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star-hp-l - Re: [Star-hp-l] STAR presentation by Sooraj Radhakrishnan for AUM 2022 submitted for review

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Subject: STAR HardProbes PWG

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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: Sooraj Radhakrishnan <skradhakrishnan AT lbl.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 Sooraj Radhakrishnan for AUM 2022 submitted for review
  • Date: Fri, 03 Jun 2022 16:59:58 +0530

Hello Sooraj,

Please find below a few comments on your nice overview slides.

Slide#2
_ "microscopic mechanism jet suppression in QGP" -> not clear what is microscopic mechanism? please rephrase it.
_ "Jet substructure dependence of suppression " -> "Modification of jet substructure"

Slide#10:
You could also mention in Isobar analysis "high pT charged particles with pT > 5.1"


slide#11:
_I think this IAA plot is good to show.
_But, main result in this analysis is "medium-induced Intra-jet Broadening"
And this is our first clear observation in STAR (Please highlight this result).
You could consider to add that Ratio plot in another slide or merge these two results in one slide.
And please mention in your summary slide#19.
Please have a look at slide#17.
Derek's QM2022 talk:https://indico.cern.ch/event/895086/contributions/4717079/attachments/2421604/4145053/AndersonTalk_QM2022.v11_manualAnimations.pdf

Slide#12:
In Title, please remove "intrajet broadening and Acoplanarity" -> "Medium-induced jet Acoplanarity"
Because Intrajet broadening and acoplanarity are two physics and you are showing latter.

Slide#13:
_ "Study HF jets to better understand the mechanism of redistribution" ->
"Study HF mesons in jets are sensitive to the production mechanism of mesons, energy loss and diffusion of heavy flavor quarks in QGP."
_ "D0 jets " —> please use either "D0 within jet" or "D0+jet"
_ "higher statistics p+p dataset in 2024 " I would not mention this because we don't have HFT for future runs.
_ You can mention that we are working on to lower the D0 pT range.

Before summary slide:
You could show the STAR HardProbe program's past, current, and future kinematic coverage:
https://drupal.star.bnl.gov/STAR/system/files/STARLHCHardProbes_v5.png


Thank you
Nihar




On 2022-06-02 23:51, Sooraj Radhakrishnan via Star-hp-l wrote:
Dear All,
I was invited to give a talk on 'The STAR Results and Perspective'
at the HF+Jet session for the RHIC AGS AUM. Sorry for the late
submission. Please let me know if you have any comments or suggestions

thanks
Sooraj

On Thu, Jun 2, 2022 at 11:47 PM webmaster--- via Star-hp-l
<star-hp-l AT lists.bnl.gov> wrote:

Dear Star-hp-l AT lists.bnl.gov members,

Sooraj Radhakrishnan (skradhakrishnan AT lbl.gov) has submitted a
material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/59836

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

Sooraj Radhakrishnan

Research Scientist,
Department of Physics

Kent State University
Kent, OH 44243

Physicist Postdoctoral AffiliateNuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road
Berkeley, CA 94720
Ph: 510-495-2473 [1]

Email: skradhakrishnan AT lbl.gov


Links:
------
[1] tel:%28510%29%20495-2473
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