STAR Flow, Chirality and Vorticity PWG

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

Prithwish Tribedy ( ptribedy AT bnl.gov ) has commented on a material originally 
 
submitted by Yunshan Cheng ( yunshancheng AT g.ucla.edu ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2025/Search-Chiral-Magnetic-Wave-STAR

Comment:
Nice abstract !! I don't know what happened -- I sent comments last time, it  
didn't work. Anyway I sign off with the following comments.

The abstract overall needs a bit polishing to to strengthen it:

Title:
"Search for the Chiral Magnetic Wave at STAR"
-->
"Search for the Chiral Magnetic Wave at STAR with Isobar & Au+Au collisions"

Move a modified version of line 15 after this line:
"Experimental searches for the CMW, however, face challenges from background  
contributions related to elliptic flow and nonflow."
Add something like:
"Similar to the CME search, we use RHIC isobar collisions (Ru+Ru, Zr+Zr) for  
the CMW search, anticipating a stronger signal in Ru+Ru due to its larger  
magnetic field.
In addition, we compare Au+Au to study system dependence at top RHIC energy,  
examining the magnetic field effects from isobar to Au+Au."

line 11: Add "The prerequisite of CMW is expected to change with energy"

clarify "slope r_2" by adding "slope r_2 of v_2 vs. A_ch correlation"

line 17:
Move this line:
"The v_3- A^{ch} correlation will be discussed as a background indication."
Place it after line 9, following:
"The CMW leads to charge-dependent elliptic flow (v_2) which correlates with  
charge asymmetry (A^ch) of the system."











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