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Parton Density Function Fitting Update

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Obtain usual Hessian matrix Mjk = 1. 2 2 2. pj pk s allowed to ... Obtain 2nd Hessian matrix Cj = 1. 2 2 2. pj s Systematic covariance matrix = Vsy = M-1CCTM-1 ... – PowerPoint PPT presentation

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Title: Parton Density Function Fitting Update


1
Parton Density Function Fitting Update
  • ZEUS Collaboration Meeting
  • 19-June-2003
  • Chris Collins-Tooth
  • Amanda Cooper-Sarkar, Claire Gwenlan

2
Introduction
  • How we parameterise the PDFs
  • Method for fitting data to obtain the PDFs
  • Where does the information come from for the
    fits?
  • What can we add/What data do we have to study?
  • Which parameters are best/worst determined?
  • Comparing new ZEUS O fit with old O fit and
    ZEUS-S
  • To Do Ideas for the future

3
How we parameterise the PDFs
  • At some particular value of Q02 (7 GeV2) we
    parameterise the parton momentum distribution
    with the parameters pi
  • xf(x) p1.xp2(1-x)p3(1p5x)
  • Gives flexibility at low (p2), high (p3) and mid
    (p5) x.
  • Distributions we parameterise are
  • xuv(x) u-valence p1u,p2u,p3u,p5u
  • xdv(x) d-valence p1d,p2d,p3d,p5d
  • xS(x) total sea p1S,p2S,p3S,p5S
  • xg(x) gluon p1g,p2g,p3g,p5g
  • x? x(d-u) p1?,p2?,p3?,p5?

4
  • 5 distributions ? 4 parameters 20 possible free
    params.
  • Luckily, some we can fix (eg ZEUS-S fit 11 free
    params)
  • p1u, p1d fixed through number sum rules
  • p1g fixed through momentum sum rule
  • p2u, p2d 0.5 little information exists for
    low-x valence after data cuts
  • p2? 0.5 , p3?(p3S2), p5?0 as per MRST eg EPJ
    C4, 463(1998)EPJ C14 133(2000)
  • p5g 0 since this choice constrains high-x gluon
    to be positive (leaves 11 free)
  • Additionally, for the ZEUS-O fit (ZEUS data
    only)
  • p1? fixed to value determined by ZEUS-S (10 free
    params)
  • The values are evolved in Q2 using NLO DGLAP
    equations, convoluted with coefficient functions
    in Roberts-Thorne Variable Flavour Number scheme
  • This list of parameters is fed to an evaluation
    function which calculates Chi-squared based on
    the data and theory PDFs

5
Chi-squared definition
  • ?2 ?i (Fi(p,s)-Fi(meas))2 ?? s?2
  • (?2i,stat ?2i,unc)
  • Fi(p,s) FiNLOQCD(p) ?? s? ?i?
  • Fi(meas) represents a measured data point
  • ?2i,stat and ?2i,unc represent stat. and uncorr.
    syst errors.
  • ? are systematic error sources. 1 s.d.
    uncertainty on a data point i, due to source ? ,
    is ?i ?
  • s? are independent Gaussians, with zero mean and
    unit variance.
  • Accounts for systematic errors AND
    normalisations.
  • Applied conservatively by OFFSET method
  • see J.Phys.G 28(2002) 2717

6
Fitting method
  • Parameters s? 0 for central values of fit
  • Obtain usual Hessian matrix Mjk 1 ?2?2

  • 2 ?pj?pk
  • s? allowed to vary for error analysis
  • Obtain 2nd Hessian matrix Cj? 1 ?2?2

  • 2 ?pj?s?
  • Systematic covariance matrix Vsy M-1CCTM-1
  • Stat. and uncorr. syst. covariance matrix Vst
    M-1
  • Uncertainty on any distribution (eg PDF)
    calculated using Vsy,Vst

7
  • Errors on the PDF parameters are given by the
    error matrices Vij .
  • These are propagated to quantities of interest
    like structure functions, parton densities and
    reduced cross sections via lt ? F2gt ?ij ?F Vij
    ?F

  • ?pi ?pj
  • Clearly, this is easier if V is diagonalised
  • Diagonalisation has various other benefits
  • It tells you if you have a stable fit - are the
    eigenvalues all positive?
  • It tells you if you actually NEED all the
    parameters you are using
  • It tells you which parameters are constrained
    best

8
Where does the information come from in the fits?
  • ZEUS-S, short for ZEUS-Standard is a fit using
    GLOBAL data. Some ZEUS data (96-97) is included
    in this.
  • Valence xF3 x(uvdv) from neutrino-Fe heavy
    target data
  • F2n/F2p xdv/xuv at high-x
    from muonD/p data (NMC)
  • Sea Low-x from HERA F2 e p data
  • High-x predominantly from
    fixed target F2 muonp data
  • Flavour structure from muonD
    and p
  • Gluon Low-x from HERA dF2/dlnQ2 e p data
  • High-x from mom-sum rule only
    (unless we add JET DATA)
  • ZEUS-O, short for ZEUS-Only is a fit using ZEUS
    data only.
  • Still makes some assumptions from ZEUS-S fit, eg
    p1?.
  • The old ZEUS-O fit (94-99 ZEUS data) is available
    - see
  • http//www-pnp.physics.ox.ac.uk/cooper/zeus2
    002.html for PDF sets.
  • Now, using 99/00 CC/NC ep data with correlated
    systematic error sources this fit is being
    improved.

9
What can HERA high Q2 data add?
  • TODAY HERA-I
  • High-x valence info-particularly on xdv from ep
    CC. No deuterium or heavy target corrections.
  • TOMORROW HERA-II
  • xF3/xG3 measurement valence info from low to
    high-x
  • More accurate xdv, xuv flavour separated from CC
    interactions
  • More accurate high-x sea distributions too (and
    better jet data for high-x glue)

10
What data do we have to study?
  • We have about 100pb-1 per experiment of NC and
    CC data (only 16pb-1 of it e-)
  • A new round of NLO QCD fits now to ZEUS data
    alone
  • Can use ZEUS high-Q2 data to constrain valence
    distributions independent of nuclear corrections
    needed by fixed target data.
  • ZEUS-S published fits used fixed target data and
    only 30pb-1 of NC e data.
  • Phys Rev D67, 012007 (2003)

http//durpdg.dur.ac.uk/hepdata/zeus2002.html
11
Which parameters are best/worst determined?
  • For both ZEUS-S and ZEUS-O fits, p1S and p2S are
    the best determined - ie the low-x behaviour of
    the sea.
  • Next best is the p2g - the low-x gluon
  • After that, p3u (high-x, u valence) is best
    determined from fixed target data, but high Q2
    ZEUS data is nearly as good.
  • p3d, p3S (high-x d valence and sea) and p5u
    (mid-x u valence) are moderately well determined
    by fixed target data, but in new ZEUS-O fit, high
    Q2 ZEUS ep CC data now determines p3d (high-x d
    valence) just as well
  • p3g (high-x glue) and p5S,p5g,p5d (mid-x
    sea,glue,d valence) are the least well determined
    in both fits, but are better determined from
    fixed target data.

12
ZEUS-S
New ZEUS-O 94-00 -amcs
  • At one stage, the ZEUS-S fit was used to
    determine as, by allowing it to vary as a fit
    parameter, and this error (blue) is only shown
    for reference.
  • Low-x Sea and Gluon in ZEUS-S fits were strongly
    constrained by ZEUS 96/7 ep data so are well
    constrained using ZEUS data alone

13
PUBLISHED ZEUS-O Sea and glue distributions from
ZEUS only with 94-99 data 16pb-1 e- and 30pb-1 e
NEW ZEUS-O 94-00 Sea and glue distributions from
ZEUS only with 94-00 data 16pb-1 e- and 93pb-1 e

14
ZEUS-S
NEW ZEUS-O 94-00.
  • ZEUS-S constrained valence distributions by using
    fixed target data
  • Now the new 99/00 ep data allows high-x valence
    distributions to be well constrained from a fit
    to ZEUS data alone

15
NEW ZEUS-O 94-00
PUBLISHED ZEUS-O
Valence distributions from ZEUS data alone 16pb-1
e- data and 37pb-1 e data
Valence distributions from ZEUS data alone 16pb-1
e- data and 100pb-1 e data
16
ZEUS-S
NEW ZEUS-O 94-00
NEW ZEUS-O Gluon is almost as well determined as
ZEUS-S gluon for all x
17
ZEUS-S
NEW ZEUS-O 94-00
Medium to high x sea is not as well determined
for ZEUS-O as for ZEUS-S
18
NEW ZEUS-O 94-00
ZEUS-S
Errors on high-x xuv for ZEUS-O not quite as good
as for ZEUS-S but HERA-II will improve
19
NEW ZEUS-O 94-00
ZEUS-S
Errors on High-x xdv from ZEUS-O as good as
ZEUS-S and mostly statistical so that HERA-II
will improve more!
20
NEW ZEUS-O amcs
2nd Analysis
A second analysis is underway (by me!) . Results
so far look very promising.
21
To do...
  • Investigate model dependence further - effect of
    fixing/freeing various parameters e.g.
  • valence shapes of ZEUS-O and ZEUS-S do differ
    significantly (and hence differ from MRST/CTEQ)
  • Look back and try to understand comparison of
    ZEUS-S fit with latest high Q2 data sets (seems
    higher at x0.2, so this diff could be genuine)
  • Aside- you will NOT see any difference between
    ZEUS-O and MRST if you parameterise like H1 have
    done in DESY-03-38 (their H1-only fit). In such a
    plot, a comparison ZEUS/H1 or ZEUS/MRST looks
    quite sensible!
  • Ideas
  • free low-x valence parameters
  • investigate effect of freeing/fixing sea
    parameters on valence shapes- the high-x sea also
    differs significantly from ZEUS-S fit and is not
    well determined in ZEUS-O since we have very
    little data for xgt0.4
  • vary assumptions on flavour structure of sea
  • Other model dependences not yet thought of!

22
ZEUS-O vs MRST
23
xU xD xU xD xg at Q210 and 1000 Gev2 compared to
MRST2001 (can compare to H1s plots)
But this can hide a multitude of sins!
24
For the new ZEUS-O fit, the following data is
used
96/97 ep NC 30 pb-1 2.7 lt Q2 lt 30000 GeV2 242
d.p. 10 corr..err. 2 norms 94/97 ep CC 33 pb-1
280. lt Q2 lt 30000 GeV2 29 d.p. 3 corr. err.
98/99 e-p NC 16 pb-1 200 lt Q2 lt
30000 GeV2 92 d.p. 6 corr err. 1 norm 98/99
e-p CC 16 pb-1 200 lt Q2 lt 30000 GeV2 26 d.p.
3 corr. err. 99/00 ep NC 63 pb-1 200 lt Q2 lt
30000 GeV2 90 d.p. 9 corr. err. 1 norm 99/00
ep CC 61 pb-1 200 lt Q2 lt 30000 GeV2 29 d.p.
3 corr. err.
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