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Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review
- From: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
- To: Xiaofeng Luo <xfluo.star AT hotmail.com>, "star-cf-l AT lists.bnl.gov" <star-cf-l AT lists.bnl.gov>
- Subject: Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review
- Date: Tue, 30 Aug 2022 15:37:24 +0200
Hi Ashish,
Nice proceedings.
I sign off with comments implemented from Xiaofeng.
Thanks,
Hanna
Hanna Paulina Zbroszczyk
PhD DSc Eng, Professor WUT
E-mail: hanna.zbroszczyk AT pw.edu.pl
Tel: +48 22 234 5851 (office)
Address:
Warsaw University of Technology
Faculty of Physics
Nuclear Physics Division
Koszykowa 75
Office: 117b (via 115)
00-662 Warsaw, Poland
Wiadomość napisana przez Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 27.08.2022, o godz. 19:02:Hi Ashish,
Nice proceedings.
Please find my suggestions below :
1. Title : number -> multiplicity
2. 2nd line in the introduction: atleast -> at least
3. quark-gluon-plasma -> quark-gluon plasma
4. " The negative values, albeit with large uncertainties, and energy dependence is consistent with lattice QCD prediction for a crossover [6]."
It seems the conclusion is too strong indicating 7.7-200 GeV are all crossover. The reference 6 only has calculation with muB less than 200 MeV.(<20 GeV)
Please specify the energy range and use the conclusions in the STAR paper 2207.09837.
5. The journal # of reference 14 should be Phys. Rev. D 104, 094047 (2021). Please update it.
https://urldefense.com/v3/__https://journals.aps.org/prd/abstract/10.1103/PhysRevD.104.094047__;!!P4SdNyxKAPE!ErePFd-OSsUqN-l7Q7P66gPduiKe8g8bDJAGQbDJRM6w7jY9i2-hiQIgdyjYE_CpD6fa1g6WF2YtVLsTEqsj1_-XoXft$
6. Starting from "Interestingly, the combined signs of χ B 6 and χ B 8 can probe different phases...."
I would suggest not argue like this simply and may even not show Fig.2.
Because : 1) C6 and C8 are complicated as a function of T and muB. The Fig. 1 only shows results at muB=0.
https://urldefense.com/v3/__https://iopscience.iop.org/article/10.1088/1674-1137/43/5/054109__;!!P4SdNyxKAPE!ErePFd-OSsUqN-l7Q7P66gPduiKe8g8bDJAGQbDJRM6w7jY9i2-hiQIgdyjYE_CpD6fa1g6WF2YtVLsTEqsj1w3bm12V$ 2) In heavy-ion collisions, non-equilibrium effect and other background effects, such as baryon number conservation should be carefully studied
they may have different impact on C6 and C8.
You may say something like : they show negative values around Tc, which can be used to probe the quark-hadron phase transition boundary
and smooth crossover at muB=0, predicted by Lattice QCD.
7. Please specify the year taken for the 27 GeV.
8. In summary : ∼ 20 billion Au+Au collision events -> ∼ 20 billion Au+Au collision minimum bias events
scheduled to be -> are scheduled to be
With those implemented, I sign off.
Thank you,
Best Regards,
Xiaofeng
On 2022/8/24 01:03, webmaster--- via Star-cf-l wrote:Dear star-cf-l AT lists.bnl.gov members,
Ashish Pandav (apandav10 AT gmail.com) has submitted a material for a review,
please have a look:
https://drupal.star.bnl.gov/STAR/node/60597
Deadline: 2022-08-28
---
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Xiaofeng Luo
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[Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review,
webmaster, 08/23/2022
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Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review,
Xiaofeng Luo, 08/27/2022
- Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review, Hanna Paulina Zbroszczyk, 08/30/2022
-
Re: [Star-cf-l] STAR presentation by Ashish Pandav for SQM 2022 submitted for review,
Xiaofeng Luo, 08/27/2022
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