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  • From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
  • To: STAR HardProbes PWG <star-hp-l AT lists.bnl.gov>
  • Subject: Re: [Star-hp-l] My CFNS-npQCD talk
  • Date: Wed, 25 Oct 2023 12:13:39 +0530

Hello Rongrong,

Thank you for sharing your nice presentation slides on heavy-flavor.
Overall your slides look nice and capture all physics measurements of STAR.

Here are my additions comments for your consideration.

Slide5:
- "Charm quark gain v2 at T close to Tc" -> what is "Tc" here ? And What is the value of Tc? Why it is important?

Slide7:
- "About a factor of 2 suppression…" -> Not clear, with respect to what

Slide9:
- Do you need to refer "QM2023" for this D^0+jet results? Same for next slide

SLide13:
- Better to motivate this result with QGP effect can smear D^0-D^0bar correlation. But uncertainty limits to pin down

Slide14:
- "Coalescence is important" -> Do we need to mention also "at low pT"?

After Slide16, It would be good to summarize the key physics that we observed from open heavy flavor measurements at STAR. Otherwise people may be lost.

Slide18:
-"Hint of rising trend toward low energy" -> Is that correct to comment within these uncertainties?
_ You could hint to the "primodial" and "Regeneration" effects at high and low energies.

Slide19:
-Could you comment on QGP thermal temp based on sequential suppression of quarkonia? That is important take away from these results at RHIC.

SLide20-22:
Physics motivation is missed here. Better to say a few words.
Slide21-23: better to motivate with other pesudoscalar meson results from FCV.

After Slide23: You could summarize the key physics learnt from QGP point of view.
And then you can go to UPC J/psi results discussion to study other Physics not related to QGP.


Best
Nihar


On 2023-10-24 20:33, Ma, Rongrong via Star-hp-l wrote:
Dear All

I was invited by the CFNS-npQCD workshop
(https://indico.cfnssbu.physics.sunysb.edu/event/110/) organizers to
present an overview of the STAR heavy flavor results. Even though it
is not a STAR talk, I will exclusively present STAR results. So I
would like to seek your comments and suggestions on my talk, a first
draft of which can be found here:
https://drupal.star.bnl.gov/STAR/system/files/RMa_CFNS_npQCD_v1.pdf.

Your feedback is more than welcome. Thanks.

Best
Rongrong
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