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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review
- From: Gavin Wilks <gwilks3 AT uic.edu>
- 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 Gavin Wilks for SPIN 2023 submitted for review
- Date: Fri, 19 Jan 2024 22:07:26 +0100
Dear Subhash,
abstract:
s = s_NN =
- Done
nuclear structure --> What do you mean by nuclear structure here, I didn't get the context here.
- The structure of nucleons within nuclei. I should also include nucleon structure as well.
- I have rewritten the last sentence as βThese differential measurements can help understand the roles of the $\phi$-meson force field in nucleon and nuclear structure, in addition to the evolution of nuclear matter.β
l#10: At the center of non-central --> At the non-central
- Done
l#25: rest frame
- Corrected
l#43-44: Along this line, you may mention BES-II allow more precision and differential measurements which were not possible from BES-I.
- I added this in a sentence at the end of the paragraph.
l#61: some temporary complications of signal extraction --> I think this line is not needed, since it do not explain what is the underlying complication. It seems too technical.
- Removed.
Or may be you can rephrase something like, In future we will extend measurements beyond 1.0 !
- I added βand we will extend measurements to $\eta<1.5$ in the future.
l#68: The mixed-event method is used to generate the combinatorial background ....
- Changed.
l#72-73: Have you varied background shape eg poly-3 vs poly-2 for systematics?
- I have studied this recently and I plan to include this contribution to the systematics, but it is not included in the preliminary results shown.
l#75: Is the width fixed to PDG or extracted from data for integrated theta* bins?
- The width is extracted from data for the integrated theta* bins.
l#94-95: Do you apply any PID efficiencies?
- Not currently, I am planning to study this.
l#115: The fit presented for the second-order event plane results is s fit only to BES-I
--> may be rephrased as, the solid line is a fit only to BES-I data ...
- Done.
l#117: The BES-II data at βπ NN = 19.6 GeV is consistent with the model fit from BES-I and the details of the fit can be found in [1].
--> I think this line is not necessary and can be removed. A better approach would be to fit when precise data will be available for all BES-II energies.
- I removed the line.
l#153: to be more specific: ... increasing π00 with rapidity (|y|>0.5) for both energies ...
- Done
l#156: many collision energies --> remaining collision energies
- Done
l#157: I'd suggest a rephrase: This work explores the potential link between the π-meson field and global spin alignment, ...
- Done
On Jan 19, 2024, at 16:40, Gavin Wilks <gwilks3 AT uic.edu> wrote:Dear Subhash,I will remove it. Thanks for the clarification.Best,GavinOn Jan 19, 2024, at 16:37, subhash <subhash AT rcf.rhic.bnl.gov> wrote:Dear Gavin,
I mean to remove the line 117.
For the fit in the Figure, I am fine with it either ways.
Thanks and regards,
Subhash
On 2024-01-19 09:35 PM, Gavin Wilks wrote:Dear Subhash,
Thank you for the comments.
Regarding your comment on line 117, are you suggesting that I remove
the fit to BES-I data in the figure?
Best,
GavinOn Jan 19, 2024, at 04:16, subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:
Dear Gavin,
Very nice proceedings. I have a few questions and suggestions below for your consideration:
abstract:
s = s_NN =
nuclear structure --> What do you mean by nuclear structure here, I didn't get the context here.
l#10: At the center of non-central --> At the non-central
l#25: rest frame
l#43-44: Along this line, you may mention BES-II allow more precision and differential measurements which were not possible from BES-I.
l#61: some temporary complications of signal extraction --> I think this line is not needed, since it do not explain what is the underlying complication. It seems too technical.
Or may be you can rephrase something like, In future we will extend measurements beyond 1.0 !
l#68: The mixed-event method is used to generate the combinatorial background ....
l#72-73: Have you varied background shape eg poly-3 vs poly-2 for systematics?
l#75: Is the width fixed to PDG or extracted from data for integrated theta* bins?
l#94-95: Do you apply any PID efficiencies?
l#115: The fit presented for the second-order event plane results is s fit only to BES-I
--> may be rephrased as, the solid line is a fit only to BES-I data ...
l#117: The BES-II data at βπ NN = 19.6 GeV is consistent with the model fit from BES-I and the details of the fit can be found in [1].
--> I think this line is not necessary and can be removed. A better approach would be to fit when precise data will be available for all BES-II energies.
l#153: to be more specific: ... increasing π00 with rapidity (|y|>0.5) for both energies ...
l#156: many collision energies --> remaining collision energies
l#157: I'd suggest a rephrase: This work explores the potential link between the π-meson field and global spin alignment, ....
I sign off with these addressed.
Thanks and regards,
Subhash
On 2024-01-19 01:52 AM, webmaster--- via Star-fcv-l wrote:Dear star-fcv-l AT lists.bnl.gov members,_______________________________________________
Gavin Wilks (gwilks3 AT uic.edu) has submitted a material for a review, please
have a look:
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-
[Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
webmaster, 01/18/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
subhash, 01/18/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
Gavin Wilks, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
subhash, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
Gavin Wilks, 01/19/2024
- Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review, Gavin Wilks, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
Gavin Wilks, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
subhash, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
Gavin Wilks, 01/19/2024
-
Re: [Star-fcv-l] STAR presentation by Gavin Wilks for SPIN 2023 submitted for review,
subhash, 01/18/2024
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