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Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review
- From: Risa Nishitani <s2312412 AT gmail.com>
- To: Xiaofeng Luo <xfluo.star AT hotmail.com>, STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
- Subject: Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review
- Date: Sun, 12 Sep 2021 23:27:25 +0900
Dear Xiaofeng,
Thank you for your comments and suggestions.
I have revised my proceedings and you can find it in the following link;
https://drupal.star.bnl.gov/STAR/node/56188
Please kindly let me know if you have further comments or suggestions.
Best regards,
Risa
2021年9月11日(土) 1:53 Xiaofeng Luo via Star-cf-l <star-cf-l AT lists.bnl.gov>:
Hi Risa,
Nice proceedings,
Please find my comments/suggestions below :
1. In the abstract, the last few sentence, suggest to modify to : "In
this paper, we present the results of higher-order fluctuations up to
the sixth-order from p+ p collisions at √ s = 200 GeV. It provides
precise physics baselines to be compared to Au + Au collisions. The
positive signs of the fifth- and sixth-order fluctuation in p+p
collisions are observed and their multiplicity dependence are found to
connect smoothly to those from Au + Au collisions. "
2. If protons and antiprotons follow Poisson distributions
-> If protons and antiprotons follow independent Poisson distributions
3. assuming that efficiencies follow binomial distributions
-> assuming that detector responses follow binomial model
4. Page 3, bottom:
√ sNN 200 GeV
-> √ sNN = 200 GeV
5. Page 4, summary :
√ s 200 GeV
-> √ s = 200 GeV (some times use √ sNN, please make it consistent in
the paper)
6. Delete “This could not be the case for p+ p collisions.” In the last
sentence of summary.
7. Ref. 5, Cn the sign of kurtosis near the QCD critical point -> on the
sign of kurtosis near the QCD critical point
With those implemented, I sign off.
Thank you,
Best Regards,
Xiaofeng
On 2021/9/10 10:32, Risa Nishitani via Star-cf-l wrote:
> Dear Hanna,
>
> Thank you for your comments.
>
>
> I have revised the proceedings and you can find it in the following link;
>
>
> https://drupal.star.bnl.gov/STAR/node/56188
> <https://drupal.star.bnl.gov/STAR/node/56188>
>
>
> Please kindly let me know if you have further comments or suggestions.
>
>
> Best regards,
>
> Risa
>
>
>
>
>
> 2021年9月8日(水) 19:44 Hanna Paulina Zbroszczyk via Star-cf-l
> <star-cf-l AT lists.bnl.gov <mailto:star-cf-l AT lists.bnl.gov>>:
>
> Dear Risa,
>
> Please find below comments to your nice proceedings:
>
> Abstract:
> heavy ion -> heavy-ion
> at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV
> If you use p+p in the math mode, you should do the same for Au+Au
> (general comment to the whole draft)
>
> Introduction:
> at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV
>
> Cumulants:
> Please control numbering of your references, the reference [16]
> should change the number as it is cited after [6-8]
>
> Data set:
> 30 (cm) -> 30 cm
> 2 (cm) -> 2 cm
> 1 (cm) -> 1 cm
>
> Results:
> at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV
>
> Summary:
> at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV (when you refer to Au+Au)
> at 200 GeV -> at \sqrt{s} = 200 GeV (when you refer to p+p)
> at 200 GeV -> at \sqrt{s_{NN}} = 200 GeV (when you refer to Au+Au)
>
> With those implemented I sign off.
>
> Thanks,
> Hanna
>
> *Hanna Paulina Zbroszczyk*
> PhD DSc Eng, Professor WUT
>
> *E-mail*: hanna.zbroszczyk AT pw.edu.pl
> <mailto: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 webmaster--- via Star-cf-l
>> <star-cf-l AT lists.bnl.gov <mailto:star-cf-l AT lists.bnl.gov>> w dniu
>> 03.09.2021, o godz. 04:01:
>>
>> Dear star-cf-l AT lists.bnl.gov <mailto:star-cf-l AT lists.bnl.gov>
>> members,
>>
>> Risa Nishitani (s2312412 AT gmail.com <mailto:s2312412 AT gmail.com>)
>> has submitted a material for a review,
>> please have a look:
>> https://drupal.star.bnl.gov/STAR/node/56188
>> <https://drupal.star.bnl.gov/STAR/node/56188>
>>
>> ---
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> --
> ——————————————————————
> Risa Nishitani
> _s1930070 AT s.tsukuba.ac.jp <mailto:s1930070 AT s.tsukuba.ac.jp>_
> s2312412 AT gmail.com <mailto:s2312412 AT gmail.com>
> ---------------------------------------------
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--
Xiaofeng Luo
Professor of Physics
College of Physical Science and Technology
Central China Normal University
Luoyu Road 152, Wuhan China
Office Phone #: +86-27-67867963
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Risa Nishitani
-
[Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
webmaster, 09/02/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Hanna Paulina Zbroszczyk, 09/08/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Risa Nishitani, 09/09/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Xiaofeng Luo, 09/10/2021
- Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review, Risa Nishitani, 09/12/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Xiaofeng Luo, 09/10/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Risa Nishitani, 09/09/2021
-
Re: [Star-cf-l] STAR presentation by Risa Nishitani for CPOD March Meeting 2021 submitted for review,
Hanna Paulina Zbroszczyk, 09/08/2021
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