STAR Correlations and Fluctuations PWG

[Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>]

Hi Hanwen,

   Thanks for preparing these nice slides. I have a question for my own understanding

The energy dependence of the B-S correlator seems similar to that for the hadron gas shown on slide 4. Do you have a comparison of those calculations to the data? What does this mean, that the values are consistent with hadron gas at these energies?

On S.17, the comparison to QGP expectation is labelled 'Ideal QGP'. What is meant by ideal here? What deviations from it could affect the B-S correlator? The FRG calculations are consistent at 39 and 64 GeV, what do the calculations include? Do we measurements at 200 GeV, how does it compare to FRG or LQCD calculations?

thanks,

Sooraj

On Thu, May 9, 2024 at 7:37 AM Hanwen Feng via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Nu,

Thanks for your suggestions, I have changed the position of legends and texts in Slide 15 and removed the duplicate 2-nd bullets in the summary part. The revised version can be accessed with the same path as the previous one.

Best regards,

Hanwen Feng 

From: webmaster--- via Star-cf-l

Date: 2024-05-08 20:27

To: star-cf-l

CC: webmaster

Subject: [Star-cf-l] STAR presentation by Hanwen Feng for CPOD 2024 submitted for review

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

 

Hanwen Feng (hwfeng AT mails.ccnu.edu.cn) has submitted a material for a review, 

please have a look:

https://drupal.star.bnl.gov/STAR/node/67708

 

Deadline: 2024-05-20

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

webmaster AT www.star.bnl.gov

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--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44242

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov