STAR Flow, Chirality and Vorticity PWG

[胡晨露 <huchenlu AT impcas.ac.cn>]

Dear Jiangyong,

Thank you for your comments.

For slide 13 middle panel, By definition, v1 has to go through zero, so we used a f(x)=kx function to fit the data. For H3L(2-body), we doesn't see a significant linear trend in its distribution, which is due to its low statistics. The v1 slope for H3L is mainly constrained by H3L(3-body) points, still fitted results of 2-body and 3-body are consistent with their statistical error.

For the nucleon number scaling, it is shown in slide 15, like the cases for light nuclei, hyper-nuclei v1 follows the mass number scaling within uncertainties.

I updated the slides and you can check the file through the link below：

https://drupal.star.bnl.gov/STAR/presentations/sqm-2021/light-hyper-nuclei-production-3-gev-auau-collisions-rhic

If you have further comments or suggestions, please let me know.

Best regards,

Chenlu

-----原始邮件-----
发件人:"Jiangyong Jia via Star-fcv-l" <star-fcv-l AT lists.bnl.gov>
发送时间:2021-05-10 21:35:23 (星期一)
收件人: star-fcv-l AT lists.bnl.gov
抄送:
主题: Re: [Star-fcv-l] STAR presentation by Shaowei Lan for SQM 2021 submitted for review

Hi, Chenlu,

Thank you for the very clear set of slides. Just a few comments

For all your physics plot, could you add STAR preliminary in the ROOT macro, not add inside the Power Point.

slide 13 middle panel v1 does not show a linear trend. A natural question would be how you justify fitting a v1 slope and then apply nucleon number scaling.

Cheers,

Jiangyong

On 5/7/21 9:49 PM, 胡晨露 via Star-fcv-l wrote:

Dear Rongrong,

I'm really sorry that I uploaded the file to the wrong place before, so you can't read the file.

Shaowei helped me upload it to the right place. You can check the file through the link below：

https://drupal.star.bnl.gov/STAR/node/54864

I will send an email to the LFSUPC mailing list to get comments from them as well.

Thank you very much!

Best regards,

Chenlu

-----原始邮件-----
发件人:"Rongrong Ma via Star-fcv-l" <star-fcv-l AT lists.bnl.gov>
发送时间:2021-05-08 06:19:56 (星期六)
收件人: "Shaowei Lan" <shaoweilan AT mails.ccnu.edu.cn>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
抄送:
主题: Re: [Star-fcv-l] STAR presentation by Shaowei Lan for SQM 2021 submitted for review

Hello Chenlu (Shaowei)

The posted PDF version of the talk is unreadable. Please double check and update a new version. 

Since this talk is relevant for both LFSUPC and CFV PWGs, please send an email to the LFSUPC mailing list to get comments from them as well. Thanks!

Best

Rongrong

On May 6, 2021, at 3:49 PM, Shaowei Lan via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear All,

There are some problems with Chenlu's account.

I create this content for her.

Please feel free to send comments and suggestions to her.

Thanks,

Shaowei

 

 

------------------ Original ------------------

From:  "webmaster--- via Star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Date:  Thu, May 6, 2021 12:44 PM

To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;

Subject:  [Star-fcv-l] STAR presentation by Shaowei Lan for SQM 2021 submitted for review

 

Dear star-fcv-l AT lists.bnl.gov members,

Shaowei Lan (shaoweilan AT mails.ccnu.edu.cn) has submitted a material for a 
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/54864

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