STAR Flow, Chirality and Vorticity PWG

[Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>]

Hi Xingrui,

   Nice results and very well put together slides. I have a few minor comments, please find below

S6: Please use a more recent version with iTPC, EPD and ETOF

S7: What are the predictions for the difference? Does it make sense to have them in the figure to compare?

S10: Could give a brief introduction to local polarization 

S15: Is it ideal hydro used in the claculations?

S17: With two energies, can we conclude no SHE is favored by data? What is the significance of the deviation from curve with SHE?

S18: Instead of listing by topics, you could directly highlight the main conclusion from each, like no splitting between Lambd and Lambda bar, no system size dependence etc

Best,

Sooraj

On Mon, Aug 28, 2023 at 12:30 AM subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear Xingrui,

Very nice slides. I have only a few suggestions for your consideration:

Please try unifying the style of reference eg PRL vs Phys Rev Lett
across slides.

s#7: Add a space 27GeV in title
1st bullet: about 10 times increase in statistics

4th bullet: upper limit on late stage Magnetic field

s#9: Please consider adding a reference for model

s#15: "Local polarization pT dependence" is repeated in three
consecutive bullets, you can consider a re-phrase.


Thanks and regards,
Subhash


On 2023-08-23 09:53 PM, webmaster--- via Star-fcv-l wrote:
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>
> Xingrui Gou (Gouxr AT sdu.edu.cn) has submitted a material for a review,
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--

Sooraj Radhakrishnan

Research Scientist,

Department of Physics

Kent State University

Kent, OH 44243

Physicist Postdoctoral Affiliate

Nuclear Science Division
Lawrence Berkeley National Lab
MS70R0319, One Cyclotron Road

Berkeley, CA 94720

Ph: 510-495-2473

Email: skradhakrishnan AT lbl.gov