STAR Correlations and Fluctuations PWG

[Rutik Manikandhan <manikandhan.rutik AT gmail.com>]

Hello Nu,

I have made the changes as you've asked for. 

Link : https://drupal.star.bnl.gov/STAR/system/files/WWND__2024_ver_5.pdf

Here are our comments for your responses:

 

1) slide 10 - last bullet: I do not see the connections with other points. I suggest remove it;
    The elastic interactions would possibly widen the distribution for <pT> as now more particles gain momentum in either direction.
2) slide 11: It is not clear from the texts if the efficiency is extracted from embedding or other methods. Please make it clear;
    The plot has embedding efficiency on it, and I've added a QM reference
3) slide 13: (i) again, the notion for eta is for different frame, please make it consistent. Otherwise it will lead to confusion; (ii) plot: for y-axis, I suggest change the lower limit to something like -0.25;
   Changed accordingly
4) slide 16: (i) 2nd-bullet: the sentence is incomplete. Should be something like “Calculations from transport model …”; (ii) The meaning of bullet 3,4,5 is unclear. Not sure what do you want to say;
    Changed accordingly and added a relation between Temp and <pT>, we are trying to establish a thermal fluctuations scenario
5) slide 18 - 2nd bullet: the sentence is incomplete. Something like “STAR data from 200 GeV Au+Au collisions …”. The same for the 4th bullet;
    Changed accordingly
6) slide 19: It is redundant with respect to slide 18. I suggest remove it.
    This slide shows that UrQMD also follows an increase with decreasing centrality and that we might not have sensitivity at most central collisions, so we would like to keep it
7) slide 21 - last bullet: at the end, add “especially at the 3GeV Au+Au collisions. The effect is not yet fully understood” or something like this. This means that we are still thinking about the new result. This is th eke slide of the talk. The UrQMD model is a hadronic transport model. Supposedly, it works better for low energy collisions where partonic medium may not be dominant, see Ref. 5 and 6. However, here as one can see that the model result is totally failed while the model calculations show a reasonable energy dependence of the pT-correlation at higher collision energies. I do not understand why so.
   Changed accordingly
8) slide 21 - References: do we need 5 and 6?

    Changed accordingly

Best,

Rutik Manikandhan

PhD Candidate, Experimental Nuclear High Energy Group

Physics Dept.

University of Houston

On Fri, Feb 9, 2024 at 12:05 PM Nu Xu <nxu AT lbl.gov> wrote:

Dear Rutik and All,

Here are my suggestions for the draft:
1) slide 10 - last bullet: I do not see the connections with other points. I suggest remove it;

2) slide 11: It is not clear from the texts if the efficiency is extracted from embedding or other methods. Please make it clear;

3) slide 13: (i) again, the notion for eta is for different frame, please make it consistent. Otherwise it will lead to confusion; (ii) plot: for y-axis, I suggest change the lower limit to something like -0.25;

4) slide 16: (i) 2nd-bullet: the sentence is incomplete. Should be something like “Calculations from transport model …”; (ii) The meaning of bullet 3,4,5 is unclear. Not sure what do you want to say;

5) slide 18 - 2nd bullet: the sentence is incomplete. Something like “STAR data from 200 GeV Au+Au collisions …”. The same for the 4th bullet;

6) slide 19: It is redundant with respect to slide 18. I suggest remove it.

7) slide 21 - last bullet: at the end, add “especially at the 3GeV Au+Au collisions. The effect is not yet fully understood” or something like this. This means that we are still thinking about the new result. This is th eke slide of the talk. The UrQMD model is a hadronic transport model. Supposedly, it works better for low energy collisions where partonic medium may not be dominant, see Ref. 5 and 6. However, here as one can see that the model result is totally failed while the model calculations show a reasonable energy dependence of the pT-correlation at higher collision energies. I do not understand why so.

8) slide 21 - References: do we need 5 and 6?

That is all for now.

Best regards,

Nu



> On Feb 9, 2024, at 8:51 AM, Rutik Manikandhan <manikandhan.rutik AT gmail.com> wrote:
>
> Hello Nu,
>
> The version is v4 now, and this is the link:
> https://drupal.star.bnl.gov/STAR/system/files/WWND_2024_ver4.pdf
>
> Do let me know if this works for you.
> Thank you.
>
> Best,
> Rutik Manikandhan
> PhD Candidate, Experimental High Energy Group
> Physics Dept.
> University of Houston
>
>
> On Fri, Feb 9, 2024 at 10:47 AM Nu Xu <nxu AT lbl.gov> wrote:
> Dear Rutik,
> Somehow the link to drupal does not work.
> Please fix it asap.
>
> Thank you,
> Nu