STAR Flow, Chirality and Vorticity PWG

[Ding Chen <dchen087 AT ucr.edu>]

Dear Subhash,

Thank you for your nice comments and patience! I've updated the slides according to your comments in version 3:

https://drupal.star.bnl.gov/STAR/node/61324

Best,

Ding

On Sun, Oct 16, 2022 at 1:22 AM subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:

Dear Ding.

Nice slides. I believe you do not have any new preliminary requests.
I sign off with following suggestions for your consideration:

In general the fonts for math-symbols looks odd, please change
fonts/style, if it is possible.

sl#3: I would suggest re-arranging bullets to reflect the following:
 From BES-I we saw a sign change in net-p and net-L (baryons), which
could be due associated to the softest EoS.
The phi mesons from BES-I also show a hint of sign change around similar
energy range for baryons
Then add a question what is the origin of sign change for phi mesons.

sl#4: You could add STAR detector diagram instead of phase diagram.

sl#5: Please add Yaxis labels. Try to avoid figures touch the bullet
texts.

sl#6: You could add details for PID, like Nsigma or mass-square range
etc.

sl#8: v1 is measured by event plane method using EPD. v1 corrected for
....

The v1(y) linear fit function is constrained to pass through the origin,
right? Please mention the fit function.

sl#9: Add reference for 7.7 GeV phi meson data.

sl#10: I would not say "softest point of EoS" here. I think the sign
change prediction is for baryons. While why phi mesons change sign is
not clear, at least not to me.

I would suggest adding a wording that a precise measurement of phi v1
will help probing the v1 sign change.

Thanks and regards,
Subhash



On 2022-10-14 05:19 AM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Ding Chen (dchen087 AT ucr.edu) has submitted a material for a review,
> please
> have a look:
> https://drupal.star.bnl.gov/STAR/node/61324
>
> Deadline: 2022-10-27
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