STAR Flow, Chirality and Vorticity PWG

["Md. Nasim" <mnasim2008 AT gmail.com>]

Hi Shuai,

                 For my highlight talks, I need an NCQ scaling plot using all particles pi,k,p, and strange hadrons at 14.6 GeV.

Could you please provide me with such a plot?

On Wed, Nov 23, 2022 at 6:32 PM zs155167 via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

 

 Dear Subhash,

 Thanks for your comments and suggestion. Here are my illustrations:

For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a comparison
with BES-I that we can take a look?

 Yes, please find my slide here: https://drupal.star.bnl.gov/STAR/system/files/v2ratio.pdf

I see, you have presented individual pi, K, p v2 at FCV, but I feel that
the NCQ scaling results especially on slide 12 and 13 are new. Could you
discuss it today at the FCV?

 

OK, I will illustrate it today at the FCV

Do you observe any centrality dependence in NCQ scaling behavior?

Within errors, no obvious centrality dependence is observed.

Is it possible to make a single NCQ scaling plot, including all
particles measured. I mean pi, K, p (from you) and multi-stranges from
Prabhupada.

  OK, I will contact Prabhupada about this.

 There was some discussions at the FCV related to the asymmetric

mass-square selection. Could you indicate if you have done any check?

 

Yes, I have checkd it, please find: https://drupal.star.bnl.gov/STAR/system/files/star_prelimilary_update.pdf

Please include, collision system, energy, TPC+iTPC etc within the figure
where these informations are missing; Add X and Y-axis labels etc.

s4: last bullet: identification using m2

s6: For resolution plot, it would be good to comparison with BES-I

s10, 11: Could you increase legends size

Yes, I will improve it

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

From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;

Date:  Wed, Nov 23, 2022 05:43 PM

To:  "周帅"<zs155167 AT mails.ccnu.edu.cn>; "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;

Subject:  Re: [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD 2022 submitted for review

 

Dear Shuai,

Thanks for reminder. I have a few comments and suggestions.

General:
For the new BES-II 14.6 GeV pi, K, p v2 data, do you have a comparison
with BES-I that we can take a look?

I see, you have presented individual pi, K, p v2 at FCV, but I feel that
the NCQ scaling results especially on slide 12 and 13 are new. Could you
discuss it today at the FCV?

Do you observe any centrality dependence in NCQ scaling behavior?

Is it possible to make a single NCQ scaling plot, including all
particles measured. I mean pi, K, p (from you) and multi-stranges from
Prabhupada.

There was some discussions at the FCV related to the asymmetric
mass-square selection. Could you indicate if you have done any check?

Please include, collision system, energy, TPC+iTPC etc within the figure
where these informations are missing; Add X and Y-axis labels etc.

s4: last bullet: identification using m2

s6: For resolution plot, it would be good to comparison with BES-I

s10, 11: Could you increase legends size

Thanks and regards,
Subhash


On 2022-11-23 02:11 PM, zs155167 via Star-fcv-l wrote:
> Dear convenors,
>
>  I have submitted my slides for CPOD 2022. If you have any suggestion
> or comments, please let me know. Thank you!
>
> Best regards,
> Shuai Zhou
>
> ------------------ Original ------------------
>
> From:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
> Date:  Mon, Nov 21, 2022 04:18 PM
> To:  "STAR Flow,Chirality and"<star-fcv-l AT lists.bnl.gov>;
>
> Subject:  [Star-fcv-l] STAR presentation by Shuai Zhou for CPOD 2022
> submitted for review
>
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Shuai Zhou (zs155167 AT mails.ccnu.edu.cn) has submitted a material for a
>
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/61798
>
> Deadline: 2022-11-28
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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--

Thanks,

With Best Regards,

Nasim