Skip to Content.
Sympa Menu

star-cf-l - Re: [Star-cf-l] STAR presentation by Yevheniia Khyzhniak for WWND 2024 submitted for review

star-cf-l AT lists.bnl.gov

Subject: STAR Correlations and Fluctuations PWG

List archive

Chronological Thread  
  • From: Eugenia Khyzhniak <eugenia.sh.el AT gmail.com>
  • To: Nu Xu <nxu AT lbl.gov>
  • Cc: STAR Correlations and Fluctuations PWG <star-cf-l AT lists.bnl.gov>
  • Subject: Re: [Star-cf-l] STAR presentation by Yevheniia Khyzhniak for WWND 2024 submitted for review
  • Date: Fri, 9 Feb 2024 00:22:38 -0500

Dear Nu,
Thank you!

Updated: https://drupal.star.bnl.gov/STAR/system/files/wwndKhyzhniak_2.pdf

Best regards,
Yevheniia

On Fri, Feb 9, 2024 at 12:10 AM Nu Xu <nxu AT lbl.gov> wrote:
Dear Yevheniia and All,

I have no further issues with the presentation, except the reference in the up-right plot on slide 43.
After replace it with the correct one, I sign off.

Best regards,
Nu

> On Feb 8, 2024, at 9:01 PM, Eugenia Khyzhniak via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>
> Dear Hanna and Nu,
>
> I updated my talk according to today's meeting discussion: https://drupal.star.bnl.gov/STAR/system/files/wwndKhyzhniak_1.pdf
> I also added link to my preliminary plots to the page with all reliminaries: https://drupal.star.bnl.gov/STAR/blog/gos/correlations-and-fluctuations-preliminary-plots
>
> Thank you,
> Yevheniia
>
> On Mon, Feb 5, 2024 at 7:38 AM Hanna Paulina Zbroszczyk via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
> Dear Yevheniia,
>
> Thank you for posting your talk in advance.
> I can’t find your results in our preliminary page:
> https://drupal.star.bnl.gov/STAR/blog/gos/correlations-and-fluctuations-preliminary-plots
>
> We should discuss during next CF PWG preliminary requests to results you intend to show during WWND.
>
> Thanks,
> Hanna
>
> Hanna Paulina Zbroszczyk
> PhD DSc Eng, Professor
>
> 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 Eugenia Khyzhniak via Star-cf-l <star-cf-l AT lists.bnl.gov> w dniu 05.02.2024, o godz. 04:56:
>>
>> Dear Nu,
>>
>> I've updated my slides: https://drupal.star.bnl.gov/STAR/system/files/wwndKhyzhniak.pdf
>>
>> >lide 42 - Summary - 4th and last bullet: (i) The ‘good agreement’ between data and the UrQMD calculation is reached only for '7.7 Au+Au collisions, 30-50% centrality, from the SL correlation'. It is not the case, for example see slide 41, for 10-30% collision centrality. Please add these conditions to the bullet;
>> I tried to clarify what I meant in my updated summary slide. Please take a look.
>>
>> >Why it is important to observe the consistence between the HBT result from the pair measurement and “the tilt from the freeze-out distribution” from single particles, at k_T = 0?
>> I'm looking for the correspondence between HBT results and freeze-out (FO) distribution of pions, but I'm not claiming that those have to be the same. This is more like a test. I'm extrapolating my HBT tilt to zero kT in order to get the biggest possible homogeneity region and trying to see if the HBT tilt agrees with the same from FO dist.
>>
>> >slide 42 - 2nd bullet - up-right figure: Where did you find the data points from low collision energies? In the listed reference, I could not see the experimental data points.
>> You're right, thanks! I mixed it up with another PLB paper from 2000. I've put the right one now. Please take a look.
>>
>> Thank you,
>> Yevheniia
>>
>> On Sun, Feb 4, 2024 at 8:17 PM Nu Xu via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>> Dear Yevheniia and All,
>>
>> Here are my suggestions/questions about the draft of your WWND2024 talk:
>>
>> 1) slide 42 - Summary - 4th and last bullet: (i) The ‘good agreement’ between data and the UrQMD calculation is reached only for '7.7 Au+Au collisions, 30-50% centrality, from the SL correlation'. It is not the case, for example see slide 41, for 10-30% collision centrality. Please add these conditions to the bullet; (ii) Why it is important to observe the consistence between the HBT result from the pair measurement and “the tilt from the freeze-out distribution” from single particles, at k_T = 0?
>>
>> 2) slide 42 - 2nd bullet - up-right figure: Where did you find the data points from low collision energies? In the listed reference, I could not see the experimental data points.
>>
>> Thank you,
>> Nu
>>
>>
>>
>> > On Feb 4, 2024, at 2:36 PM, webmaster--- via Star-cf-l <star-cf-l AT lists.bnl.gov> wrote:
>> >
>> > Dear star-cf-l AT lists.bnl.gov members,
>> >
>> > Yevheniia Khyzhniak (eugenia.sh.el AT gmail.com) has submitted a material for a 
>> > review, please have a look:
>> > https://drupal.star.bnl.gov/STAR/node/66727
>> >
>> > Deadline: 2024-02-11
>> > ---
>> > If you have any problems with the review process, please contact 
>> > webmaster AT www.star.bnl.gov
>> > _______________________________________________
>> > Star-cf-l mailing list
>> > Star-cf-l AT lists.bnl.gov
>> > https://lists.bnl.gov/mailman/listinfo/star-cf-l
>>
>> _______________________________________________
>> Star-cf-l mailing list
>> Star-cf-l AT lists.bnl.gov
>> https://lists.bnl.gov/mailman/listinfo/star-cf-l
>> _______________________________________________
>> Star-cf-l mailing list
>> Star-cf-l AT lists.bnl.gov
>> https://lists.bnl.gov/mailman/listinfo/star-cf-l
>
> _______________________________________________
> Star-cf-l mailing list
> Star-cf-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-cf-l
> _______________________________________________
> Star-cf-l mailing list
> Star-cf-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-cf-l




Archive powered by MHonArc 2.6.24.

Top of Page