STAR Flow, Chirality and Vorticity PWG

["Zuowen Liu" <liuzw AT mails.ccnu.edu.cn>]

Dear Subhash,

Thanks a lot for your suggestions.

It's good to add "nature" to avoid misunderstanding.

I have modified the poster.

Thanks and Best regards,

Zuowen

 

 

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

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

Date:  Fri, Jun 10, 2022 08:32 AM

To:  "Zuowen Liu"<liuzw AT mails.ccnu.edu.cn>;

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

Subject:  Re: [Star-fcv-l] STAR presentation by Zuowen Liu for SQM 2022 submitted for review

 

Dear Zuowen,

Thanks for considering my suggestions. I am fine with your poster and
sending it to star-talks with a few additional comments:

abstract
"...important insights on the nature of QCD phase transition."
slide#2: sensitive to nature of QCD phase transition.
I suggested this because there are models with cross-over transition
also produce a sign change.
slide#4: Top panels: Indicate uncertainties are statistical.

Thanks and regards,
Subhash

On 2022-06-08 09:42 AM, Zuowen Liu wrote:
> Dear Subhash,
>
> Thank you very much for your nice suggestions.
>
> I have removed results from 14.6 GeV.
> And other suggestions have been taken and implemented to the slides.
>
> Kindly find the modified slides by the link below:
> https://drupal.star.bnl.gov/STAR/node/59770
>
> Best regards,
> Zuowen
>
> ------------------ Original ------------------
>
> From:  "subhash"<subhash AT rcf.rhic.bnl.gov>;
> Date:  Tue, Jun 7, 2022 06:47 PM
> To:  "star-fcv-l"<star-fcv-l AT lists.bnl.gov>;
> Cc:  "liuzw"<liuzw AT mails.ccnu.edu.cn>;
> Subject:  Re: [Star-fcv-l] STAR presentation by Zuowen Liu for SQM
> 2022 submitted for review
>
> Dear Zuowen,
>
> Nice poster.
> As decided by the management, we will only release 0-80% centrality
> for
> 14.6 GeV. So please remove results of v1 figures for 14.6 GeV at
> 10-40%
> centrality (slide 4 and 5).
>
> slide#2: "v1 is sensitive to the 1st order phase transition." --> v1
> is
> sensitive to the QCD order phase transition. Because depending on
> cross-ver or 1st order PT the v1 can be different.
> Can you add a reference for data and model here?
>
> slide#3: Inside figure indicate run year or BES-II.
> Can you indicate the improved 1st order EP resolution in BES-II
> compared
> to BES-I?
>
> slide#5: Modify the summary accordingly, since 14.6 GeV is removed.
>
> Thanks and regards,
> Subhash
>
> On 2022-05-30 07:57 PM, webmaster--- via Star-fcv-l wrote:
>> Dear star-fcv-l AT lists.bnl.gov members,
>>
>> Zuowen Liu (liuzw AT mails.ccnu.edu.cn) has submitted a material for a
>> review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/59770
>>
>> ---
>> If you have any problems with the review process, please contact
>> webmaster AT www.star.bnl.gov
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