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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Alexey Povarov for Nucleus-2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: Alexey Povarov <povarovas AT gmail.com>
  • To: subhash <subhash AT rcf.rhic.bnl.gov>
  • Cc: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Alexey Povarov for Nucleus-2022 submitted for review
  • Date: Fri, 1 Jul 2022 19:01:54 +0300

Dear Subhash,

Thank you for your comments.

These v2 and v3 measurements have already been shown and have received the status of preliminary. Here is the link to the v2 and v3 preliminary: 

https://drupal.star.bnl.gov/STAR/blog/gnigmat/v2-and-v3-preliminary


In our analysis we used 27 GeV from BES-II and other energies from BES-I. I added this on slide#4.

> slide#5: It would be good to indicate BES-I vs BES-II. For BES-I resolutions, are you using published values or, are they from your own analysis?


> slide#6: Are these v2 values from published results? If yes, please add the journal reference.


We used event plane resolutions and v2 values from our own analysis.


> slide#7: How do you calculate integrated v2, would be good to indicate them like you do on slide#6. Do you use corrected pt spectra for example?


I added the definition of v_int like on slide#6. We have not applied any corrections for these values.


> slide#9: Is there a way you can quantify the quality of scaling?

We are working on it and it will be discussed at the PWG when results will be ready.


I implemented your comments. You can find slides here: https://drupal.star.bnl.gov/STAR/system/files/ASPovarov_NUCLEUS_2022_pres_ver2_0.pdf

Best regards,
Alexey


пт, 1 июл. 2022 г. в 05:35, subhash <subhash AT rcf.rhic.bnl.gov>:
Dear Alexey,

Nice results. I have following comments to your slides:

You have three duplicate entries in Drupal. I am discarding the
following ones:
https://drupal.star.bnl.gov/STAR/node/60123
https://drupal.star.bnl.gov/STAR/node/60124

General:
Is this triangular flow measurements are new preliminaries that will be
shown for the first time? If yes, could you please provide us a document
with a following format:
https://drupal.star.bnl.gov/STAR/system/files/Prelim_Request_template.pdf

It would be good into indicate BES-I/BES-II in all the relevant results
and slides. Recently STAR released a lot of BES-II measurements, so it
would help distinguish BES-I and BES-II.

Title: You can indicate BES-I here as well.

slide#3: Probably you can apply formatting to the bullets, so the words
will have equal spacing.
baryons then mesons --> baryons than mesons

slide#5: It would be good to indicate BES-I vs BES-II. For BES-I
resolutions, are you using published values or, are they from your own
analysis?

slide#6: Are these v2 values from published results? If yes, please add
the journal reference.
"Elliptic flow is more dependent on centrality than triangular flow" -->
Elliptic flow has stronger dependence on centrality than triangular flow

slide#7: How do you calculate integrated v2, would be good to indicate
them like you do on slide#6. Do you use corrected pt spectra for
example?

slide#8: Indicate BES-I and BES-II in relevant figures.
First measurement of identified particle v3 at BES energies.

slide#9: You can also add scaling holds better for particles than
anti-particles. Is there a way you can quantify the quality of scaling?

slide#10&11: positively charged particle species

v3 results (not corrected for efficiency) --> Do you expect any
significant change in v3 due to application of efficiency. If not, you
can change this "not corrected for efficiency" to a normal (not bold)
font.

Thanks and regards,
Subhash



On 2022-06-30 05:53 AM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Alexey Povarov (povarovas AT gmail.com) has submitted a material for a
> review,
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/60125
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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