STAR Correlations and Fluctuations PWG

[Kincses Dániel <kincses AT ttk.elte.hu>]

Dear Nu,

Thank you for the suggestions; I uploaded a revised version:

https://drupal.star.bnl.gov/STAR/system/files/kincses_ISMD2023_proceedings_v2.pdf

I would prefer to keep the title, as it was the title of the contribution to the conference. The phrase "with Lévy-stable sources" in the title refers to the fact that the fits to the correlation functions were done with a Lévy-stable source assumption (instead of the usual Gaussian), which is an essential fact for the content of the paper. 

The pion acceptance is detailed in lines 102-106.

I changed the variable in Equations 4-5 to match the figure. Q denotes the one-dimensional variable, and the q in Equation 1 denotes the multi-dimensional variable. The q variable in Equation 3 is just an integration variable, needed for the Fourier-transform definition of the stable-distribution.

I removed the single-panel figure of R(mT). The idea behind showing the two different versions is that it is easier to see the centrality dependence on the single-panel version, with the four cases on top of each other. However, indeed it is the same information as the four-panel one.

Thanks again,
Best regards,
Daniel

---

Feladó: Nu Xu <nxu AT lbl.gov>
Elküldve: 2024. január 4., csütörtök 20:37
Címzett: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
Másolatot kap: Nu Xu <nxu AT lbl.gov>; Kincses Dániel <kincses AT ttk.elte.hu>
Tárgy: Re: [Star-cf-l] STAR presentation by Daniel Kincses for ISMD 2023 submitted for review

 

Hi Daniel and All,

Here are my suggestions/comments about the proceedings:

1) Title: Since it is an experimental report, I suggest change the title as “Pion Interferometry from \sqrt(s_{NN} - 200 GeV Au+Au Collisions at STAR”. I also do not really understand what does it mean by 'Levy-stable sources’.

2) Somewhere, we need to make it clear about acceptance of pions used in the analysis. For example, “identified both positive and negative pion pairs,  from |y|<0.5 and 0.15<p_T (GeV/c) <1.0, are used to construct the one-dimensional correlation function.” or something like that;

3) In Fig. 1, the x-axis variable is “Q (GeV/c), but in Eqs. (1), (3), (4) and (5) the variable is “q”. Let us define the variable clearly in the text and use it consistently;

4) Fig. 3 and Fig. 4 contain the same experimental information. I suggest remove Fig. 3;

That is all for now.

Best regards,
Nu



> On Jan 4, 2024, at 4:51 AM, Kincses Dániel via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>
> Dear All,
>
> I have prepared a proceedings contribution to ISMD2023; please find the draft here:
> https://drupal.star.bnl.gov/STAR/system/files/kincses_ISMD2023_proceedings.pdf
>
> Any comments or suggestions would be welcome,
> Thanks,
> DanielFeladó: Star-cf-l <star-cf-l-bounces AT lists.bnl.gov>, meghatalmazó: webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov>
> Elküldve: 2024. január 4., csütörtök 11:43
> Címzett: star-cf-l AT lists.bnl.gov <star-cf-l AT lists.bnl.gov>
> Másolatot kap: webmaster AT star.bnl.gov <webmaster AT star.bnl.gov>
> Tárgy: [Star-cf-l] STAR presentation by Daniel Kincses for ISMD 2023 submitted for review
>  Dear star-cf-l AT lists.bnl.gov members,
>
> Daniel Kincses (kincses AT ttk.elte.hu) has submitted a material for a review, 
> please have a look:
> https://drupal.star.bnl.gov/STAR/node/66357
>
> ---
> If you have any problems with the review process, please contact 
> webmaster AT www.star.bnl.gov
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