STAR HardProbes PWG

[wy157543 AT mail.ustc.edu.cn]

Hi, Nihar

Thank you for your nice comments. New version can be found in this link: 
https://drupal.star.bnl.gov/STAR/system/files/HP_v4_0.pdf
"Red vertical upward arrow" mean debey radius reduce with temperature 
increase.
Isobar RAA at 60-80% close to 1.so we think no significant suppression and pT 
depedence is observed.

best,
Yan

> -----原始邮件-----
> 发件人: "Nihar Sahoo" <nihar AT rcf.rhic.bnl.gov>
> 发送时间: 2023-03-18 17:25:12 (星期六)
> 收件人: wy157543 AT mail.ustc.edu.cn, "STAR HardProbes PWG" 
> <star-hp-l AT lists.bnl.gov>
> 抄送: webmaster AT star.bnl.gov
> 主题: Re: [Star-hp-l] STAR presentation by Yan Wang for Hard Probes 2023 got 
> commented by Xin Dong
> 
> Hello Yan,
> 
> Thank you for your nice comments.
> Please find my comments below.
> 
> Slide-3:
> "Jet quenching" -> Since you are discussing on J/psi so jet quenching 
> may not relevant. You could mention "J/psi suppression"
> 
> In the top cartoon, what does "Red vertical upward arrow" represent 
> there along with "T"?
> 
> Slide-4
> "All these effects are expected to strongly depend on collision system 
> size " -> "All these effects are expected to show strong dependence on 
> collision system size"
> 
> Slide-6:
> Please increase the X,Y-axis title size.
> 
> SLide-8:
> Sorry, I have not followed this before.
> Could you inform me what does "Isobar, 60-80%" represent in RAA plot?
> 
> 
> Slide-14:
> "Indicate that the color-screening effect is dominant in isobaric 
> collisions"
> I think you could add this "color-screening effect" in one of Silde8,9;
> Although you have mentioned suppression but if you could add 
> "Significant suppression observed at large Npart due to color-screening 
> effect" (in SLide9) then it would be good to say at the end.
> 
> 
> Cheers
> Nihar
> 
> 
> 
> 
> 
> 
> On 2023-03-17 08:17, wy157543--- via Star-hp-l wrote:
> > Hi Xin Dong,
> > 
> >   Thanks for your comments, I will update the figure later.
> > I am sorry for the link issue, the slide can be found in this link:
> > https://drupal.star.bnl.gov/STAR/system/files/HP_v2_2.pdf
> > 
> > best,
> > Yan
> > 
> > 
> > 
> >> -----原始邮件-----
> >> 发件人: "webmaster--- via Star-hp-l" <star-hp-l AT lists.bnl.gov>
> >> 发送时间: 2023-03-17 05:31:13 (星期五)
> >> 收件人: Star-hp-l AT lists.bnl.gov
> >> 抄送:
> >> 主题: [Star-hp-l] STAR presentation by Yan Wang for Hard Probes 2023 got 
> >> commented by Xin Dong
> >> 
> >> Dear Star-hp-l AT lists.bnl.gov members,
> >> 
> >> Xin Dong ( xdong AT lbl.gov ) has commented on a material originally 
> >> submitted
> >> by Yan Wang ( wy157543 AT mail.ustc.edu.cn ) at
> >> https://drupal.star.bnl.gov/STAR/presentations/Hard-Probes-2023/Jpsi-production-RuRu-and-ZrZr-collisions-200GeV-STAR-experiment
> >> 
> >> Comment:
> >> Hi Yan, it looks like the link below doesn't work. But I managed to 
> >> access it
> >> by changing the filename to "HP_v2_0.pdf" (believe it is the current 
> >> draft).
> >> I have one suggestion to your nice result in slide 13. I think it 
> >> would be
> >> better to add the D0 v2 data points together to better illustrate the
> >> conclusion you have on the slide "limited regeneration". Thanks /xin
> >> 
> >> ---
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