STAR Flow, Chirality and Vorticity PWG

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

Dear Xionghong

The followings are comments on your merged talk abstract from conveners. 

Best regards, Jiangyong, Prithwish and ShinIchi

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Jiangyong 

Title: How about "Measurement of collective flow for light-nuclei and hyper-nuclear in Au+Au collisions from STAR"

L6 Measurements of light-nuclei and hyper-nuclei yields and collectivity provide--> The yield and collective flow of light-nuclei and hyper-nuclei are sensitive to the production mechanics and the dynamics of the late-time hadronic medium produced in high-energy nuclear collisions.

Comment: this statement is very generic. Can you state what kind of unique information and production mechanism?

L8 The results from hyper-nuclei would shed--> In particular, the production and flow of hyper-nuclei probes directly the hyperon-nucleon interactions in the high baryon density region.

L15 how about: Model comparison suggests that the dynamics of light-nuclei and hyper-nuclei are dominated by hadronic interactions.

Prithwish

L7: “underlying production mechanism” → “underlying particle production mechanism” 

L8: “The results from” → “In addition, the results from”

L12: “compared with those” → “compared to those”  

ShinIchi

I’m OK to sign off.

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On Nov 17, 2021, at 13:07, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

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

Xionghong He (hexh AT impcas.ac.cn) has submitted a material for a review,  
please have a look:
https://drupal.star.bnl.gov/STAR/node/57277

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