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25/03/2008 H1Z Meeting Joël Felt esse 1 Update on QCD Fits, error estimates

Update on QCD Fits, error estimates

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Update on QCD Fits, error estimates. Outlook. Parameterizations Assumptions for central fit Systematics from model dependence Variations Options to be decided. Parameterizations. All based on the same PDF functional form : x f(x) = A x B (1 - x) C (1 + D x + E x 2 +F x 3 ) - PowerPoint PPT Presentation

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25/03/2008 H1Z Meeting Joël Feltesse 1

Update on QCD Fits,error estimates

25/03/2008 H1Z Meeting Joël Feltesse 2

Outlook

• Parameterizations• Assumptions for central fit• Systematics from model dependence• Variations• Options to be decided

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Parameterizations

• All based on the same PDF functional form :

x f(x) = A xB (1 - x)C (1 + D x + E x2 +F x3 )

• The optimal number of parameters depend on the data set.

• The former ‘H1 parameterization’ (H1PDF2K), ‘ZEUS-Jet’, ‘Inbetween’ (EP) have been optimised to the H1-ZEUS combined data set (see previous meetings)

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Comparison between parameterizations

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Comparison between parameterizations

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Additional assumptions for heavy quark

• H1 param : s = 0.33 Dbar• ZEUS param : (s + sbar) = 0.2 sea• Wthin the Zero Mass Variable Flavour Number (ZMVFN)

– H1 : charmed quark = 0.15 Ubar above threshold.– ZEUS : charmed quark, dynamically introduced by

evolution • H1 parameterization: dbar/ubar → 1 as x → 0. • ZEUS param’s : dbar – ubar = fixed function of x• In between : same assumptions as H1 parameterization.

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Choice of parameterization

• All parametrizations give an excellent Chi2 / 573 :– Inbetween : 476.3– H1 param : 479.1– ZEUS_Jet : 475.6

• Chosen central parameterization : ‘optimized Inbetween’ • Motivations :

– Less model dependence on B parameters than in H1 param.– No need for an additional input (ubar-dbar) x distribution as in

ZEUS-Jet param– Most conservative errors.– It is inspired by both H1 and ZEUS parameterizations.

• The two other parameterizations are considered in the model dependence or in the variations ?

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Central fit uses :

• The data sets which we have already been using for our comparisons- not any new MB99 or ZVTX 2000 (low Q2 from H1).

• Parameterization : ‘optimized in_between‘• DGLAP NLO fit based on QCDNUM package• alpha_s = PDG 2006 = 0.1176• Cuts Q2 = 3.5 GeV2

• Q02 = 4. GeV2

• mc = 1.4 GeV2

• mb = 4.75 GeV2

• fs = 0.33• fc = 0.15• ZMVFNS • Chi2 definition : uncorrelated for the 43 errors of the two

experiments, but correlated for the 4-procedural errors (here Hessian method, but ZEUS uses offset method)

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Model dependence

Each source to be considered as a variation from the central job.1) Q0

2 = 2.0 GeV2 - 6.0 GeV2

2) Q2 min = 2.5 GeV2 - 5.0 GeV2

3) mc = 1.3 GeV2 - 1.55 GeV2

4) mb = 4.3 GeV2 - 5. GeV2

5) fs = 0.25 – 0.406) fc = 0.10 – 0.207) Optimized  H1 and New ZEUS_JETS parameterization

(debatable)

Each systematic effect has been compared between H1 and ZEUS package → Excellent agreement.(one minor issue : Q2 min = 2 (H1) or 2.5 (ZEUS))

Excellent agreement also with QCDFIT (Li et al.) tested on a few key issues.

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Variation of Q02 of

the input parameterization

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Variation of the Q2 cut applied to the

data

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Variation of the Q2 cut applied to the

data

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Variation of fs,the fraction of Dbar strange = fs * dbar

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Variation of fc,the fraction of cbar charm = fc * Ubar

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Variation of mb, the mass of b quark

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Blue : experimental errorsRed : (exp + model) errors.

Q2 = 4 GeV2

uv

dv

gluon

All model dependence with uncertainty on input parametrisation(i.e. 7 sources)

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All model dependence without uncertainty on input parametrisation(i.e. 6 sources)

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Blue : experimental errorsRed : (exp + model) errors.

Q2 = 4 GeV2

Ubar

Dbar

Sea

All model dependence with uncertainty on input parametrisation(i.e. 7 sources)

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All model dependence without uncertainty on input parametrisation(i.e. 6 sources)

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Variation with Q2

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Blue : experimental errorsRed : (exp + model) errors

Q2 = 10000 GeV2

uv

dv

gluon Impressive shrinkage oferrors at low x

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Blue : experimental errorsRed : (exp + model) errors

Q2 = 10000 GeV2

Ubar

Dbar

Sea

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Variations - not model dependences.

Not to be added together in quadrature but shown separately.– use of general mass VFN -like Robert Thorne's or

(and) ACOT (not yet ready but not mandatory for preliminary results)

– use of alpha_s = 0.1176 +/- 0.002 – use of humpy not straight solution.

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Alpha_s variation +- 0.002

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Comparison between straight and humpy minima

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Comparison with humpy solution

Reminder : two minima havebeen observed:Chi2 straight = 476.3 / 573Chi2 humpy = 494.6 / 573(With original inbetween parameterization)

All model dependence with uncertainty on input parametrisation without double minima

uv

dv

gluon

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All model dependence with uncertainty on input parametrisationand on double minima(i.e.8 sources)

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Comparison with published H1 and ZEUS PDFs (2002-2003)

Without double minima uncertainty

Much narrowerError band !

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Comparison with published H1 and ZEUS PDFs (2002-2003)

With double minima uncertainty

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Comparison with published H1 and ZEUS PDFs (2002-2003)

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Comparison with published H1 and ZEUS PDFs (2002-2003)

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New H1/ZEUS combined PDFs with total experimental uncertainty bands plus model uncertainty bands from 6 sources of model variation:

AT THE STARTING SCALE Q20 = 4 GeV2

Last result from ZEUS Package Last result from H1 Package

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New H1/ZEUS combined PDFs with total experimental uncertainty bands plus model uncertainty bands from 6 sources of model variation:

AT THE STARTING SCALE Q20 = 4 GeV2

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New H1/ZEUS combined PDFs with total experimental uncertainty bands plus model uncertainty bands from 6 sources of model variation:

AT THE STARTING SCALE Q20 = 4 GeV2

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Final options to decide today

• Q2 min = 2.5 or 2 GeV2 ?• Offset or Hessian for the 4 correlated errors ?

• Add parameterizatios uncertainty in model dependence or show it as a variation ?

• Add double minima uncertainty in model dependence or show it as a variation ?

• Which plots do we want to be stamped by H1 and ZEUS ?

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EXTRA SLIDES

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The sources of procedural errors related to the averaging procedure :

– Center of Mass Energy correction

– Multiplicative vs additive systematic errors

– Uncertainty on correlations between experiments

They are at the few permille level across most of

kinematic plane (with few exceptions)

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Results of ZEUS-Jet

Old ZEUS-JET parametrisation (11 parameters) A B C D E!

gluon From Sum Rule

0.

uv From Sum Rule

0.

dv From Sum Rule

= Buv 0.

ubar - dbar from Z_S_11 fit

from Z_S_11 fit

from Z_S_11 fit

0. 0.

Sea

0. 0.

New ZEUS-JET parametrisation (11 parameters) A B C D E!

gluon From Sum Rule

0.

uv From Sum Rule

0.

dv From Sum Rule

= Buv 0.

ubar - dbar from Z_S_11 fit

from Z_S_11 fit

from Z_S_11 fit

0. 0.

Sea

0. 0.