STAR Correlations and Fluctuations PWG

[Jinjin Pan <jpan AT tamu.edu>]

Dear Nandita, all,

Thanks to Takafumi's insights, I qualitatively compared our B(delta-y) and B(delta-phi) projections along with the BF integrals. I am attaching the comparison slide in this email. Here are the major take-aways:

Nandita‘s 𝐵(∆𝜑) & 𝐵(∆𝑦) (e.g. 𝜋𝜋) seems too large given their relatively small rapidity range. -> This indicates the projection calculation might not be right (if assuming the 2D BF is correct).
Nandita‘s calculation of BF integral (e.g. 𝜋𝜋) seems too small given their large 𝐵(∆𝜑) projections. -> This indicates the BF integral calculation might not be right.

Thanks and best regards,
Jin

On Fri, Jul 15, 2022 at 10:20 AM Nandita Raha via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Hi All, I uploaded a revised version for the WPCF talk. Please take a look in the following link: https://drupal.star.bnl.gov/STAR/system/files/WPCF_nraha_07192022_ver1.pdf Please let me know what you think. Thanks a lot! Best, ‍ ‍ ‍ ‍ ‍ ‍ ‍ ‍ ‍ ‍ ‍ ‍

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Hi All,

I uploaded a revised version for the WPCF talk.

Please take a look in the following link:

https://drupal.star.bnl.gov/STAR/system/files/WPCF_nraha_07192022_ver1.pdf

Please let me know what you think.

Thanks a lot!

Best,

Nandita

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