STAR Flow, Chirality and Vorticity PWG

[ShinIchi Esumi <esumi.shinichi.gn AT u.tsukuba.ac.jp>]

Dear Haojie

The followings are comments on your talk abstract from conveners. 

Best regards, Jiangyong, Prithwish and ShinIchi

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Jiangyong

L2 -->dense nuclear matter in neutron stars and heavy ion collisions.

L5 by the aforementioned strong interaction means-->in hadronic collisions

L6 remove "completely apart"

L7 traditional low-energy scatterings-->traditional method

L12 world-wide data -->World data

L12 effect-->implication

Prithwish

"by smashing isobar nuclei" -->"by colliding isobar nucleai

"mean transverse momentum" -->"mean transverse momenta" 

"world-wide data" --> "global data"

It's not clear what is meant by "and the recent PREX-II tension" -- do you mean "tension with PREX-II data" ?

ShinIchi

Should we mention some relations to the deformation study/talk from Chunjian/Jiangyong? 

This might be asked to merge later on by QM organizers. I’m fine to sign-off. 

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On Nov 16, 2021, at 13:17, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

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

Haojie Xu (haojiexu AT zjhu.edu.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/57251

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