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Add ATLASZPT8TEV{M,Y}DIST datasets #61
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- just for the time being to avoid LHAPDF bug
- grid compression is done at the very end of `run.sh`
In NNPDF there's a cut on the jet transverse momentum of 5 GeV, which shouldn't be there. I expect this to make a large difference for |
There might be a comment about this point in this paper |
Here the comparison against the NLO QCD APPLgrids with NNPDF31_nlo_as_0118, showing differences in per mille, negative numbers correspond to a larger APPLgrid result: MDIST:
YDIST:
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@enocera I'd say for |
@enocera Thanks to Marco and Maria we've very likely found the source of disagreement. Maria was able to find the MCFM runcards, in which the scale is set to
If you read the MCFM documentation (p. 20, table 11) it says that
which I (and also Alberto, who generated the grids) read as being the invariant mass of particles 3 and 4. However, Marco explicitly verified that it's actually the on-shell Z mass 😩. |
@cschwan Thanks for investigating this issue! |
@enocera @marcozaro What I said above isn't the explanation (Alberto manually fixed the scale problem in MCFM), as the numbers are clearly worse:
I'll keep investigating this problem. |
Here the differences from #61 (comment) again, split up into the invariant mass slices:
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Note to myself: compare the numbers at LO! |
@enocera I'm finally certain to have a found a proper difference between the APPLgrid and our PineAPPL grid. Starting from PineAPPL v0.5.0 you can print out the factorization and renormalization grid values that each subgrid uses to interpolate the PDFs, and for our runcards I find results what I'd expect, given that we set
where
which means the scale choice is bounded by
Because of the interpolation not only the grid points in the interval For APPLgrid the used grid points are:
These points are much higher and don't overlap with our points, so my conclusion is that also the chosen scale must be larger than the one chosen for our runcards. |
Thanks @cschwan . Looking at Eq.(3.2) of arXiv:1705.00343, I understand that they use pTZ, where the values of ptZ (look at Fig.1) seem compatible to the larger values of the grid points that you find, would you agree? |
Fig. 1 should correspond to the rapidity distribution (YLL) and Fig. 2 should match the invariant-mass distribution (MLL). In Fig. 2 the ptZ values correspond to the ones that we call |
Sorry @cschwan I take it back. I did the algebra and I agree with your conclusion. Unfortunately, I'd say there's no way to know which values have been used, as we don't have the runcards. |
@enocera shouldn't the runcards be in our external repository, for instance for the first slice here: https://github.com/NNPDF/external/blob/4e842676deada26d882e1932a5ffd53d4b87709e/MCFM-6.8/Bin/Input/ATLASZPT8TEVMDIST-BIN1.DAT? |
Thanks Christopher,
these discrepancies are indeed puzzling, something strange should have ended up into the ApplGrids.
I don’t know, we may consider the issue solved, but it would be interesting to understand how they got those strange numbers (there are infinite ways one can screw up a scale, and we would need the code to see what was done)…
Let me know if you have any idea
cheers,
Marco
… On 23 Feb 2022, at 14:20, Christopher Schwan ***@***.***> wrote:
Fig. 1 should correspond to the rapidity distribution (YLL) and Fig. 2 should match the invariant-mass distribution (MLL). In Fig. 2 the ptZ values correspond to the ones that we call ptll. Nevertheless I find for the first bin mu < 59 GeV, but the first grid point in the APPLgrid is much higher, mu = 81 GeV.
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Do you trust them? I don't. Are you sure that the applgrids have been produced with these runcards? I'm not. Are you sure that this line https://github.com/NNPDF/external/blob/4e842676deada26d882e1932a5ffd53d4b87709e/MCFM-6.8/Bin/Input/ATLASZPT8TEVMDIST-BIN1.DAT#L25 is equivalent to choosing sqrt(mll^2+ptll^2)? I'm not. |
And isn't this the ambiguity? |
Hi,
as far as I can remember Maria also wrote that Guffanti changed this behaviour in order to match what they write in the paper
Marco
… On 23 Feb 2022, at 16:29, Emanuele R. Nocera ***@***.***> wrote:
@enocera <https://github.com/enocera> Thanks to Marco and Maria we've very likely found the source of disagreement. Maria was able to find the MCFM runcards, in which the scale is set to
sqrt(M^2+pt34^2)
If you read the MCFM documentation <https://mcfm.fnal.gov/manual.pdf> (p. 20, table 11) it says that
M = mass of particle 3+4
which I (and also Alberto, who generated the grids) read as being the invariant mass of particles 3 and 4. However, Marco explicitly verified that it's actually the on-shell Z mass weary.
And isn't this the ambiguity?
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If I did my checks in the past properly, then according to #61 (comment) this shouldn't be able to explain the difference. But obviously the scale is different, so maybe I missed something. I've asked Maria to send me the corresponding emails again, as I've lost my INFN account; then I should be able to redo the check I did in the past. |
OK, sorry, I should have read the discussion more carefully. |
Maria sent me her runcards and they are exactly the ones in the repository. I still have to check the scale setting procedure. |
This branch adds the ATLASZPT8TEV datasets from arXiv:1512.02192, with datasets available at https://www.hepdata.net/record/ins1408516. The runcards were copied from the CMS_Z_13TEV dataset and adjusted.
Issues: