STAR Flow, Chirality and Vorticity PWG

["Xionghong" <hexh AT impcas.ac.cn>]

Dear Subhash,

Thanks very much for your nice suggestions.
Please find the updated slides at the same link:
https://drupal.star.bnl.gov/STAR/node/59716.
Please let me know if there any further comments.

Best regards,
Xionghong

> -----Original Message-----
> From: subhash [mailto:subhash AT rcf.rhic.bnl.gov]
> Sent: Friday, May 27, 2022 2:32 PM
> To: STAR Flow, Chirality and Vorticity PWG <star-fcv-l AT lists.bnl.gov>
> Cc: hexh AT impcas.ac.cn
> Subject: Re: [Star-fcv-l] STAR presentation by Xionghong He for 2022 
> RHIC/AGS
> submitted for review
> 
> Dear Xionghong,
> 
> Very nice and comprehensive presentation. I have a few suggestions for your
> consideration:
> 
> In general, you don't need to mention individual STAR presenter's name,
> because this a STAR talk. I think it is fine if you have journal/conference 
> name.
> 
> sl#2:
> Anisotropic Flow --> Anisotropic flow
> Stiffness of Equation of State  --> Change in Equation of State or simply
> Equation of State (It can probe both softening and stiffness of
> EoS)
> Do you mean: Number of constituent quark (nucleon) scaling?
> 
> sl#3:
> 3~39 GeV --> 3 - 39 GeV, 𝑠𝑁𝑁(GeV)
> 
> sl#5:
> Non-zero proton v3,  increases monotonically with ...
> Negative v3 slope (dv3/dy = ....)
> "v3 is not only a consequence of initial fluctuations. It is sensitive to 
> EoS." -->
> This v3(Psi1) is not likely to originate from initial state fluctuations 
> since it is
> correlated to Psi1. You can simply say v3 is found to be correlated with 
> the first
> order event plane, sensitive to EoS.
> 
> sl#6:
> You can probably mention scaling holds better for anti-particles than 
> particles.
> Label inside figure "2.7 X improvement ..."  --> Can it be moved somewhere 
> else
> in the figure so it doesn't interfere with legend.
> 
> sl#9:
> Simple nucleon coalescence picture
> 
> sl#10.
> You can probably add the latest nucleon v2 preliminary from Rishabh right 
> here
> after this slide: https://drupal.star.bnl.gov/STAR/node/58790
> 
> sl#11:
> You can probably add references for left figure as well. These data are from
> multiple published papers.
> positive v1 slopes for deuteron in contrast to negative v1 slope for 
> protons is
> not clear High precision measurement at BES-II is underway
> 
> sl#13:
> What do you mean by v1 distribution, v1(y)?
> 
> sl#14:
> Hyper nucleii ?
> Multi-strange hadrons’ v1
> Make sure number of events are consistent with:
> https://drupal.star.bnl.gov/STAR/system/files/BES-
> IIFXT_event_counts_fromDan.pdf
> 
> sl#15:
> Non-zero proton v3, not likely to originate from initial state 
> fluctuations. Please
> change the conclusion accordingly.
> 
> Higher collision energies:
> NCQ scaling indicates Partonic degrees of freedom
> 
> Positive Deuteron v1 slopes, needed explanations or inputs from theory.
> 
> High precision measurements from BES-II is underway/ongoing.
> 
> 
> Thanks and regards,
> Subhash
> 
> On 2022-05-23 10:06 AM, webmaster--- via Star-fcv-l 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/59716
> >
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov
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