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star-hp-l - Re: [Star-hp-l] STAR presentation by Veronica Verkest for Rencontres de Moriond submitted for review

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Cc: webmaster AT star.bnl.gov
  • Subject: Re: [Star-hp-l] STAR presentation by Veronica Verkest for Rencontres de Moriond submitted for review
  • Date: Sun, 26 Mar 2023 22:03:32 +0530

Hello Veronica,

On my this comment,
Slide13:
I would not encourage you to show these D^0 jet results because Diptanil showed at last collaboration >meeting that our results have been changed due to some track selection cut.
I understand these are "STAR preliminary" but we now know that results have been changed.

I think we can still show these results outside though there is no significant change in physics message.
And we will discuss on this topic in future hp-pwg meeting once Diptanil updates us his detailed study in this direction.

Thank you
Nihar


On 2023-03-26 20:27, Nihar Sahoo via Star-hp-l wrote:
Hello Veronica

Thank you for this nice overview presentation.

Please find my comments below.

Slide2:
Please include the references for "Lifetime …" and "Temperature…";
It depends on different considerations so you need to cite the paper
where you picked these numbers.

What is "Slight color dipole"? "Slight"?
quarkonium state -> quarkonium states


Slide4:
"Time of flight" -> Time of flight measurement
(Because you have already used Time-of-flight at top)

"…below TPC pT acceptance" -> "…at low pT" (TPC acceptance can go to
low pT but detection not good)


Slide8
In this slide, you need to introduce what is "EA" and how do we
measure in STAR briefly.

within systematics -> within uncertainty

Slide10:
"Therefore, no CNM observed in J/ψ in small systems within systematics at
high-pT"
-> No CNM effect at high-pT [better with less words]
within systematics -> within uncertainty


SLide12:
"Energy loss at LHC is larger than at RHIC" How do you conclude this statement ?


Slide13:
I would not encourage you to show these D^0 jet results because
Diptanil showed at last collaboration meeting that our results have
been changed due to some track selection cut.
I understand these are "STAR preliminary" but we now know that results
have been changed.


SLide17:
"No significant CNM effects at low pT in J/ψ" -> Is not that "at high pT" ?
"Matched dijet asymmetry shows no angular dependence of jet energy
loss" -> This is not in general. It is only in the case of hard-core
jet selection. So please include this in this sentence

Upsilon RAA -> Upsilon R_{AA}


Cheers
Nihar





On 2023-03-23 07:03, webmaster--- via Star-hp-l wrote:
Dear Star-hp-l AT lists.bnl.gov members,

Veronica Verkest (vverkest AT gmail.com) has submitted a material for a review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/63056

Deadline: 2023-03-25
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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