently published result (1 fb-1)
APS 5-MAY-2009 G. Gutierrez, Fermilab
Run II: Top mass at D0
lepton+jets most recently published result (1 fb-1)
APS 5-MAY-2009 G. Gutierrez, Fermilab
Top, W and Higgs masses are related
)/ln(
and 2802.37
)1/()/1(
222
2222
WHt
ZWW
MMcmbar
GeVA
rAMMM
Accurate measurements of the top quark and W boson masses put constraints on the mass of the Higgs boson. Because of the log dependence to have meaningful constraints on the Higgs mass high precision measurement of the W and top quark masses are required.
APS 5-MAY-2009 G. Gutierrez, Fermilab
LEP EWWG as of March 2009
These (almost) lines are EW the predictions.
APS 5-MAY-2009 G. Gutierrez, Fermilab
Higgs limits as of March 2009
The SM Higgs mass limit from the EW fit is: mH<163 GeV/c2 at 95% CL.
Footnote: There is a 3 σ discrepancy between the hadronic and leptonic F-B asymmetries. If any of this two are removed there are big changes in the Higgs mass limits (see M. Chanowitz, PRD 66:073002, 2002 and Fermilab W&C 2/23/2007)
APS 5-MAY-2009 G. Gutierrez, Fermilab
gg HW+W-l+l-Basic selection:• Two opposite sign isolated
leptons• missing transverse momentum
Main backgrounds:• WW, WZ, ZZ• W+jets and Drell-Yang
Geometry help
Use full power of Matrix element
APS 5-MAY-2009 G. Gutierrez, Fermilab
HW+W- in CDF (1.9 fb-1)
Calculate probabilities
Calculate discriminant
Check for observation
If no observation set limit
APS 5-MAY-2009 G. Gutierrez, Fermilab
Conclusion
To conclude I would like to thank my colleagues for the exiting times during the past decade (when all this work was done) and many thanks to the young people that are carrying this work forward.
APS 5-MAY-2009 G. Gutierrez, Fermilab
The general method
N
ii
dxxpNxPeL
1
);();()(
),()()();(1
);( 2121 yxWqfqfdqdqydxPtt
);()();( xPxAccxP
Most people would agree that if the probability of an event could be calculated accurately then the best estimate of a parameter will maximize a likelihood like:
The detector and reconstruction effects are always multiplicative and independent of the parameter to be estimated:
The probability P(x;α) can be calculated as:
Where x is the set of variables measured in the detector, y is the set of parton level variables, dσ is the differential cross section and f(q) are the parton distribution functions. W(x,y) is the probability that a parton level set of variables y will show up in the detector as the set of variables x. The integration reflects the fact that we want to sum over all the possible parton variables y leading to the observed set of variables x.
APS 5-MAY-2009 G. Gutierrez, Fermilab
Transfer function W(x,y)W(x,y) is the probability of measuring x when y was produced (x measured variables, y parton variables):
where Ey energy of the produced quarks Ex measured (and corrected) jet energy py
e produced electron momenta px
e measured electron momenta y
j xj produced and measured jet angles
)(),()(),( 24
1
3 xi
yi
i
xi
yijet
xe
ye EEWppyxW
The energy of the electrons is considered well measured. And due to the excellent granularity of the D calorimeter the angles are also considered as well measured. A sum of two gaussians is used for the jet transfer function (Wjet), the parameters were extracted from MC simulation.
APS 5-MAY-2009 G. Gutierrez, Fermilab
Probability for tt events
2(in) + 18(final) = 20 degrees of freedom
3 (e) + 8 (1..4) + 3 (Pin=Pfinal) + 1 (Ein=Efinal) = 15 constraints
20 – 15 = 5 integrals
Sum over 12 combinations of jets
All values of the neutrino momentum are considered
1 momentum of one of the jets m
1,m
2 top mass in the event
M1,M
2 W mass in the event f(q
1),f(q
2) parton distribution functions (CTEQ4) for qq incident chann.
q1,q
2 initial parton momenta
6 six particle phase space
W(x,y) probability of measuring x when y was produced in the collision
We chose these variables of integration because |M(α)|2 is almost negligible everywhere except near the peaks of the four Breit-Wigners in |M(α)|2.
,
621
21222
22
21
211 ),(
||||
)()(|)(|),(_
combjet
ttyxW
qfqfMdMdmdMdmdxP
APS 5-MAY-2009 G. Gutierrez, Fermilab
Matrix Element
no ttbar spin correlation included s
qt sine of angle between q and t in the q q CM
top quark's velocity in the q q CM g
s strong coupling constant
Leptonic decay
Hadronic decay
Mt, MW pole mass of top and W mt top mass in any eventme ,mdu invariant mass of the e and du (or cs) systemt ,W width of top and W gW weak coupling constant(cos eb,db) angular distribution of the W decay
)2(9
|| 224
2qt
s sFFg
M
22222222
224
)()(
)(cos
)()(4 WWWe
be
tttt
etw
MMmMMm
mmgF
22222222
224
)()(
)(cos
)()(4 WWWud
bd
tttt
udtw
MMmMMm
mmgF
2
2
222 )1()1()( x
m
mxmx
t
Wt
APS 5-MAY-2009 G. Gutierrez, Fermilab
Acceptance Corrections
Detector Acceptance
Likelihood
Production probability
Detector acceptance
N
ii dxxPNxPL
1
);();(ln)(ln
);()();( xPxAccxP Measured probability
N
ii dxxPxAccNxPL
1
);()();(ln)(ln
N
jgenN
VdxxPxAcc
1
112
);()(
)()()( 2121 qfqfdqdqydV n , and Ngen(N) is the number of generated(accepted) events