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Legacy of HERA A M Cooper-Sarkar INT 10-3 October 18 2010

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Legacy of HERA A M Cooper-Sarkar INT 10-3 October 18 2010. Combination of ZEUS and H1 data and PDF fits to these data: Inclusive cross-sections HERA-1 (1992-2000):arxiv:0911.0884 - improved constraints at low-x F2(charm) data (preliminary)- constraints on the charm mass parameter, m c (model) - PowerPoint PPT Presentation
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Legacy of HERA A M Cooper-Sarkar INT 10-3 October 18 2010 Combination of ZEUS and H1 data and PDF fits to these data: 1. Inclusive cross-sections HERA-1 (1992-2000):arxiv:0911.0884 - improved constraints at low-x 2. F2(charm) data (preliminary)- constraints on the charm mass parameter, m c (model) 3. Low energy runs – FL- 2007- (preliminary) –tension with low x, Q2 data? 4. Inclusive cross-sections HERA-II (2003-2007)- (preliminary) - improved constraints at high-x Predictions for LHC cross-sections Predictions for Tevatron cross-sections Still to come F2(beauty)
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Page 1: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Legacy of HERAA M Cooper-Sarkar

INT 10-3 October 18 2010

Combination of ZEUS and H1 data and PDF fits to these data:

1. Inclusive cross-sections HERA-1 (1992-2000):arxiv:0911.0884 -improved constraints at low-x

2. F2(charm) data (preliminary)- constraints on the charm mass parameter, mc(model)

3. Low energy runs – FL- 2007- (preliminary) –tension with low x, Q2 data?

4. Inclusive cross-sections HERA-II (2003-2007)- (preliminary) -improved constraints at high-x

Predictions for LHC cross-sectionsPredictions for Tevatron cross-sections Still to comeF2(beauty)Jets and αS(MZ), perhaps forward jets

NOT COVERED: dffractive physics

Page 2: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Why combine ZEUS and H1 data?

At the LHC we collide protons Protons are full of partons. Our knowledge of partons comes from Deep Inelastic Scattering data. HERA dominates these data and is most relevant for the kinematic region of early LHC data

We think we know how to extrapolate in Q2 using (N)NLO QCD (using the DGLAP equations) but we don’t a priori know the shapes of the parton distributions in x. The HERA data is our best guide

DGLAP eqns

AT this meeting I am also allowed to say that having the highest precison measurements in the low-x region is interesing in its own right!

Page 3: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Averaging H1 and ZEUS data provides a model independent tool to study consistency of the data and to reduce systematic uncertainties:

Experiments cross calibrate each other JHEP 1001.109 arxiv:0911.0884

The combination method includes accounting for full systematic error correlations.

The resulting combination is much more accurate than expected from the increased statistics of combining two experiments. It’s like having had the best features of both detectors

The post-averaging systematic errors are smaller than the statistical across a large part of the kinematic plane

A substantial part of the uncertainty on parton distributions comes from the need to use many different input data sets with large systematic errors and questionable levels of consistency- i ncreased χ2 tolerances are used to account for this

Page 4: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

2009 average based on the complete HERA-I inclusive NC and CC DIS data: Ep=820 (s=300) and Ep=920 (s=320) GeV 200 pb-1 of e+p , 30 pb-1 of e-p

• CC e- p data: H1 98, ZEUS 98 (250 ≤ Q2 ≤ 15000 GeV2)

• CC e+p data: H1 94-97, H1 99-00, ZEUS 94-97, ZEUS 99-00 (250 ≤ Q2 ≤ 15000 GeV2)

• NC e- p data: H1 98, ZEUS 98 (200 ≤ Q2 ≤ 30000 GeV2

• NC e+p data: ZEUS 96-97, ZEUS 99-00, H1 99-00 “high Q2”,H1 96-00 “bulk”, H1 95-00 “low-Q2”, ZEUSBPC/BPT, SVX95 “low-Q2” (0.045 < Q2 < 30,000 GeV2)

The NCe+p data sets cover 5 decades of the kinematic plane in Q2 and x. The scaling violations of these data give us our best handle on the low-x gluon which is very important for Standard Model LHC physics at the W/Z scale but is also interesting in its own right

Data Sets

The new combination supercedes all these data sets

This gives 110 correlated systematic error sources

3 “procedural uncertainties” related to the averaging procedure

But they are all small !

Page 5: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

1402 data points are averaged to 741 combined data points

χ2/ndf =637/656

Combining the experiments accounting for the systematic uncertainties is like having had a much better detector

ZEUS γp background uncertainty is reduced by a factor of 3

H1 LAr hadron calorimeter energy scale uncertainty is halved

Resulting total uncertainties are <2% over a large part of the kinematic plane AND the contribution of correlated systematics to this errors is now < statistical error

Page 6: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Results of the combination compared to the separate data sets-

illustration just for a few of the NCe+ data

This page shows NC e+ combined data but NCe- and CCe+ and e- are also combined

Page 7: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

These data are used for extracting parton distributions: HERAPDF1.0

Some of the debates about the best way of estimating PDF uncertainties concern the use of many different data sets with varying levels of consistency.

The combination of the HERA data yields a very accurate and consistent data set for 4 different processes: e+p and e-p Neutral and Charged Current reactions.

Whereas the data set does not give information on every possible PDF flavour it does:

•Give information on the low-x Sea (NCe+ data)

•Give information on the low-x Gluon via scaling violations (NCe+ data)

•Give information on high-x u (NCe+/e- and CCe-) and d ( CCe+ data) valence PDFs

•Give information on u and d-valence shapes down to x~3 10-2 (from the difference between NCe+ and NCe-)

We can set the experimental uncertainties on our PDFs at 68% CL by the conventional χ2 tolerance Δχ2 = 1, because we have a consistent data set

NOTE the use of a pure proton target means d-valence is extracted without need for heavy target/deuterium corrections or strong iso-spin assumptions these are the only PDFs for which this is true

Furthermore, the kinematic coverage at low-x ensures that these are the most crucial data when extrapolating predictions from W, Z and Higgs cross-sections to the LHC

Page 8: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

d2(e-p) = GF2 M4

W [x (u+c) + (1-y)2x (d+s)] d2(e+p) = GF2 M4

W [x (u+c) + (1-y)2x (d+s)] dxdy dxdy2x(Q2+M2

W)2 2x(Q2+M2W)2

CC e-p CC e+p

•We can use the reduced cross-sections to learn about high-x valence PDFs

For NC e+ and e-

d2(e±N) = Y+ [ F2(x,Q2) - y2 FL(x,Q2) ± Y_xF3(x,Q2)], Y± = 1 ± (1-y)2

dxdy 4

22

Q

s

Y+ Y+

F2 = F2γ –ve PZ F2

γZ + (ve2+ae

2)PZ2 F2

Z

xF3 = - ae PZ xF3γZ + 2veae PZ

2 xF3Z

Where PZ2 = Q2/(Q2 + M2

Z) 1/sin2θW , and at LO

[F2 ,,F2γZ, F2

Z] = i [ei2,2eivi,vi

2+ai2][xqi(x,Q2) + xqi(x,Q2)]

[xF3γZ, xF3

Z ] = i [eiai,viai] [xqi(x,Q2) - xqi(x,Q2)]

So that xF3γZ = 2x[euauuv + edaddv] = x/3 (2uv+dv)

Where xF3γZ is the dominant term in xF3

The difference between NC e+ and e- cross-sections gives the valence structure function xF3 due to γ/Z interference and Z exchange

Note this is obtained on a pure proton target so

•No heavy target corrections

•No assumptions on strong isospin

(Unlike xF3 determined from neutrino scattering on heavy isocalar targets)

Where does the information on parton distributions come from?

Page 9: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

RESULTS for HERAPDF1.0 –arxiv:0911.0884

And here is a summary plot of the PDF results. We estimate model and parametrisation uncertainties as well as experimental uncertainties

To appreciate how much better this is than uncombined HERA data compare the red experimental errors to this plot which shows the experimental errors for a smilar PDf fit to uncombined data

Page 10: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Consequences for W and Z production at the LHC

Look at predictions for W/Z rapidity distributions: Pre- and Post-HERA

Why such an improvement

?

It’s due to the improvement in the low-x sea and gluon At the LHC the q-qbar which

make the boson are mostly sea-sea partons And at Q2~MZ

2 the sea is driven by the gluon

Note difference in scale for fractional errors

These illustrations at 14 TeV

Just fixed target DIS data ~15%

uncertainty

Separate HERA data sets~5%

uncertainty

Combined HERA data set~1.5%

uncertainty

Page 11: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

However PDF fitting should also include consideration of

model errors and parametrisation errors

HERAPDF1.0 experimental plus model errors plus parametrisation

Model errors are the most signficant in the central region: mc, mb, fs, Q2

min

mc =1.35 – 1.65 GeV is the dominant contribution… but this can be improved if F2(charm) data are used…..

Page 12: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Comparisons of W+ cross-section as a function of αS(MZ)

MSTW08CTEQ66HERAPDF1.0NNPDF2.0ABKM09GJR08

The PDF4LHC group has been considering all these PDFs at NLO

Plot from G.Watt -MSTW

Recently the PDF4LHC group has been considering the role that the uncertainty in the value of αS(MZ) plays in the overall uncertainty of predictions- PDFs are provided at a fixed αS(MZ) .

This is not a large effect for W/Z production

But the value of mc AND the scheme used to account for heavy quark production are..

NOTE many of the PDFs (NNPDF, CTEQ, MSTW,HERAPDF) are now provided for a range of αS(MZ) values

Page 13: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

H1 and ZEUS have also combined charm data recently

And the HERAPDF1.0 gives a good description of these data –within its error band-

The error band spans mc=1.35 (high) to mc=1.65 (low) GeV

The data show some preference for higher charm mass than the standard choice mc=1.4 GeV

Page 14: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

If we input the charm data to the PDF fit it does not change the PDFs significantly BUT

After charm is input the χ2 profile vs the charm mass

parameter gives

mc = 1.57 ± 0.02 GeV

Before charm is input the χ2 profile vs the charm mass

parameter is shallow..

Page 15: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

But the HERAPDF uses the Thorne General Mass Variable Flavour Number Scheme for heavy quarks as used by MSTW08

This is not the only GMVFN

CTEQ use ACOT- χ

NNPDF2.0 use ZMVFN

These all have different preferred charm mass parameters, and all fit the data well when used with their own best fit charm mass

Model and param. Errors included

We have re-analysed the HERAPDF+F2c data using several different heavy quark schemes

Page 16: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

We then use each of these schemes to predict W and Z cross-sections at the LHC (at 7 TeV) as a function of charm mass parameter

If a fixed value of mc is used then the spread is considerable (~7%)- but if each prediction is taken at its own optimal mass value the spread is dramatically reduced (~2%) even when a Zero-Mass (ZMVFN) approximation has been used

The PDFs MSTW08, CTEQ6.6, NNPDF2.0 do NOT use charm mass parameters at the optimal values- and this may explain their differing predictions.

Page 17: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

H1 and ZEUS have also combined the e+p NC inclusive data from the lower proton beam energy runs (PP = 460 and 575) and produced a common FL measurement

Page 18: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

When the low energy data are input to the HERAPDF fit it becomes evident that the low Q2/low-x data are not so well fit –

Imposing a harder Q2 cut Q2 > 5 improves the situation

The resulting PDFs have a somewhat different shape- less valence-like gluon at low Q2… steeper gluon at higher Q2

This is also true if you make an x cut x > 5 10-4 or a combined cut Q2 > 0.5 x-0.3

Page 19: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Our Regge prejudices led us to think that the sea and gluon would have soft slopes at low x ~ x -0.08 at the starting scale and THEN evolution would make them steeper. However at Q2~2

the sea has a steeper slope x -0.15

and the gluon is valence-like x +0.2 If however we distrust the formalism for low x and Q2 and we fit only data for Q2 > 5the sea has a softer slope x -0.11

But the gluon is less valence-like x +0.08

i.e. they are both closer to the Regge soft Pomeron value of -0.08

So NLO DGLAP maybe showing signs failure at low-x, Q2 But how about NNLO DGLAP?...

Page 20: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

HERAPDF1.0 is also available at NNLO for two values of αS(MZ)

since many analyses indicate that alphas seems to be smaller at NNLO than at NLO and our own data prefer a lower value

NNLO fits to HERA-I data give: First fit αS(MZ) for NLO → 0.1166 ± 0.0044(exp) χ2= 574.8 /592Then fit αS(MZ) at NNLO→0.1145 ± 0.0042(exp) χ2= 623.5 /592

NNLO is important for precision studies of cross-section uncertainties.

There are far fewer NNLO PDFS: MSTW08, ABKM

NOTE: NNLO has worse χ2 than NLO and does not fit low-x Q2 data better. The χ2 is also improved if low x, Q2 cuts are imposed.

In fact it is the 920 data which are worst fit at NNLO. Tension between the low and high-energy data shows up at low-x,Q2 and is not solved by moving to NNLO.

Page 21: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

NNLO Q2 > 5Χ2/ndf 762.4/771 X/N CCEP = 0.93 34 X/N CCEM = 0.56 34 X/N NCEP= 1.10 353 X/N NCEM= 0.76 145 X/N NCEP 460/575 = 0.85 215

NNLO using αs(MZ)=0.1145

NLO Q2 > 5Χ2/ndf 698.3/771 X/N CCEP = 0.85 34 X/N CCEM = 0.58 34 X/N NCEP= 1.03 353 X/N NCEM= 0.75 145 X/N NCEP 460/575 = 0.82 215

NLO using αs(MZ)=0.1176

NLO χ2 818.5/806 X/N CCEP = 0.86 34 X/N CCEM = 0.59 34 X/N NCEP= 1.13 379 X/N NCEM= 0.74 145 X/N NCEP 460/575 = 1.04 224

NNLO Χ2/ndf 873.7/806 X/N CCEP = 1.04 34 X/N CCEM = 0.57 34 X/N NCEP= 1.24 379 X/N NCEM= 0.75 145 X/N NCEP 460/575 = 1.07 224

Page 22: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

RT VFN χ2 818.5/806

X/N CCEP = 0.86 34 X/N CCEM = 0.58 34 X/N NCEP= 1.13 379 X/N NCEM= 0.74 145

X/N NCEP 460/575 = 1.04 224

ACOT VFN χ2 788.6/806

X/N CCEP = 0.89 34 X/N CCEM = 0.59 34 X/N NCEP= 1.09 379 X/N NCEM= 0.74 145

X/N NCEP 460/575 = 0.98 224

ACOT-χ VFN χ2 793.2/806

X/N CCEP = 0.88 34 X/N CCEM = 0.58 34 X/N NCEP= 1.13 379 X/N NCEM= 0.75 145

X/N NCEP 460/575 = 0.92 224

What about changes in the heavy quark scheme?Changes in the Thorne GMVFN make little differenceBut a change to ACOT does – this has one less power of αS in the definition of FL

And so does the use of a Fixed Flavour Number sheme

FFN χ2 724.7/738 X/N CCEP = X/N CCEM =

X/N NCEP= 1.08 379 X/N NCEM= 0.76 145

X/N NCEP 460/575 = 0.92 224

But all of these are improved further by x or Q2 cuts

Page 23: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

NOTE there is no improvement from cutting high y.

Applying x,Q2 cuts does NOT have a big effect on the description of FL.

Changes of heavy quark scheme to ACOT, FFN

or a change from NLO to NNLO have a bigger effect on FL

Describing the integrated FL vs Q2 plot and describing the full differential cross-section data for three different proton energies are not achieved in identical ways. A precision measurement of FL(x,Q2) would have been nice.

Page 24: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

575

This implies that the ‘true’ gluon could be a little bit steeper than the HERAPDF1.0 gluon- or indeed CTEQ6.6 or MSTW08 gluons

However this effect only starts to become important for x < 10-3 so W/Z cross-sections at the LHC are only marginally affected- 1-1.5% up at 7 TeV

Returning to NLO fits: How hard do we need to cut such that DGLAP fits of just Ep=920 data and fits including lower energy data are once more in good agreement?

Q2 > 1.0 x-0.3

Page 25: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

HERA- I combination only ~250 pb-1 of data

HERA-II gives 4 times as much data in total

The triggers were such that most of this is at higher x and Q2

We have made a preliminary HERA-II combination- not all of the separate ZEUS and H1 inclusive data which go into this combination are yet published.

Page 26: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

H1 and ZEUS have also combined preliminary high Q2 HERA-II data along with the HERA-I data and HERAPDF1.0 has recently been updated to HERAPDF1.5 by including these data

The data on the left has been updated to the data on the right

The HERAPDF1.0 fit on the left has been updated to the HERAPDF1.5 fit on the right

Page 27: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

The data on the left has been updated to the data on the right

The HERAPDF1.0 fit on the left has been updated to the HERAPDF1.5 fit on the right.

The CCe- data is improved because at HERA-1 there were only 30 pb-1 of e- data, at HERA-II there are ~350pb-1

Page 28: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

The data on the left has been updated to the data on the right

The HERAPDF1.0 fit on the left has been updated to the HERAPDF1.5 fit on the right

In this case ~200pb-1 of HERA-I data has been supplemented by ~300pb-1 of HERA-II data. Extra CCe+ helps to determine the d quark at high-x

Page 29: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

The PDF uncertainties have been reduced at high-x

These plots show total uncertainties (model and parametrization included)

Improved determination of the d/u ratio at high-x.

The only PDF which measures d in a proton rather than an isoscalar target

Page 30: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

This reduced high-x error results in a reduced error at high rapidity for W/Z production at the LHC

Page 31: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

How about Tevatron results?

We don’t include Tevatron data in the fits but we can describe it – we CAN describe Tevatron jet data despite having a relatively soft gluon (we have harder quarks) AND we have a reasonable description of the D0 electron asymmetry data which is troublesome for some of the PDFs

Note some of the trouble comes from tension with NMC and BCDMS fixed target deuteron data- deuterium corrections are one possible explanation- the HERAPDF uses only proton data and is not subject to this uncertainty

Page 32: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Things still to come:

Inclusion of F2b- more information on gluon/heavy quark schemes

Inclusion of HERA jets data--- decrease in gluon uncertainty using fixed αS(MZ)-- decrease in gluon uncertainty using free αS(MZ) and determination of alphas and PDF simultaneously within the fit --decrease in the uncertainty of αS(MZ)

NOTE the HERA-jet data already give very competitive αS(MZ) determinations (not covered here)

Jet illustrations use ZEUS combined

HERA not yet ready

Page 33: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Comparison to conventional LO and NLO calculations- NLO below

data, especially at small xBj

What about Forward Jets?- combined data are still to comeWhat about Forward Jets?- combined data are still to come

Look at the hadron final states..lack of pt ordering has its consequences. Forward jets with xj » x and ktj 2 ~ Q2 are suppressed for DGLAP evolution but not for kt disordered BFKL evolution

Page 34: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

But there are some things that HERA did not do

(apart from fail to fully exploit the low-x region!):

flavour separation in the sea

Strangeness has been assigned a large model error at Q2

0=2

sbar = (0.45± 0.15) dbar

Could HERA measure strangeness?

W+ +s → c

Charm production in CCe+..

There is still some work going on, but statistics will be poor

There is also some HERMES data which suggests that strange is not the same shape as dbar….

Page 35: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Then there is dbar-ubar

We know this is not zero at high-x from E866 Drell-Yan measurements

The HERAPDFs are NOT in disagreement with this but could do better!

Along with most other PDFs it assumed that dbar=ubar at small-x

What if we relax this assumption…

This Toy PDF is called the HERAPDF1.u ‘unconstrained’ or ‘dissident’ PDF

It comes in two varieties:

1. dbar≠ubar at small x

2. dbar≠ubar at small x plus strangeness fixed to the HERMES shape

Page 36: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

The dissident fit has dbar very much smaller than ubar at small-x (although slightly larger at high-x so not in disagreement with Drell-Yan data).

Page 37: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

As Q2 increases the difference between dbar and ubar remains constant but the size of ubar and dbar increase rapidly at low-x so that by Q2~MW,Z

2 this difference is not very significant. However for the LHC it is still visible….

Strangeness evolves to become almost the same size as dbar, ubar and the difference in the Standard and the HERMES strangeness is not significant

Page 38: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

For the Tevatron x values are higher and W,Z are q-q dominated so such a

‘dissident’ PDF is not excluded

For the LHC there should be obvious differences – we may even be able to exclude this with data taken this year

Page 39: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

SUMMARYCombination of ZEUS and H1 data and PDF fits to these data:

1. Inclusive cross-sections HERA-1 (1992-2000):arxiv:0911.0884 -improved constraints at low-x

2. F2(charm) data (preliminary)- constraints on the charm mass parameter, mc(model)

3. Low energy runs – FL- 2007- (preliminary) –extends the kinematic reach in the same direction as EIC-- tension with low x, Q2 data?

4. Inclusive cross-sections HERA-II (2003-2007)- (preliminary) -improved constraints at high-x ----using only proton target

Still to come:

1. F2(beauty)

2. HERA jet data

What HERA could not do: u,d,s flavour separation in the SeaWhat HERA did not do: fully exploit the low-x region, precision measurement of FL

Page 40: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

extras

Page 41: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

LHeC

PDF improvement

100 GeV e on 7 TeV

Page 42: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

LHeC

Low-x

Expansion of the kinematic regime so that low-x, x~10-4 now has Q2 up to 100 rather than 10

Can measure F2 and FL and hope to distinguish models with/without saturation etc

Page 43: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

• Swim all points to a common x-Q2 grid• Moved 820 GeV data to 920 GeV p-beam energy• Calculate average values and uncertainties

This is done by making a χ2 fit to the data points of both experiments which simply assumes that for each process (NC or CC, e+ or e-) and each x, Q2 point (i) there is only one ‘true’ value of the cross-section- these are the predictions mi – whereas there can be several measurements of this value, from ZEUS and H1 and from different years of running- these are the measurements µi

• The chisq accounts for the correlated systematics of the data points- each data point can have several such uncertainties Γ, hence sum over j for each data point i, but these uncertainties are common to all data points for large sub-sets of data. The fit determines the value of the cross-sections mi and the systematic shift parameters bj

• Evaluate further uncertainties due to choices in combination procedure,e.g. Correlations between ZEUS and H1

Averaging procedure

Page 44: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

1402 data points are averaged to 741 combined data points

χ2/ndf =637/656

Systematic shift parameters b, shift most systematics < 1 std deviation

But the fit also determines uncertainties on the shift parameters Δb, some of these are much reduced e.g

ZEUS γp background uncertainty is reduced by a factor of 3

H1 LAr hadron calorimeter energy scale uncertainty is halved

Resulting total uncertainties are <2% over a large part of the kinematic plane AND the contribution of correlated systematics to this errors is now < statistical error

Page 45: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

The data combination results in a data set which not only has improved statistical uncertainty, but also improved systematic uncertainty.

Even though there are 113 sources of correlated systematic uncertainty on the data points these uncertainties are small. The total systematic uncertainty is significantly smaller than the statistical uncertainty across the the kinematic region used in the QCD fits

This means that the method of treatment of correlated systematic uncertainties in our PDF fits is not crucial. We obtain similar results treating all systematic errors as correlated or as uncorrelated.

For our PDF fits we combine 110 sources of systematic uncertainty from the separate experiments in quadrature and OFFSET the 3 procedural systematics which derive from the method of data combination.

We set the experimental uncertainties on our PDFs at 68% CL by the conventional χ2 tolerance

Δχ2 = 1

Correlated systematic uncertainties, χ2 and Δχ2

Page 46: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

We chose to fit the PDFs for:

gluon, u-valence, d-valence and the Sea u and d-type flavours:

Ubar = ubar, Dbar = dbar+sbar (below the charm threshold)

To the functional form

The normalisations of the gluon and valence PDFs are fixed by the momentum and number sum-rules resp. Further constraints are:

B(d-valence) = B(u-valence), B(Dbar) = B(Ubar), low-x shape of Sea same for u-type+d-type

A(Ubar) = A(Dbar) (1-fs), where sbar = fs Dbar, so that ubar → dbar as x→ 0 (fs=0.31)

Theoretical framework

Fits are made at NLO in the DGLAP formalism -using QCDNUM 17.00

The Thorne-Roberts massive variable flavour number scheme is used (2008 version) and compared with ACOT

The staring scale Q20 (= 1.9 GeV2) is below the charm mass2 (mc=1.4 GeV) and charm and

beauty (mb=4.75) are generated dynamically

A minimum Q2 cut Q2 > 3.5 GeV2 is applied to stay within the supposed region of validity of leading twist pQCD (no data are at low W2 )

Parametrisation and model assumptions

Page 47: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Uncertainties due to model assumptions are evaluated by varying input values

Variation of heavy quark masses:

Mc=1.35 to1.65 GeV (the pole-mass)

Mb= 4.3 to 5.0 GeV

Variaion of the sea fraction

Fs=s/(d+s) = 0.23 to 0.38

Variation of the minimum Q2 cut on data entering the fit

Q2 min= 2.5 to5.0 GeV2

We also vary the value of the starting scale Q20 from1.5 to 2.5 GeV2:

this is considered as a parametrisation uncertainty rather than a model uncertainty…

Page 48: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Parametrisation uncertainties- indicative, not exhaustive

The central fit is chosen as follows: start with a 9 parameter fit with all D and E parameters = 0 and then add D and E parameters one at a time noting the χ2 improvement. Chose the fit with the lowest χ2. This has E(u-valence) ≠ 0 and χ2/ndf = 574/582.

This is the central fit

We then start with this 10 parameter fit and add all the other D and E parameters one at a time noting the χ2 improvement. It turns out that there is no significant further improvement in χ2 for 11 parameter fits.

An envelope of the shapes of these 11 parameter fits is formed and used as a parametrization error. This gives the parametrization uncertainty at high-x.

Low-x parametrisation uncertainty is accounted for by the following additional variations:

1. Bdv free –this results in Bdv ≈ Buv 2. A negative gluon term: - A xB(1-x)C is added to the usual gluon term, when the

starting scale of the fit is lowered to Q20=1.5 GeV2 – this results in a small –ve gluon

term but the gluon itself does not become negative in the kinematic range of the data

Page 49: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010
Page 50: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

And compared to alternative theoretical predictions:

White and Thorne (WT) which has NLL ln1/x resummation

included

Dipole Models which can accommodate non-linear effects/

saturation eg IIM colour glass condensate

So do we have a smoking gun?

Maybe not- but the circumstantial evidence is building up….

Compared to various NLO DGLAP fits

Page 51: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

HERAPDF1.0 has a rather high q-qbar luminosity at high scale.

This is reduced in HERAPDF1.5

The PDF4LHC group has been comparing PDFs at the level of parton-parton lumiosities

Plot from G.Watt -MSTW

Page 52: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Let’s look at the modern PDFsetsMSTW08CTEQ66HERAPDF1.0NNPDF2.0ABKM09GJR08Overall disagreement ~8% in W, Z cross-sectionsThe PDF4LHC recommendation is to take the envelope of the NNPDF, MSTW, CTEQ predictions --even this may not be enough!

Plots from G.Watt -MSTW

Page 53: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Plots from G.Watt -MSTW

Page 54: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Plots from G.Watt -MSTW

Page 55: Legacy of HERA A M Cooper-Sarkar INT 10-3  October 18 2010

Spread in Higgs production cross-sections is now > 15%

Dependence on alphas is also increased

Plots from G.Watt -MSTW


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