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1 theory database out of which a single record is selected for a fit
the record contains tentatively all information needed for evolution and DIS
(this is of course mainly due to historic reasons)
Problems
FNS actually should only matter for cross sections, but instead is also (ab-)used for evolution
FONLL is not involved in evolution and its threshold does not play any role in evolution
instead a dedicated threshold for cross section is needed, that can be chosen freely and independent of evolution thresholds
some of the settings are redundant: M_Z, M_W, sin(theta_w), G_F, alphaqed are not linearly independent
in principle the card could be divided into two parts (evolution <-> cross sections) with some few settings shared
Configurations ("o-cards")
both eko and yadism will be shipped default-less (in big contrast to APFEL)
both eko and yadism require some additional configurations:
in eko "operators": the target scale of the operators, the discretization and some numerical details
in yadism "observables": the discretization, DIS configurations (currents, hadron, lepton) and the target functions, e.g. F2total(x=0.1, Q2=90)
we require a mapping of the old settings to the new settings (which both programs already use at this point)
our current implementation of this remapping is given here
the current status of eko already ignores the FNS setting, but instead it has to be fed with the correct kcThr
yadism has to be fed with the correct kDIScThr (the name can of course be changed to kxscThr or similar) to determine the thresholds and FNS to determine the (re-)combination of heavy/light coefficient functions
in order to implement FONLL correctly (to our understanding) we need to deactivate the charm threshold in eko, but not in yadism
Proposed Workflow
pineko should determine a consistent configuration for both eko and yadism
ask them each in turn to compute their ingredients
join their respective outcome to provide what is needed: a mapping f_j(x,Q_0) -> theory prediction
Questions
how are the "observables" currently determined?
how can we organize and maintain the configurations?
how can we ensure the consistency between (experimental) dataset and theory?
Current status
Problems
FNSactually should only matter for cross sections, but instead is also (ab-)used for evolutionFONLLis not involved in evolution and its threshold does not play any role in evolutionM_Z, M_W, sin(theta_w), G_F, alphaqedare not linearly independentConfigurations ("o-cards")
ekoandyadismwill be shipped default-less (in big contrast toAPFEL)ekoandyadismrequire some additional configurations:eko"operators": the target scale of the operators, the discretization and some numerical detailsyadism"observables": the discretization, DIS configurations (currents, hadron, lepton) and the target functions, e.g.F2total(x=0.1, Q2=90)ekoalready ignores theFNSsetting, but instead it has to be fed with the correctkcThryadismhas to be fed with the correctkDIScThr(the name can of course be changed tokxscThror similar) to determine the thresholds andFNSto determine the (re-)combination of heavy/light coefficient functionseko, but not inyadismProposed Workflow
pinekoshould determine a consistent configuration for bothekoandyadismf_j(x,Q_0) -> theory predictionQuestions