STAR Flow, Chirality and Vorticity PWG

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

Dear Subhash,

Thanks for these nice suggestions.
The updated version can be find at
https://drupal.star.bnl.gov/STAR/node/59716.

Best regards,
Xionghong

> -----Original Message-----
> From: subhash [mailto:subhash AT rcf.rhic.bnl.gov]
> Sent: Friday, May 27, 2022 5:59 PM
> To: Xionghong <hexh AT impcas.ac.cn>
> Cc: 'STAR Flow, Chirality and Vorticity PWG' <star-fcv-l AT lists.bnl.gov>
> Subject: Re: [Star-fcv-l] STAR presentation by Xionghong He for 2022 
> RHIC/AGS
> submitted for review
> 
> Dear Xionghong,
> 
> Thanks for considering my suggestions. I have a few additional suggestions. 
> I
> sign off once these are addressed.
> 
> General, you can modify all the labels e.g. "STAR poster/talk at Quark 
> Matter
> 2022" --> "Quark Matter 2022"
> 
> slide 8: EOS --> EoS (to be consistent with other slides)
> 
> sl#10: You can stress that 27 GeV is from BES-II (verbally). Actually there 
> is a
> 10-20% deviation from mass number scaling with better precision which is
> different than our previous conclusion from BES-I measurements. You can
> change the conclusion:
>   10-20% deviation from mass number scaling, coalescence production (?)
> 
> sl#12: Unclear --> Unsettled
> 
> sl#14: EoS
> 
> sl#15: Non-zero proton v3 (psi1) ...
> 
> Light nuclei v2 shows tension in the atomic-mass number scaling
> 
> Positive deuteron v1 slopes need inputs from theory
> 
> Thanks and regards,
> Subhash
> 
> On 2022-05-27 04:59 PM, Xionghong wrote:
> > 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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