STAR Flow, Chirality and Vorticity PWG

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

Dear Li-ke Liu, Priyanshi Sinha, Ding Chen, Prabhupada Dixit

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

Best regards, Jiangyong, Prithwish and ShinIchi

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Jiangyong

L1: people know what v1 and v2 are, so I suggest delete "are the first and second harmonic coefficients in the Fourier expansion of the final state azimuthal distribution relative2

to the collision reaction plane"

Just write "In low energy heavy ion collisions, directed and elliptic flow v1 and v2 are sensitive to the dynamics...

L4-5  Higher harmonic triangular flow, v3, originating from initial geometry fluctuations, is suggested to be an even more sensitive probe for the viscosity of the medium

and initial density profile of the colliding nuclei. --> The triangular flow v3 provides complementary information on the initial geometry fluctuations and transport properties of the medium.

L14 when collision....->around √s_NN=10-20 GeV

L15 seems to be lower

L16 how about "With the much enhanced statistics from the BES-II dataset, we present precision measurement of v1 and v2 for k+-..... together with the v3 for phi...

L19. How about "Implication of these measurements on the QCD phase structure at high mu region is discussed."

Prithwish

Line 12: “In the first phase RHIC” → “From the measurements based on the first phase of RHIC” 

Line 16: “the second phase RHIC” →”the second phase of RHIC” 

ShinIchi

L16-21: In stead of giving different beam energy regions for different particle species that we are going to present, we can just mention v1, v2 and v3 for all the particle species and full energy energy range including fixed target mode.

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On Nov 14, 2021, at 2:35, webmaster--- via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

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

Prabhupada Dixit (prabhupadad AT iiserbpr.ac.in) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/57200

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