STAR Correlations and Fluctuations PWG

["Li'Ang Zhang" <liangzhang AT mails.ccnu.edu.cn>]

Hi Grigory,

Thanks very much for you suggestions.

-Motivation section:

  -Acctrually the K0s and K0l are weak interaction eigenstates. They do not have there anti-particle. We even can not detect the stonge interaction eigenstates K0 and K0bar. The K0 and K0bar will have different FSI contribution, I think it can be measured in principle.

  -I assume the the precast sentence corrosponding the second sentence. One can found the reference at here: https://arxiv.org/abs/nucl-ex/0608012v1. The comma removed.

-Particle reconstruction section:

 

 

------------------ Original ------------------

From:  "Grigory Nigmatkulov"<nigmatkulov AT gmail.com>;

Date:  Wed, Aug 30, 2023 03:53 AM

To:  "STAR Correlations andFluctuation"<star-cf-l AT lists.bnl.gov>;

Cc:  "张李昂"<liangzhang AT mails.ccnu.edu.cn>;

Subject:  Re: [Star-cf-l] STAR presentation by Liang Zhang for Quark Matter 2023 submitted for review

 

Hi Li'Ang,

STAR Management has asked me to take a look at a few posters, including yours. The poster looks very nice.

Please find some minor suggestions below:

- Motivation section:

- The first part is very good but not sure that one can measure it experimentally (there is no way one can distinguish Ks and antiKs, or register Klong).

- Precast sentence should be proofreaded. Last sentence: remove comma.

- Particle reconstruction section:

- STAR Preliminary label is missing on the plot. Please add.

- K0s acceptance section:

- Replace ~ with -

-  -> The STAR detector

- K0s-K0s correlation function:

- Where the points for Data are coming from for the right figure?

- Results section:

- -> show reasonable agreement with the data

- Particle emission source parameters section:

- Systematic uncertainties on the plots for neighboring energies look unreliable because

  that cannot vary this much from energy to energy.

- Last bullet. I suggest to drop the last part of the sentence “, where …"

- References section:

- Currently, the reference style is different for different items. Please make reference style consistent.

Best regards,

Grigory

On Aug 27, 2023, at 3:01 AM, Li'Ang Zhang via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:

Dear Hanna and Toshihiro,

Thanks very much for you comments. I have implemented them and reupload my poster.

Please have a look: https://drupal.star.bnl.gov/STAR/node/64870

Cheers,

Li'Ang Zhang

 

------------------ Original ------------------

From:  "STAR Correlations andFluctuation"<star-cf-l AT lists.bnl.gov>;

Date:  Fri, Aug 25, 2023 08:24 PM

To:  "STAR Correlations andFluctuation"<star-cf-l AT lists.bnl.gov>; 

Cc:  "nonaka.toshihiro.ge"<nonaka.toshihiro.ge AT u.tsukuba.ac.jp>; 

Subject:  Re: [Star-cf-l] STAR presentation by Liang Zhang for Quark Matter 2023 submitted for review

 

Dear Li’Ang,

I have a few comments on your nice poster presentation.

With these considered, I sign off.

Best regards,

Toshihiro

(General)

- I think you are missing \bar for K^0 for many places

(Motivation)

- final state interaction

(Acceptance)

- K0s acceptance -> K^0_s acceptance

(K0S-K0S correlation function)

- can be described

(Results)

- Model calculations considering FSI …

---

差出人: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov> が Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> の代理で送信
送信日時: 2023年8月25日 18:02
宛先: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
CC: Hanna Paulina Zbroszczyk <hanna.zbroszczyk AT pw.edu.pl>
件名: Re: [Star-cf-l] STAR presentation by Liang Zhang for Quark Matter 2023 submitted for review

 

Hi Li’Ang,

Please find my comments on your nice poster.

Please remove the comma after your email.

Motivation:

Consider making the motivation part shorter. The content can remain the same but I suggest to make the statement shorter to give a space to some extra definitions.

Correct \bar{K^0} where appropriate,

Define S(\vec{r}), \vec{r}, \Psi.

k* usually denotes momentum of the first particle in PRF (if PRF is used, but at your measurements I see q_{inv} instead, which is also undefined). Instead of k* formalism I suggest to work with q, that you can define as relative momentum.

Define q_{inv}

Particle reconstruction:

Add please a reference [3] to KF where you describe the 3rd bullet.

Correlation function:

Can you add missing \bar at some K^0?

Please briefly define all symbols you use in the LL parametrization.

Define \epsilon

Particle emission source parameters:

Lednicky-Lyuboshitz Weight -> Lednicky-Lyuboshitz model.

Please add a reference to CRAB

With those implemented, I sign off.

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 25.08.2023, o godz. 08:25:

Dear star-cf-l AT lists.bnl.gov members,

Liang Zhang (liangzhang AT mails.ccnu.edu.cn) has submitted a material for a  
review, please have a look:
https://drupal.star.bnl.gov/STAR/node/64870

Deadline: 2023-09-03
---
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webmaster AT www.star.bnl.gov
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