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Subject: STAR Flow, Chirality and Vorticity PWG
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Re: [Star-fcv-l] STAR presentation by Aditya Prasad Dash for Quark Matter 2023 submitted for review
- From: ADITYA PRASAD DASH <adityadash55 AT g.ucla.edu>
- To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
- Cc: subhash <subhash AT rcf.rhic.bnl.gov>, Huan Zhong Huang <huang AT physics.ucla.edu>, Gang Wang <gwang AT physics.ucla.edu>, Yan Gaoguo <15192958793 AT 163.com>, niseem magdy <niseemm AT gmail.com>
- Subject: Re: [Star-fcv-l] STAR presentation by Aditya Prasad Dash for Quark Matter 2023 submitted for review
- Date: Fri, 1 Dec 2023 15:58:11 -0800
Dear Dr. Subhash,
l#7-10: you can probably split it into two/three sentences. e.g.
In this work, we report measurements of two types of observables: (i)
charge-dependent directed flow (∆v1), which is sensitive to the initial
ultra-strong electromagnetic fields, and (ii) flow correlation, such as
rn(η), which is sensitive to the initial longitudinal de-correlation and
correlations among flow harmonics. These measurements contribute to
constraining the initial state of the collisions.
Done
l#15-16: of heavy-ion collisions at RHIC energies.
Done
l#19: the medium properties (such as electrical conductivity) and on the
formation time
Done
l#20: "is essential to understanding the evolution" --> is essential for
understanding the evolution
Done
l#40: should contribute --> could contribute to a
Done
l#46: "Data at √sNN = 200 GeV..." --> to be more specific you can
mention, the negative splitting in peripheral collisions at 200 GeV
right?
l#77: "We have presented STAR preliminary measurements" --> We have
presented measurements ... in the Beam Energy Scan program by STAR
experiment.
Done. Should we mention preliminary measurements or just measurements?
Thanks for your nice suggestions! The proceedings has been updated and can be found at the same link https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2023/Exploring-Electromagnetic-Field-Effects-and-Constraining-Transport-6
Here are the updates
title: BES-II
Done
Done
l#7-10: you can probably split it into two/three sentences. e.g.
In this work, we report measurements of two types of observables: (i)
charge-dependent directed flow (∆v1), which is sensitive to the initial
ultra-strong electromagnetic fields, and (ii) flow correlation, such as
rn(η), which is sensitive to the initial longitudinal de-correlation and
correlations among flow harmonics. These measurements contribute to
constraining the initial state of the collisions.
Done
l#15-16: of heavy-ion collisions at RHIC energies.
Done
l#19: the medium properties (such as electrical conductivity) and on the
formation time
Done
l#20: "is essential to understanding the evolution" --> is essential for
understanding the evolution
Done
l#40: should contribute --> could contribute to a
Done
l#46: "Data at √sNN = 200 GeV..." --> to be more specific you can
mention, the negative splitting in peripheral collisions at 200 GeV
right?
The same sentence mentions peripheral collisions, does this look fine/ can you give a suggested sentence?
l#48: "The larger magnitudes of ∆dv1/dy in peripheral collisions at
lower energies" ---> How about: An increase in magnitude of ∆dv1/dy in
peripheral collisions with decrease in beam energies. Along this lines,
you could mention we observed a similar pattern in data. It is not
evident from the text.
Done. The increase in the magnitude of ∆dv1/dy in peripheral collisions with decrease in beam energy, observed in data, is expected from the longer passage times 2R/gamma and shorter lifetimes of the fireball (due to which the late-time dilution of the $v_1$ splitting is smaller) at lower collision
lower energies" ---> How about: An increase in magnitude of ∆dv1/dy in
peripheral collisions with decrease in beam energies. Along this lines,
you could mention we observed a similar pattern in data. It is not
evident from the text.
Done. The increase in the magnitude of ∆dv1/dy in peripheral collisions with decrease in beam energy, observed in data, is expected from the longer passage times 2R/gamma and shorter lifetimes of the fireball (due to which the late-time dilution of the $v_1$ splitting is smaller) at lower collision
l#62-63: "r3(η) shows hints of larger deviation at lower beam energies"
--> I am not sure we can make conclusion on energy dependence based on
uncertainties. You can rephrase it with keeping only AMPT comparison.
Done
--> I am not sure we can make conclusion on energy dependence based on
uncertainties. You can rephrase it with keeping only AMPT comparison.
Done
l#77: "We have presented STAR preliminary measurements" --> We have
presented measurements ... in the Beam Energy Scan program by STAR
experiment.
Done. Should we mention preliminary measurements or just measurements?
Thanks,
Aditya
On Wed, Nov 29, 2023 at 1:35 AM subhash via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:
Dear Aditya,
Nicely written proceedings. I have a few suggestions for your
consideration:
title: BES-II
l#7-10: you can probably split it into two/three sentences. e.g.
In this work, we report measurements of two types of observables: (i)
charge-dependent directed flow (∆v1), which is sensitive to the initial
ultra-strong electromagnetic fields, and (ii) flow correlation, such as
rn(η), which is sensitive to the initial longitudinal de-correlation and
correlations among flow harmonics. These measurements contribute to
constraining the initial state of the collisions.
l#15-16: of heavy-ion collisions at RHIC energies.
l#19: the medium properties (such as electrical conductivity) and on the
formation time
l#20: "is essential to understanding the evolution" --> is essential for
understanding the evolution
l#40: should contribute --> could contribute to a
l#46: "Data at √sNN = 200 GeV..." --> to be more specific you can
mention, the negative splitting in peripheral collisions at 200 GeV
right?
l#48: "The larger magnitudes of ∆dv1/dy in peripheral collisions at
lower energies" ---> How about: An increase in magnitude of ∆dv1/dy in
peripheral collisions with decrease in beam energies. Along this lines,
you could mention we observed a similar pattern in data. It is not
evident from the text.
l#62-63: "r3(η) shows hints of larger deviation at lower beam energies"
--> I am not sure we can make conclusion on energy dependence based on
uncertainties. You can rephrase it with keeping only AMPT comparison.
l#77: "We have presented STAR preliminary measurements" --> We have
presented measurements ... in the Beam Energy Scan program by STAR
experiment.
Thanks and regards,
Subhash
On 2023-11-25 06:14 AM, webmaster--- via Star-fcv-l wrote:
> Dear star-fcv-l AT lists.bnl.gov members,
>
> Aditya Prasad Dash (adityaprasaddash55 AT gmail.com) has submitted a
> material
> for a review, please have a look:
> https://drupal.star.bnl.gov/STAR/node/66077
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
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- Re: [Star-fcv-l] STAR presentation by Aditya Prasad Dash for Quark Matter 2023 submitted for review, ADITYA PRASAD DASH, 12/01/2023
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