The New HERAPDF Nov26 2008 HERA SFgroup AM Cooper-Sarkar Appears compatible with HERAPDF0.1 when doing fits at Q20=4.0 GeV2 But humpy gluon is Chisq favoured.

Slides:



Advertisements
Similar presentations
Formal Computational Skills
Advertisements

High Energy neutrino cross-sections HERA-LHC working week Oct 2007 A M Cooper-Sarkar, Oxford Updated predictions of high energy ν and ν CC cross-sections.
Mr Barton’s Maths Notes
H1/ZEUS averaging meeting Sep 22 nd 2008 A M Cooper-Sarkar Studies on heavy quark scheme LHAPDF implementation.
Measurement of FL at HERA Have we seen anything beyond (N)NLO DGLAP? AM Cooper-Sarkar for the ZEUS and H1 Collaborations Why measure FL? How to measure.
Precision Measurement of F 2 with H1 Workshop on DIS and QCD, Florence, Max Klein for the H1 Collaboration Towards today The Measurement Results.
1 META PDFs as a framework for PDF4LHC combinations Jun Gao, Joey Huston, Pavel Nadolsky (presenter) arXiv: , Parton.
Report on fitting FINAL new data: e- CC (175pb -1 : P=0.30, 71pb -1, P=-0.27, 104pb -1 )(DESY ) e- NC (169pb -1, P=+0.29, P=-0.27)(DESY ) Now.
Investigate model uncertainties OLD/NEW But what about u,d,s,c?
HERAPDF0.2 and predictions for W/Z production at LHC PDF4LHC A M Cooper-Sarkar 29 May 2009 Motivation Some of the debates about the best way of estimating.
H1/ZEUS fitters meeting Jan 15 th 2010 Am Cooper-Sarkar Mostly about fitting the combined F2c data New work on an FFN fit PLUS Comparing HERAPDF to Tevatron.
HERAPDF0.2 and predictions for W/Z production at LHC PDF4LHC A M Cooper-Sarkar 29 May 2009 Motivation Some of the debates about the best way of estimating.
We illustrate some of the other choices as variations compared to our central value: α S (Mz) = → New H1 ‘optimized’ parametrization New.
The Analysis of Variance
Studies on heavy quark scheme. Comparison of central fit plus total uncertainties to variation of heavy quark scheme: using massive variable flavour number.
Systems of Linear Equations
Senior Cycle Crana College. First lay down a basic outline. You can either grid or freehand your outline. I prefer to grid because it's a lot faster and.
Mixed-level English classrooms What my paper is about: Basically my paper is about confirming with my research that the use of technology in the classroom.
Psy B07 Chapter 8Slide 1 POWER. Psy B07 Chapter 8Slide 2 Chapter 4 flashback  Type I error is the probability of rejecting the null hypothesis when it.
Key Stone Problem… Key Stone Problem… next Set 22 © 2007 Herbert I. Gross.
TH EDITION Copyright © 2013, 2009, 2005 Pearson Education, Inc. 1 1 Equations and Inequalities Copyright © 2013, 2009, 2005 Pearson Education,
Update on fits for 25/3/08 AM Cooper-Sarkar Central fit: choice of parametrization Central fit: choice of error treatment Quality of fit to data PDFs plus.
Announcements Homework returned now 9/19 Switching to more lecture-style class starting today Good luck on me getting powerpoint lectures ready every day.
Why Bother. I have a Calculator!  You might press a button wrong. It is good to have an idea of what your answer should be.  These visualizations and.
Frictionless Friction and Simply Simple Machines Nathan Smart October 23, 2009
Benefits/Features/Specs Benefits, Features, Specs Benefits, Features, Specifications (and Targets)
O. Music Classrooms and Teaching Spaces: These are used for teachers and children. They can be used for music practical and music theory.
STAR Sti, main features V. Perevoztchikov Brookhaven National Laboratory,USA.
ZEUS PDF analysis 2004 A.M Cooper-Sarkar, Oxford Low-x 2004 New Analysis of ZEUS data alone using inclusive cross-sections from all of ZEUS data from HERA-I.
Update of ZEUS PDF analysis A.M Cooper-Sarkar, Oxford DIS2004 New Analysis of ZEUS data alone using inclusive cross-sections from all of HERA-I data –
May 14 th 2008 averaging meeting A M Cooper-Sarkar Look at the HERA-I PDFs in new ways Flavour break-up High-x Compare to ZEUS data alone/ H1 data alone.
Predictions for high energy neutrino cross-sections from ZEUS-S Global fit analysis S Chekanov et al, Phys Rev D67, (2002) The ZEUS PDFs are sets.
PDF fitting to ATLAS jet data- a first look A M Cooper-Sarkar, C Doglioni, E Feng, S Glazov, V Radescu, A Sapronov, P Starovoitov, S Whitehead ATLAS jet.
PDF fits with free electroweak parameters Overview of what has happened since March’06 Collaboration meeting Emphasis on the NC couplings au,vu,ad,vd and.
Flavour break-up July7th 2008 Our aim was modest: 1)To alter fc=0.15 to fc=0.09 following investigations of the charm fraction 2)To take into account the.
By: Maisha Loveday 8C Maths Reflection: Binomial Expansion.
Quadratic Regression ©2005 Dr. B. C. Paul. Fitting Second Order Effects Can also use least square error formulation to fit an equation of the form Math.
HERA-LHC workshop 21 st -24 th March 2005 Claire Gwenlan (with the help of Sasha Glazov, Max Klein, Gordana Lastovicka-Medin, Tomas Lastovicka)  Introduction.
NLO QCD fits How far can we get without jet data/HERA-II data? A. M. Cooper-Sarkar March-04 Collaboration Meeting ZEUSNOTE Extended ZEUS-S fits.
More on NLOQCD fits ZEUS Collab Meeting March 2003 Eigenvector PDF sets- ZEUS-S 2002 PDFS accessible on HEPDATA High x valence distributions from ZEUS-Only.
Further investigations on the fits to new data Jan 12 th 2009 A M Cooper-Sarkar Considering ONLY fits with Q 2 0 =1.9 or 2.0 –mostly comparing RTVFN to.
Treatment of correlated systematic errors PDF4LHC August 2009 A M Cooper-Sarkar Systematic differences combining ZEUS and H1 data  In a QCD fit  In a.
In the context of the HERA-LHC workshop the idea of combining the H1 and ZEUS data arose. Not just putting both data sets into a common PDF fit but actually.
11 QCD analysis with determination of α S (M Z ) based on HERA inclusive and jet data: HERAPDF1.6 A M Cooper-Sarkar Low-x meeting June 3 rd 2011 What inclusive.
June 1st 2008 averaging meeting A M Cooper-Sarkar Model dependence fs Model dependence fc Model dependence need to be consistent when varying Q2_0 Model.
When the program is first started a wizard will start to setup your Lemming App. Enter your company name and owner in the fields designated “Company Name”
In the QCD sector the PDFs limit our knowledge - transport PDFs to hadron-hadron cross-sections using QCD factorization theorem for short-distance inclusive.
Sorting Algorithms Written by J.J. Shepherd. Sorting Review For each one of these sorting problems we are assuming ascending order so smallest to largest.
H1 and ZEUS Combined PDF Fit DIS08 A M Cooper Sarkar on behalf of ZEUS and H1 HERA Structure Function Working Group NLO DGLAP PDF fit to the combined HERA.
Algebra Geek Patrol The Pocket Protectors of Algebra  2007 Scott Endres.
MSTW update James Stirling (with Alan Martin, Robert Thorne, Graeme Watt)
Tools08 1 st July1 PDF issues for Monte Carlo generators Peter Richardson IPPP, Durham University.
Reliability of Disk Systems. Reliability So far, we looked at ways to improve the performance of disk systems. Next, we will look at ways to improve the.
1 Proton Structure Functions and HERA QCD Fit HERA+Experiments F 2 Charged Current+xF 3 HERA QCD Fit for the H1 and ZEUS Collaborations Andrew Mehta (Liverpool.
1 A M Cooper-Sarkar University of Oxford ICHEP 2014, Valencia.
HERAPDF1.0 and predictions for W/Z production at LHC PDF4LHC A M Cooper-Sarkar August 2009 Motivation Some of the debates about the best way of estimating.
1 Proton Structure and Hard QCD AM Cooper-Sarkar, Oxford Phys Rev D93(2016)
AM Cooper-Sarkar PDF4LHC July 4th 2010 HERAPDF fits update We have more combined H1 + ZEUS data: The low energy run data which was used to measure FL has.
Michigan State University
News from HERAPDF A M Cooper-Sarkar PDF4LHC CERN March
AMCS, A Glazov, V Radescu, S Whitehead, A Sapronov
Error Handling Summary of the next few pages: Error Handling Cursors.
HERA I - Preliminary H1 and ZEUS QCD Fit
Treatment of heavy quarks in ZEUS PDF fits
Where did we stop? The Bayes decision rule guarantees an optimal classification… … But it requires the knowledge of P(ci|x) (or p(x|ci) and P(ci)) We.
Sorting "There's nothing in your head the sorting hat can't see. So try me on and I will tell you where you ought to be." -The Sorting Hat, Harry Potter.
May 14th 2008 averaging meeting A M Cooper-Sarkar
ATLAS 2.76 TeV inclusive jet measurement and its PDF impact A M Cooper-Sarkar PDF4LHC Durham Sep 26th 2012 In 2011, 0.20 pb-1 of data were taken at √s.
Presentation transcript:

The New HERAPDF Nov HERA SFgroup AM Cooper-Sarkar Appears compatible with HERAPDF0.1 when doing fits at Q20=4.0 GeV2 But humpy gluon is Chisq favoured and there are two humpy mimima Fitting with Q20=1.9 GeV2 is tricky Straight gluon is favoured but shape of d-valence has changed a lot and is softer than d-bar at high-x This situation is improved if GMVFN rather than ZMVFN dynamical heavy quark scheme is used Moving from QCDNUM16 to QCDNUM17 gives the possibility of greater accuracy at high-x A combination of QCDNUM17 quadratic spline interpolation on the high-x grid, and the use of GMVFN give results compatible with HERAPDF0.1 (and by implication with CTEQ MRSTW etc)

Fit to new post-Oct data set, using formalism of HERAPDF0.1 gives very compatible results 19 extra points brings total to 592 data points: Chisq errors added in quadrature- no procedural as yet Chisq/ndp for NCe+ data increases to 1.10

Let’s see the comparison of new to old in more detail for various flavours Conclusion: compatible

Fit to new post-Oct data set, using ZEUS-JETS parametrization gives total chisq 574 and very compatible results: both to old ZEUS-JETS and to new fit using HERAPDF0.1 form of parametrization Now look at alternative parametrizations: first ZEUS-JETS optimization gives the same form of parametrization as in April 2008

The PDF uncertainties for the inbetween parametrization (left) are more conservative than those for the zeus-jets parametrization (middle) and than the H1 parametrization (right) just as we found earlier. Inbetween styleZeus-jets style H1-style

Let’s see the comparison of new inbetween to new zeus-jets in more detail for various flavours Conclusion: broadly compatible, need model dependence to really judge

Now look at alternative parametrizations: humpy version of inbetween Fit to new post-Oct data set, using humpy gluon parametrization with ‘inbetween’ Humpy-2 Chisq 559 is now preferred Humpy-2 is preferred by NC e+ data: chisq/ndp 1.06 compared to 1.10 It is not preffered by CCe+: chisq/ndp 0.82 compared to Other data set Chisq do not change much

Let’s see the comparison of Humpy-2 to straight in more detail for various flavours Conclusion: more or less as we saw it when investigating HERAPDF0.1

But I have not been following strict historical order First I found another humpy solution with an identical Chisq=559 Humpy-1 is preferred by NC e+ data: chisq/ndp 1.05 compared to 1.10 It is not preffered by CCe+: chisq/ndp 0.90 compared to This change in the CCe+ fit is what is giving the big change in d-valence (HERA-II CCe+ data could change this). The resulting d-valence is very soft- softer than dbar at high-x Now look at alternative parametrizations: another humpy version of inbetween It’s not the humpiness it’s the valence that worries me it’s the valence shapes

Let’s see the comparison of Humpy-1 to straight in more detail for various flavours Conclusion: not at all like we saw when investigating HERAPDF0.1 MUCH more model dependent NOTE: Joel found only Humpy-1, Gang-li found Humpy-2, I can find both if my start parameters are shifted

This is a fit with Q20=1.9 using the ‘inbetween’ parametrization. For Q20=1.9 the straight gluon solution is preferred. Now we see that the alternative behaviour of the valence has nothing to do with Humpyness of the gluon. It is hard to get the original HERAPDF0.1 valence shapes with low Q20. In fact low Q20 fits are much less stable Again d-valence is softer than d- bar at high-x Now start looking at jobs with low Q20, so that we can move to dynamic heavy quark treatment and to the NNLO QCDNUM programme Remember HERAPDF NEW means fitting with Q20=4 exactly as for HERAPDF0.1 AND it is compatible with HERAPDF0.1

Let’s see the comparison of Q20=1.9 to Q20=4.0 straight gluon solutions for fits to the new data in more detail for various flavours Conclusion: very large model dependence- and some amount of embarassment wrt what we have already said to the world- also if we use this Q20=1.9 minimum for our central value we’ll be way out of line with CTEQ/MSTW Also if you look in detail you will see that dbar > dvalence at large x> 0.7

NOTE the problem is not just the low start point We used to get compatible shapes from q20=2.0 before the new data were added This shows the OLD Q20=2.0 compared to HERAPDF NEW with Q20=4.0

Let’s see the comparison of Q20=2.0 to Q20=4.0 straight gluon solutions for fits to the older data in more detail for various flavours Conclusion: only modest model dependence for older data The new data is now emphasing the preferences of the NCe+ sample such that the ‘needs’ of the CCe+ sample are downgraded- we have thus relatively less information on d-valence. We have find a way to live with this - until we combine HERA-II (or possibly assign larger weight CCe+ - CTEQ have done this sort of thing in the past).

Of course the newer type of solution could be the correct one but since it has some nasty features I have tried various ways to recover the old one. Many unsuccessful tries with penalty Chisq, setting limits on parameters-even with fully hessian error treatment Some success with moving to Robert Thorne’s heavy quark variable flavour number scheme (2008 version more compatible to ACOT) Since the point of the move to low Q20 was to implement these schemes this is relatively good news. I remain somewhat uneasy about all this and the d-valence remains somewhat soft. The work comparing this to similar jobs with Q20=4.0, alternative parametrizations etc. has yet to be done. Now move to a dynamically generated heavy quark variable flavour number scheme

Early problems with beta-00, beta- 01 are now solved NOTE this programme is NOT BACKWARD COMPATIBLE you have to completely re-write your user routine. Motivation to use it at NLO: Botje pays more attention to accuracy at high-x Linear and quadratic spline interpolation on the x grid is available. GOOD NEWS: linear is compatible to QCDNUM16– I have recovered a similar unpleasant soft d-valence solution (see next page) BAD NEWS: quadratic is significantly different – it has somewhat harder d-valence (but still not harder than d-bar) Now move to NNLO QCDNUM:QCDNUM17-beta-02 BUT USE it at NLO

Compare the Q20=1.9 solution with QCDNUM16– red line To the Q20=1.9 solution with QCDNUM17 linear spline interpolation –black line and yellow band Compatibility of QCDNUM 16/17: Well compatibility between QCDNUM versions is GOOD, though still getting the soft d- valence doesn’t thrill me

Comparison of linear and quadratic spline interpolation in more detail Incompatibility of quadratic and linear is BAD since it means we’ve probably never been sufficiently accurate at high-x

Finally move to a dynamically generated heavy quark variable flavour number scheme But using QCDNUM17 linear and quadratic Compare the Q20=1.9 solution with QCDNUM16– red line To the Q20=1.9 solution with QCDNUM17 linear spline interpolation –black line and also note that the quadratic red-line d- valence is harder

Comparison of linear and quadratic spline interpolation for dynamical heavy quark variable flavour number in more detail

Conclusions Everything looks OK (definition: similar to what we saw before) if we stick to Q20=4.0 (except that we have a double minimum in humpy solutions!) We could stick to Q20=4 even for dynamic heavy quark generation since it is POSSIBLE to evolve backwards However we’ll have to face low Q20 for NNLO eventually. Low Q20 fits are tricky. For Q20~2.0 we have a ‘new look’ for the d-valence (and a bit for u-valence) which is not compatible to what we saw before and has dbar> dvalence at high-x (Because the CCe+ data don’t have so much relative weight) Moving from ZMVFN- GMVFN partly mitigates this –but much checking back to all types of jobs must be done and H1/ZEUS fitters must agree on the results for this type of job and its very slow Moving from QCDNUM16 to QCDNUM17 quadratic interpolation also mitigates this further (if combined with GMVFN) – but much checking of all types of jobs must be done and H1/ZEUS fitters must agree on the results for this type of job NOT QUICKLY DONE

Use of RTVFN in HERAPDF0.1 was compatible with the standard fit But for HERAPDFNEW it seems to be pushing us towards an alternative and nicer minimum than the one found in ZMVFN for Q20=1.9 EXTRAS