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star-cf-l - Re: [Star-cf-l] STAR presentation by Samuel Heppelmann for Quark Matter 2022 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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Chronological Thread  
  • From: Xiaofeng Luo <xfluo.star AT hotmail.com>
  • To: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Samuel Heppelmann for Quark Matter 2022 submitted for review
  • Date: Thu, 18 Nov 2021 15:32:39 +0800

Hi Sam,

    Nice abstract.
    Please find my comments and suggestion below :

1.   Line 6, event-by-event -> high-order

2.   Line 7,  depend on the non-equilibrium -> sensitive to the

3.   Line 8, protons and anti-protons-> fluctuations of proton number

4.   Line 9, baryons and anti-baryons -> baryon number fluctuations

5.   Line 10, showed -> shows

6. Line 12, energy range should be 7.7 to 62.4 GeV instead of 7 - 27 GeV.

7. Line 17, It would be nice to mention the baryon chemical potential for 3 GeV.

8.  Line 23, I am not sure we will compare to hydrodynamic model at 3 GeV. Please confirm.

9. At the time of QM, are we ready to present correlation function at 3 GeV ? Please confirm.

With those implemented, I sign off.

Thank you,
Best Regards,
Xiaofeng



On 2021/11/16 12:54 AM, webmaster--- via Star-cf-l wrote:
Dear star-cf-l AT lists.bnl.gov members,

Samuel Heppelmann (sheppelmann AT gmail.com) has submitted a material for a
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/57235

---
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 #: +86-27-67867963





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