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star-cf-l - Re: [Star-cf-l] STAR presentation by Ashish Pandav for DAE HEP 2020 submitted for review

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Subject: STAR Correlations and Fluctuations PWG

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  • From: apandav <apandav AT rcf.rhic.bnl.gov>
  • To: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
  • Cc: Star-cf <star-cf-l AT lists.bnl.gov>, webmaster AT star.bnl.gov
  • Subject: Re: [Star-cf-l] STAR presentation by Ashish Pandav for DAE HEP 2020 submitted for review
  • Date: Tue, 22 Sep 2020 18:23:18 +0530

Dear Hanna,

Many thanks for the sign-off.

Best regards,
Ashish


On 2020-09-22 18:20, Hanna Paulina Zbroszczyk wrote:
Dear Ashish,

With those implemented I sign-off.

Best regards,
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 apandav <apandav AT rcf.rhic.bnl.gov> w dniu
21.09.2020, o godz. 14:58:

Dear Hanna,

Many thanks for the suggestions and comments. I have incorporated
them and can be found on the link below.


https://drupal.star.bnl.gov/STAR/system/files/DAE_HEP_abstract_e2.pdf

I have slightly rephrased the sentence
"The cumulants and their ratios are related to the correlation
length of the system and the susceptibilities that are also
calculable in various QCD-based models." -> The cumulants and their
ratios are related to the correlation length of the system and
susceptibilities. The susceptibilities are calculable in various
QCD-based models and lattice QCD.

Please let me know if there are any further suggestions.

Best regards,
Ashish

On 2020-09-21 13:29, Hanna Paulina Zbroszczyk via Star-cf-l wrote:
Hi Asish,
I agree with Xiaofeng that net-proton results need more
investigation
and should not be presented during this talk. Except this, I have
found few minor parts to be improved:
nature of quark-hadron phase transition and freeze-out dynamics ->
nature of quark-hadron phase transition, and freeze-out dynamics
The cumulants and their ratios are related to the correlation length
of the system and the susceptibilities that are also calculable in
various QCD-based models. -> The cumulants and their ratios related
to
the system's correlation length and the susceptibilities are also
calculable in various QCD-based models.
the STAR detector at RHIC in the year 2018.-> the STAR detector at
RHIC in 2018.
Cumulants and ratios of cumulants of net-proton, net-kaon and
net-charge distributions -> Cumulants and ratios of cumulants of
net-kaon, and net-charge distributions.
Thank you,
With my best regards,
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 webmaster--- via Star-cf-l
<star-cf-l AT lists.bnl.gov> w dniu 17.09.2020, o godz. 08:05:
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/52110
---
If you have any problems with the review process, please contact
webmaster AT www.star.bnl.gov
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