STAR Correlations and Fluctuations PWG

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

Dear Hanna,

              Thank you for your comments and sign off.

The slides on merging and splitting were removed.

Please find the revised slides:

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

Best regards,

Chuan

 

 

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

From:  "Hanna Paulina Zbroszczyk"<hanna.zbroszczyk AT pw.edu.pl>;

Date:  Sun, Jul 24, 2022 10:56 PM

To:  "ChuanFu"<fuchuan AT mails.ccnu.edu.cn>;

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

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

 

Dear Chuan,

Thank you very much for update.

I have just one question regarding merging and splitting. As you don’t show any plot with data, do you still plan to discuss them?

If not, I propose to remove them.

With this considered I sign off. Enjoy the conference.

Thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez ChuanFu <fuchuan AT mails.ccnu.edu.cn> w dniu 22.07.2022, o godz. 23:42:

Dear Hanna,

               Thank you very much for your nice comments.

Please find my revised slides and replies below:

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

General comment: if you don’t use plots from your own resources, please add references to all plots that are not yours (e.g, slide 5).

------- The reference (Nature 588: 232-238 (2020)) was added in slide 5.

Slide 3: Since you mention all BES program, including COLL and FXT mode, I suggest to replace the plot with QCD phase diagram with one introducing all BES energies too. It is good to pay more attention to 3 GeV as you concentrate on it.

------- The new plot with all BES program was used.

Slide 4: I suggest to underline that with at HBT method in astronomy we study angular sizes of stars while in heavy-ion we problem properties of the source.

------- Revised

Slide 5: please define all quantities from the formula of k*.

Make uniform Qinv or qinv

k* = qinv/2 (but only for particles with identical masses) - make it clear on your slide

------- The qinv has been used in many figures,  I added a sentence to clarify this (see slide 5), hope can make it clearer. 

Slide 10: is it labelled as preliminary?

I don’t see the plot there:

https://drupal.star.bnl.gov/STAR/blog/fuchuan/ppcfqpt2021

I also don’t remember we granted preliminary labels for this plot

Slide 12: The same comment as for slide 10, I don’t remember preliminary granted..

------- If possible, I would like to request preliminary results for slide 10 and slide 12 in the next CF PWG meeting.

Best regards,

Chuan

 

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

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

Date:  Fri, Jul 22, 2022 10:19 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

 

Dear Chuan,

Please find below my comments to your nice slides:

General comment: if you don’t use plots from your own resources, please add references to all plots that are not yours (e.g, slide 5).

Slide 3: Since you mention all BES program, including COLL and FXT mode, I suggest to replace the plot with QCD phase diagram with one introducing all BES energies too. It is good to pay more attention to 3 GeV as you concentrate on it.

Slide 4: I suggest to underline that with at HBT method in astronomy we study angular sizes of stars while in heavy-ion we problem properties of the source.

Slide 5: please define all quantities from the formula of k*.

Make uniform Qinv or qinv

k* = qinv/2 (but only for particles with identical masses) - make it clear on your slide

Slide 10: is it labelled as preliminary?

I don’t see the plot there:

https://drupal.star.bnl.gov/STAR/blog/fuchuan/ppcfqpt2021

I also don’t remember we granted preliminary labels for this plot

Slide 12: The same comment as for slide 10, I don’t remember preliminary granted..

Thanks,

Hanna

Hanna Paulina Zbroszczyk

PhD DSc Eng, Professor WUT

E-mail: hanna.zbroszczyk AT pw.edu.pl

Tel: +48 22 234 5851 (office)

Address:

Warsaw University of Technology

Faculty of Physics

Nuclear Physics Division

Koszykowa 75

Office: 117b (via 115)

00-662 Warsaw, Poland

Wiadomość napisana przez webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 22.07.2022, o godz. 06:24:

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

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If you have any problems with the review process, please contact  
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