STAR Flow, Chirality and Vorticity PWG

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

Subhash Singha ( connectsubhash AT gmail.com ) has commented on a material  
originally submitted by Chenlu Hu ( huchenlu AT ucas.ac.cn ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/First-Measurements-Hyper-Nucleus-3%CE%9BH-Global-Polarization-AuAu-collis

Comment:
Dear Chenlu, All,
Richard made some good points. Since I am one of the PAs, let me attempt and  
suggest a few changes to make the physics message more clear. 
l#6-9: "Both large angular momenta  ... where baryon density is  
high"Â -->Â The large angular momentum generated in non-central heavy-ion  
collisions contributes to the formation of vorticity within the medium, which 
 
subsequently induces polarization of particles with non-zero spin.(I suggest  
we remove magnetic field part, because at this energy we will not be able to  
probe and it's not relevant here)

l#10-11: Since you want to focus on the high baryon region, how about the  
following wordings:Significant ... baryon region"Â -->Â The global  
polarization of Λ-hyperons near mid-rapidity increases at lower energies,  
which can be attributed to the correlation between angular momentum and  
enhanced baryon stopping. Recent model predictions suggest that the decay  
products of polarized hyper-nuclei (H3Λ) are highly sensitive to their spin  
structure. Additionally, in regions of high baryon density, the enhanced  
production of H3Λ makes their polarization measurement feasible.l#13: remove 
 
"in nuclear collisions"l#14: the global spin polarization"in 3 GeV Au+Au  
collisions" --> using  3 GeV Au+Au collisions with about 2 billion events  
collected during 2021 by STAR.
l#15: remove "from 2 billion events."l#17: Finally, the results will be  
compared with model predictions based on different assumptions of spin  
structures.

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