Skip to Content.
Sympa Menu

star-fcv-l - Re: [Star-fcv-l] STAR presentation by Xionghong He for 2022 RHIC/AGS submitted for review

star-fcv-l AT lists.bnl.gov

Subject: STAR Flow, Chirality and Vorticity PWG

List archive

Chronological Thread  
  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • 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
  • Date: Fri, 27 May 2022 17:58:30 +0800

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, ๐‘ ๐‘๐‘(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 hadronsโ€™ 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
> _______________________________________________
> Star-fcv-l mailing list
> Star-fcv-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-fcv-l




Archive powered by MHonArc 2.6.24.

Top of Page