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star-fcv-l - Re: [Star-fcv-l] STAR presentation by Ashik Ikbal Sheikh for Quark Matter 2022 submitted for review

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Subject: STAR Flow, Chirality and Vorticity PWG

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Chronological Thread  
  • From: ASHIK IKBAL <ashikhep AT gmail.com>
  • To: Jiangyong Jia <jiangyong.jia AT stonybrook.edu>, "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] STAR presentation by Ashik Ikbal Sheikh for Quark Matter 2022 submitted for review
  • Date: Mon, 22 Nov 2021 17:02:18 -0500

Dear Jiangyong,

Thanks for your nice set of comments. I have incorporated them in the version2: https://drupal.star.bnl.gov/STAR/system/files/abstract_qm2022_ver2.pdf

Regarding the model comparison at L13, I want to mention the name of the model (PHSD+EM-field). So, I kept it there. 

Please let me know if you have any further comments.

Thanks,
Ashik

On Mon, Nov 22, 2021 at 4:32 PM Jiangyong Jia via Star-fcv-l <star-fcv-l AT lists.bnl.gov> wrote:
Ashik,

Here is my comments to your nice abstract.

Jiangyong

Title: remove “baryon”

L2. Maybe just RHIC, no need to spell out. 

L3 particle species where all constituent → hadron species whose constituent quarks are produced in the medium instead transported from initial state, K-..

L5. how about “We demonstrate using a new method that ..

L6-7. The sentence is a bit different to read about “We test the coalescence sum rule for hadrons with similar quark masses but but different electric…

L8. How about “This test is performed using v1 of hadrons with different quark content,  e.g.  ∆v1=v1) −v1( ̄Ω+), which is sensitive to the violation of coalescence sum rule.

L14 how about “A comparison model calculator suggests that the violation of the sum rule is caused by the strong EM field which couples to the v1 of produced quarks and antiquarks in opposite directions.

L16. How about “In addition to EM field, the sum rule is also violated due to presence of transported quarks, such as in p(uud). Hence”

L21 might be sensitive to the EOS and the dynamics of the medium→ This decomposite provides a new way to probe separate the EOS and dynamics of the medium in BES energies.


On 11/22/21 3:50 PM, webmaster--- via Star-fcv-l wrote:
Dear star-fcv-l AT lists.bnl.gov members,

Ashik Ikbal Sheikh (ashikhep AT gmail.com) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/57352

---
If you have any problems with the review process, please contact  
webmaster AT www.star.bnl.gov
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--
Ashik Ikbal
Research Associate
Kent State University
Department Of Physics
Kent, OH 44242, USA
Contact no.s: +1 631-504-7647 (USA)
                      +91 8250216234 (India)
Alternate e-mails: asheikh2 AT kent.edu
                             ashik AT rcf.rhic.bnl.gov
                             ashik.ikbal.sheikh AT cern.ch



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