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star-hp-l - Re: [Star-hp-l] STAR presentation by Veronica Verkest for DNP 2022 submitted for review

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: webmaster AT star.bnl.gov, STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] STAR presentation by Veronica Verkest for DNP 2022 submitted for review
  • Date: Sun, 16 Oct 2022 17:57:21 +0530

Hello Veronica,

Please find my comments on your nice presentation slides.
With these implemented, I sign off.

Slide2:
"thought too small to form QGP" -> "thought too small in size to form QGP"
It would be good if you could define EA and UE (or give reference).

Slide3:
"Solenoidal Tracker At RHIC:…" -> Can you bring that to the top of the STAR detector pic?

Slide4: "iBBCEsum " -> is this "inner east beam-beam counter signal sum" ? Then introduce there first.
Slide6: ET -> Transversr energy (E_T)

SLide10:
"Consistent with QCD predictions and jet mass measured in p+p [Phys. Rev. D 104, 052007 ]
Not sure how do we draw this conclusion.
1_ We have not compared any QCD calculation here for p+A collisions.
2_ Above p+p results are between jet pT 20-25, 30-40 GeV/c, Not the same kinematic range.
And there is also no comparison plot between pp and pA jet mass.
If you have such comparison plot, please include that.
Otherwise, I would suggest just drop the above statement " Consistent with ….".


Cheers
Nihar


On 2022-10-14 03:24, 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/61322

Deadline: 2022-10-27
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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