STAR HardProbes PWG

["Mooney, Isaac" <isaac.mooney AT yale.edu>]

Thanks for implementing the comments, Monika. I sign off as well.

-Isaac

On Nov 21, 2024, at 08:09, Nihar Sahoo <nihar AT rcf.rhic.bnl.gov> wrote:

Hi Monika,

Thank you for your nice slides. I don't have any comments. I sign off.

Best
Nihar

On 2024-11-21 18:23, Robotkova, Monika wrote:

Hi Isaac,
Thank you for your useful comments, I've implemented them and
uploaded new version on Drupal.
Best regards,
Monika
-------------------------
Od: star-hp-l-request AT lists.bnl.gov <star-hp-l-request AT lists.bnl.gov>
za uživatele Mooney, Isaac <isaac.mooney AT yale.edu>
Odesláno: středa 20. listopadu 2024 22:41
Komu: star-hp-l AT lists.bnl.gov <star-hp-l AT lists.bnl.gov>
Předmět: Re: [[Star-hp-l] ] STAR presentation by Monika Robotkova
for Zimanyi School 2024 submitted for review
Hi Monika,
I have a few comments on your well-written slides, below.
Thanks,
Isaac
11. Later in passing you mention the motivation for Collinear Drop (s.
15), but since you give the physics motivation for Soft Drop on this
slide, it would also be good to mention the motivation for Collinear
Drop.
14. It would be good to specify the directionality in the second
bullet -- so, "we move from non-perturbative to perturbative region by
increasing Rg" or similar.
17. Rather than the transition region shifting with momentum, I would
emphasize the universality of the transition region when scaled by
momentum. This contains the information in your current second bullet
and adds additional information as well.
19.
       You mention that the data are captured by MC models and
theoretical predictions, but we've seen for the EEC and similarly for
rc, that models aren't simultaneously able to describe the
distribution of charge information within the jets. I think this is
nice to point out since it shows that pp is not a solved problem --
there is still interesting work to be done. It wouldn't need to have
its own slide, but maybe a bullet point on s. 17 with a citation, and
mentioned again on this slide.
       For the outlook to A+A collisions, this makes it seem as if no
substructure measurements have been done in A+A collisions at STAR
yet, but e.g. the generalized angularities have a preliminary
measurement. Of course, you don't need to include every STAR result in
your talk, but would be good to make it clear that some work has been
done already on this.

On Nov 19, 2024, at 17:12, webmaster AT star.bnl.gov wrote:
Dear Star-hp-l AT lists.bnl.gov members,
Monika Robotkova (robotmon AT fjfi.cvut.cz) has submitted a material

for a

review, please have a look:
https://nam12.safelinks.protection.outlook.com/?url="https%3A%2F%2Fdrupal.star.bnl.gov%2FSTAR%2Fnode%2F69940&data=05%7C02%7Cisaac.mooney%40yale.edu%7C4653c8b966aa435fdc0f08dd0a306977%7Cdd8cbebb21394df8b4114e3e87abeb5c%7C0%7C0%7C638677925245716044%7CUnknown%7CTWFpbGZsb3d8eyJFbXB0eU1hcGkiOnRydWUsIlYiOiIwLjAuMDAwMCIsIlAiOiJXaW4zMiIsIkFOIjoiTWFpbCIsIldUIjoyfQ%3D%3D%7C0%7C%7C%7C&sdata=EjYioL%2FTLoJmEAyTEalG3CA9txWWZDxTsPqiUskNBhY%3D&reserved=0
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