The photon PDF determination within the xFitter framework

The photon PDF determination within the xFitter framework


University of Oxford
E-mail:
on behalf of the analysis team
Abstract

The xFitter project (former HERAFitter project) is an open-source package that provides a framework for the determination of the parton distribution functions (PDFs) of the proton for many different kinds of analyses in Quantum Chromodynamics (QCD). xFitter version 2.0.0 has recently been released, and offers an expanded set of tools and options. It incorporates experimental data from a wide range of experiments including fixed-target, Tevatron, HERA, and LHC. xFitter can analyze this data up to next-to-next-to-leading-order (NNLO) in perturbation theory with a variety of theoretical calculations including numerous methodological options for carrying out PDF fits and plotting tools which help visualise the results. In this contribution, a determination of the photon PDF from fits to recent ATLAS measurements of high-mass Drell-Yan dilepton production at = 8 TeV using this framework is presented.

\ShortTitle

The photon PDF deterination within the xFitter framework \FullConferenceEPS-HEP 2017, European Physical Society conference on High Energy Physics
5-12 July 2017
Venice, Italy

xFitter overview

The essential components that allow us to make theoretical predictions for experimental measurements of protons and hadrons are the Parton Distribution Functions (PDFs). The precision of the PDF analysis has advanced tremendously in recent years, and these studies are now performed with very high precision at NLO and NNLO in perturbation theory. The xFitter project [1] is an open source QCD fit framework that can generate PDF fits, compare existing PDF sets, assess the impact of new data and perform a variety of other tasks. The xFitter framework has already been used for more than 40 analyses including many LHC studies. xFitter is continually being updated, and version 2.0.0 (Frozen Frog) was released in March 2017 with many improvements and new features. Among them, it is important to stress that, for example, xFitter is able to read and write PDFs in the LHAPDF6 format. xFitter can also generate comparison plots of data versus theory, with a several options for the definition of the function and the treatment of experimental uncertainties. Within xFitter is also possible to study the impact of a particular data set or experiment on the PDFs. xFitter is able to perform PDF profiling and reweighting studies. Furhtermore, it is possible to perform PDF reweighting in xFitter; this method allows xFitter to update the probability distribution of a PDF uncertainty set (such as a set of NNPDF replicas) to reflect the influence of new data inputs. For the PDF profiling, xFitter compares data and MC predictions based on the minimization, and then constraints the individual PDF eigenvector sets taking into account the data uncertainties. Moreover, given the fact that many PDF analyses are now extended out to NNLO QCD (), the NLO QED effects () also become important; indeed, in xFitter, the DIS structure functions and PDF evolution (computed with the APFEL program [2]) are accurate up to NNLO in QCD and NLO in QED, including the relevant mixed QCD+QED corrections. More precisely, the and the corrections to the DGLAP splitting functions on top of the ones are available, as well as the corrections , and to functions.

Data, theory and fit inputs

In [3], the photon content of the proton, , is extracted from a PDF fit to the ATLAS measurements of high-mass Drell-Yan (DY) differential cross sections at TeV [4], combined with inclusive DIS cross-section data from HERA [1]. Information on the gluon and quark content of the proton is provided by the HERA inclusive data, while a direct sensitivity to the photon PDF is provided by the high-mass DY data. The ATLAS high-mass DY 8 TeV measurements are presented in terms of both the single-differential (1D) invariant-mass distribution, as well as double differential (2D) distributions. The NLO QCD and LO QED cross sections have been supplemented by bin-by-bin -factors in order to achieve NNLO QCD and NLO EW accuracy and they have been obtained from FEWZ [5]. They are defined as follows:

(1)

where the MMHT2014 NNLO [6] PDF set is used both in the numerator and in the denominator. The explicit form of PDF parametrisation at the starting scale is determined by the technique of saturation of the  [7] and it has been found that the optimal parametrisation for the gluon and quark PDFs is . For the photon PDF, the parametrisation has been used. PDF uncertainties are estimated using the Monte Carlo (MC) replica method [8, 9, 10], and it has been cross-checked that the Hessian method [11] provides consistent results.

Results

Figure 1: Left: Comparison between the photon at GeV from the present NNLO analysis (xFitter_epHMDY) with the corresponding results from NNPDF3.0QED, LUXqed and HKR16. Right: the same comparison, now with the results normalized to the central value of xFitter_epHMDY. For the present fit, the PDF uncertainties are shown at the 68% CL obtained from the MC method. For HKR16 only the central value is shown, while for LUXqed the associated PDF uncertainty band is included.

In the following, the results that will be shown correspond to those obtained from fitting the double-differential cross-section distributions. The value of has been obtained for the baseline NNLO fit where represnts the number of degrees of freedom. In Fig. 1, the photon PDF, , is shown at the evolved scale GeV, and it is compared to the predictions obtained using HKR16 [12], LUXqed [13, 14] and NNPDF3.0QED [15]. The xFitter_epHMDY fit is shown with the associated experimental PDF uncertainties at the 68% confidence level (CL), obtained using the MC replica method. For limited sensitivity to the photon PDF, the -range is set between 0.02 and 0.9 in Fig. 1. The four determinations of the photon PDF shown in Fig. 1 are consistent within PDF uncertainties for ; for smaller values, the baseline NNLO fit is in agreement at the 2- level with the LUXqed and HKR16 predictions. It has been shown in fig. 1 that for between and the present analysis exhibits smaller PDF uncertainties as compared to those predicted by NNPDF3.0QED.
In order to test the robustness of this photon PDF determination, a number of variations has been assessed. The determination is compared with further fits, where a number of new parameters are allowed in the PDF parametrisation. In each case, one variation at a time is performed and compared with the central value of and its experimental PDF uncertainties computed using the MC method. The result of these studies show that all the different variations are contained within the experimental PDF uncertainty bands. Then, the central fit prediction has been compared with the central value of those fits for which the theory input parameters (the input parametrisation scale , the strong coupling constant , the values of the and , the ratio of strange to non-strange light quark PDFs and the minimum cut on of data to be entered in the fit) have been varied. It has been found that the effect of the variations considered is contained within the experimental PDF uncertainty bands of the reference fit. Moreover, a comparison between the MC and Hessian methods is provided, in order to estimate the robustness of the estimated experimental uncertainty of in this analysis. Fig. 2(a) shows this comparison at the evolved scale of GeV and a reasonable agreement between the two methods has been indicated (it has been cross-checked that a similar results can be found at the lower scale GeV). As expected, the MC uncertainties are larger than the ones computed with the Hessian method, indicating deviations with respect to the Gaussian behaviour of the photon PDF. In the end, the perturbative stability of the xFitter_epHMDY photon PDF fit with respect to the inclusion of higher order QCD corrections has been quantified. A comparison between the baseline fit of , based on NNLO QCD and NLO QED theoretical calculations, with the central value resulting from a corresponding fit based instead on NLO QCD and QED theory has been made. A reasonable perturbative stability is exhibited by the xFitter_epHMDY photon PDF determination; indeed, the central value of the NLO fit is always contained in the 1- PDF uncertainty band of the baseline xFitter_epHMDY fit. The agreement between the two fits is particularly good for . Fig. 2(b) shows this comparison at the starting scale, GeV; a similar result has been found at the higher scale, GeV, indicating that perturbative stability is not scale dependent.

(a)
(b)
Figure 2: (a) Comparison between the xFitter_epHMDY determinations at GeV, obtained with the MC (baseline) and with the Hessian methods, where the PDFerror band shown corresponds to the 68% C.L. uncertainties in both cases; (b) Comparison between the reference xFitter_epHMDY fit of , based on NNLO QCD and NLO QED theoretical calculations, and the central value of the corresponding fit based on NLO QCD and QED theory, at GeV. In the former case, only the experimental MC PDF uncertainties are shown.

Acknowledgements

I would like to thank Voica Radescu and Ringaile Placakyte for their contribution to this work and for their dedication as conveners of the xFitter project from 2012 until May 2017.

References

  • [1] ZEUS, H1 Collaborations. Combination of measurements of inclusive deep inelastic scattering cross sections and QCD analysis of HERA data, Eur. Phys. J. C75 (2015) 580 [hep-ex/arXiv:1506.06042]
  • [2] Bertone, V. et al. APFEL: A PDF Evolution Library with QED corrections, Comput. Phys. Commun. 185 (2014) 1647 [hep-ph/arXiv:11310.1394]
  • [3] Giuli, F. et al. The photon PDF from high-mass Drell Yan data at the LHC, Eur. Phys. J. C77 (2017) 6 [hep-ph/arXiv:1701.08553]
  • [4] The ATLAS Collaboration. Measurement of the double-differential high-mass Drell-Yan cross section in pp collisions at TeV with the ATLAS detector, JHEP 08 (2016) 009 [hep-ex/arXiv:1606.01736]
  • [5] Gavin, R. et al. W Physics at the LHC with FEWZ 2.1, Comput.Phys.Commun. 184 (2013) 208 [hep-ph/arXiv:1201.5896]
  • [6] Harland-Lang, L. A. et al. Parton distributions in the LHC era: MMHT 2014 PDFs, Eur. Phys. J. C75 (2015) 204 [hep-ph/arXiv:1412.3989]
  • [7] Wilks, S. S. The Large-Sample Distribution of the Likelihood Ratio for Testing Composite Hypotheses, Annals Math. Statist. 9 (1938) 60
  • [8] NNPDF Collaboration. Unbiased determination of the proton structure function with faithful uncertainty estimation, JHEP 3 (2005) 080 [hep-ph/arXiv:0501067]
  • [9] NNPDF Collaboration. Neural network determination of parton distributions: The nonsinglet case, JHEP 3 (2007) 039 [hep-ph/arXiv:0701127]
  • [10] NNPDF Collaboration. A determination of parton distributions with faithful uncertainty estimation, Nucl. Phys. B809 (2009) 1-63 [hep-ph/arXiv:0808.1231]
  • [11] Pumplin, J. et al. Uncertainties of predictions from parton distribution functions. 2. The Hessian method, Phys. Rev. D65 (2001) 014013 [hep-ph/arXiv:0101032]
  • [12] Harland-Lang, L. A. et al. Photon-initiated processes at high mass, Phys. Rev. D94 (2016) 074008 [hep-ph/arXiv:1607.04635]
  • [13] Manohar, Aneesh et al. How bright is the proton? A precise determination of the photon parton distribution function, Phys. Rev. Lett. 117 (2016) 242002 [hep-ph/arXiv:1607.04266]
  • [14] Manohar, Aneesh et al. The photon content of the proton, (2017) [hep-ph/arXiv:1708.0125]
  • [15] NNPDF Collaboration. Parton distributions with QED corrections, Nucl. Phys. B877 (2023) 290-320 [hep-ph/arXiv:1308.0598]
Comments 0
Request Comment
You are adding the first comment!
How to quickly get a good reply:
  • Give credit where it’s due by listing out the positive aspects of a paper before getting into which changes should be made.
  • Be specific in your critique, and provide supporting evidence with appropriate references to substantiate general statements.
  • Your comment should inspire ideas to flow and help the author improves the paper.

The better we are at sharing our knowledge with each other, the faster we move forward.
""
The feedback must be of minimum 40 characters and the title a minimum of 5 characters
   
Add comment
Cancel
Loading ...
186192
This is a comment super asjknd jkasnjk adsnkj
Upvote
Downvote
""
The feedback must be of minumum 40 characters
The feedback must be of minumum 40 characters
Submit
Cancel

You are asking your first question!
How to quickly get a good answer:
  • Keep your question short and to the point
  • Check for grammar or spelling errors.
  • Phrase it like a question
Test
Test description