STAR Correlations and Fluctuations PWG

["ChuanFu" <fuchuan AT mails.ccnu.edu.cn>]

Dear Xiaofeng,

                  Thank you very much for your nice comments.

Please find the revised slides and replies below: 

https://drupal.star.bnl.gov/STAR/node/60372

1. Please add PID plots and PID cuts in your presentation.
------ Added.

     2. In slide 5, why k* is written as q_inv ? I think if k* is
usually used, to avoid confusion, we should directly use k* instead of
using
         q_inv. because by convention, the k* and q_inv have different
_expression_.
------ All q_inv were replaced by k*.

     3. Slide 8, should mention, those are "proton" phase space.
------ Mentioned in title.

     4. Slide 11, you may add some references about this study.

------ Added.

     5. Slide 18, Based on crab and In the legend of plots, You already
obtain some source size information at 3 GeV and 7.7 GeV.
                        You may want to mention those in your slides and
what we can learn from the extracted source size information.

------ I removed the CRAB fitting since we don't know how to constrain the ratio of Rx(Ry) to Rz.

I only show the STAR measurements from 3 GeV and 7.7 GeV.

Best regards,

Chuan

 

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

From:  "Star-cf"<star-cf-l AT lists.bnl.gov>;

Date:  Sun, Jul 24, 2022 08:15 PM

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

Subject:  Re: [Star-cf-l] STAR presentation by Chuan Fu for ISMD2022 submitted for review

 

Hi Chuan,

     Nice presentation.
     Please find my suggestions below :

     1. Please add PID plots and PID cuts in your presentation.

     2. In slide 5, why k* is written as q_inv ? I think if k* is
usually used, to avoid confusion, we should directly use k* instead of
using
         q_inv. because by convention, the k* and q_inv have different
_expression_.

     3. Slide 8, should mention, those are "proton" phase space.

     4. Slide 11, you may add some references about this study.

     5. Slide 18, Based on crab and In the legend of plots, You already
obtain some source size information at 3 GeV and 7.7 GeV.
                        You may want to mention those in your slides and
what we can learn from the extracted source size information.


     With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng

On 2022/7/22 6:24 PM, webmaster--- via Star-cf-l wrote:
> Dear star-cf-l AT lists.bnl.gov members,
>
> Chuan Fu (fuchuan AT mails.ccnu.edu.cn) has submitted a material for a review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/60372

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