STAR Correlations and Fluctuations PWG

[Q Z <qinz18 AT outlook.com>]

Dear Nu,

Thanks for your nice comments, please find the updated version at this link:

https://drupal.star.bnl.gov/STAR/node/59019

We changed the abstract to focus on p-Xi results now.

For Slide 5:

(i) HAL QCD potential is used in the afterburner calculation with UrQMD, we have explicitly mentioned it in the poster now.

(ii) We have mentioned the difference of source between CATS(static) and UrQMD+CRAB(dynamic) in the poster now.

Thanks and Best regards,

Zhi

---

发件人: Nu Xu <nxu AT lbl.gov>
发送时间: 2022年4月2日 22:56
收件人: Q Z <qinz18 AT outlook.com>; STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
抄送: Nu Xu <nxu AT lbl.gov>
主题: Re: [Star-cf-l] STAR presentation by Zhi Qin for Quark Matter 2022 submitted for review

 

Hi Zhi and All,

Here are my comments on this poster:

0) Slide 2 - Motivation: (i) last bullet: I am not sure what do we what to say here, especially the claim of 'small system size’. How about something like: “The high baryon density medium is created in the 3GeV Au+Au collisions.  Precision measurements of correlation of hyperon and proton can be made from these data sets” ;
 
1) Slide 1: since the result of the p-Lambda correction function is not shown in the poster, should we change the abstract to focus on p-Xi results?

2) Slide 4: (i) title could be more precise: "Particle Identification, Purity and Background”; (ii) It is not clear what is plated in the right most plot. Add “Background from p_Xi- pairs” or something like that;

3) Slide 5: (i) Result part: It is not clear if the HAL QCD potential is used in the afterburner calculation with UrQMD. I think it is important here. (ii) I suggest add the result of the Gaussian equivalent radius from the UrQMD calculation; (iii) I am not sure we need the bullet starts with ‘CRAB tool provides …’ The important difference between CATS and UrQMD+CRAb is that in CATS a static Gaussian source is used while in UrQMD+CRAB approach, a hadronic transport dynamic model generated the space-momentum distributions. 

Summary part:
(i) I am not sure we can claim that “Make it possible to test …” I suggest remove this sentence;
(ii) replace ‘p-L correlation is ongoing’  by “The analysis of p-L correlation is ongoing”;
(iii) Last bullet: replace by something like “STAR has collected more than 2B events of Au+Au collisions at 3 GeV. Precision results of baryon correlation functions will be reported in the future"

4) Overall: I think the layout of all slides can be made better.

Thank you,

Nu


 


> On Apr 2, 2022, at 5:21 AM, Q Z via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>
> Dear Xiaofeng,
>
> Thank you very much for the comments and signing off.
> We update the slide on the same link
> https://drupal.star.bnl.gov/STAR/node/59019
>
>
> Best,
> Zhi
> 发件人: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> 代表 Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov>
> 发送时间: 2022年4月2日 10:59
> 收件人: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
> 主题: Re: [Star-cf-l] STAR presentation by Zhi Qin for Quark Matter 2022 submitted for review
> 
> Hi Zhi and Yingjie,
>
>     Nice poster, please find my minor comments below :
>     1. Slide 1, Please put ONLY ONE name there for the STAR collaboration.
>     2. Slide 2, In the 3rd bullet of the motivation : "An attractive
> p-Xi interaction is observed in p-Pb and pp collisions at ALICE "
>        Please change to "An attractive p-Xi interaction has been
> observed in Au+Au 200 GeV at STAR, p-Pb and pp collisions at ALICE "
>        Since previously, STAR has reported p-Xi results at 200 GeV and
> claim the observation of the attractive interaction in p and Xi.
>
>     With this implemented, I sign off.
>
> Thank you,
> Best Regards,
> Xiaofeng
>
> On 2022/3/28 4:23 PM, webmaster--- via Star-cf-l wrote:
> > Dear star-cf-l AT lists.bnl.gov members,
> >
> > Zhi Qin (qinz18 AT mails.tsinghua.edu.cn) has submitted a material for a review,
> > please have a look:
> > https://drupal.star.bnl.gov/STAR/node/59019
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
> > _______________________________________________
> > Star-cf-l mailing list
> > Star-cf-l AT lists.bnl.gov
> > https://lists.bnl.gov/mailman/listinfo/star-cf-l
>
> --
> Xiaofeng Luo
> Professor of Physics
> College of Physical Science and Technology
> Central China Normal University
> Luoyu Road 152, Wuhan China
> Office Phone #: +86-27-67867500
>
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