STAR Correlations and Fluctuations PWG

[Zachary Sweger <zwsweger AT ucdavis.edu>]

Dear Conveners,

Thank you very much for the comments. I've updated my slides which are available at https://drupal.star.bnl.gov/STAR/system/files/DNP2022_v1.pdf.  Please let me know if these changes are sufficient. 

Thank you,

Zachary Sweger

On Thu, Oct 20, 2022 at 6:17 AM Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Zachary,

Please find my comments below:

Slide 2: Please consider adding QCD phase diagram and explaining what are the scientific goals of the BES program

Introduce fluctuation method, some variables and quantities you use.

Slide: showing STAR detector would help to understand presented figure here.

Slide 5, 6, 9: try to put less text (rather short pieces of  information)

With those implemented, I sign off.

Best regards,

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 Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 17.10.2022, o godz. 16:43:

Hi Zach,

    Please find my comments/suggestions to your DNP slides :

    1. Title -> Prospects on Proton Cumulant Analysis at the STAR Fixed-Target Program
        In your slides, you may add a slide to discuss the QCD phase diagram and motivation of STAR Beam Energy Scan program.

    2. Slide 2, the reference below the plot : STAR,   Phys. Rev. Lett. 128, 202303 (2022) ;  arXiv : 2209.11940.
                                                                              Phys. Rev. Lett. 126, 092301 (2021);  Phys. Rev. C 104, 024902 (2021).

    3. BES-I data showed possible evidence of fluctuations -> Non-monotonic energy dependence was observed in BES-I data with a 3.1 sigma significance.
        High-statistics data  with detector improvements have been taken from 7.7 GeV to 27 GeV.-> High-statistics data (BES-II collider mode) with detector improvements have been
        taken from 7.7 GeV to 27 GeV. I think you may add a table or figure to demonstrate the stataticics of those BES-II data. Not only show FIX data.

    4. Slide 3, You should have a better figure to demonstrate the Fixed target program at STAR.  and in somewhere to show the muB coverage of FXT program.
   
    5. After slide 4, you may discuss ETOF detector in detail before showing the acceptance plot in next slide.

    6. Slide 6, Move after slide 4, but not showing the efficiency and PID plot. I think we are not ready to show those plots without proper calibrations.
      
    7. Slide 7, the title of this slide is covered by STAR logo.
   
    8. Slide 8, It is not clear to me how the right plot is produced and what does it mean. I suggest not to show this plot before it was discussed in PWG and focusing groups.
   
     9. Slide 9, Summary : A main objective of the STAR Fixed-Target Program->  "A main objective of the BES-II (Both collider and FIX target) program"
                     Third item : at low energies->at low energies (3 - 7.7 GeV).
                     Fourth item : 8 new data points -> More data points

        With those implemented, I sign off.

Thank you,     
Best Regards,
Xiaofeng

On 2022/10/14 06:05, webmaster--- via Star-cf-l wrote:

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

Zachary Sweger (zwsweger AT ucdavis.edu) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/61323

Deadline: 2022-10-27
---
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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