STAR Correlations and Fluctuations PWG

[Mate Csanad <csanad AT bnl.gov>]

Dear Daniel,

Since this is a centrally invited overview talk, may I ask to include a slide 
about the collision energy (and centrality) dependent Lévy femtoscopy analyses? 
I believe the CPOD talk of Daniel Kincses contains the necessary materials:
https://conferences.lbl.gov/event/1376/contributions/8829/attachments/5136/4936/kincsesd_CPOD2024_talk_v6.pdf
maybe just slide 18 of that talk would be good, showing Figure 8 of this 
blogpost:
https://drupal.star.bnl.gov/STAR/blog/kincses/Pion-interferometry-Levy-stable-sources-STAR-FXT-energies
https://drupal.star.bnl.gov/STAR/system/files/alpha0_sqrts_fxt.pdf
with an inset showing Figure 6 of this blogpost:
https://drupal.star.bnl.gov/STAR/blog/kincses/Two-particle-interferometry-Levy-stable-sources-sqrtsNN-200-GeV-AuAu-collisions
https://drupal.star.bnl.gov/STAR/system/files/alpha0_npart.pdf
I know you have to make a selection, but maybe this could still have a place in 
your talk.

Thanks, best regards,
Mate

2024. 08. 27. 17:28 keltezéssel, Hanna Zbroszczyk (via star-cf-l Mailing 
List) írta:
> Dear Daniel,
>
> Thank you for submitting your presentation in time.
> Please find below my comments for you:
>
> S1: I suggest adding a one paragraph break between the tittle of your 
> presentation and your name and another one between your name and the name of 
> conference
>
> S2: I suggest to increase the size of your fonts and to add some content to the 
> right size (figure / graphic / whatever you find as useful)
>
> S4: I suggest to change = to /rightarrow in all, four places
>
> Lattice QCD works -> Lattice QCD calculations available
> You may add a bullet that we have cross-over transition here  (high 
> \sqrt{s_{NN}}, low \mu_B)
> Critical Point -> Critical Point? (As it’s not obvious whether it exists)
>
> S5: I suggest to add that this is the motivation of Au-Au heavy-ion collision 
> programs
> First stage -> High collision energies program: QGP properties
> Second stage -> Beam Energy Scan program I, II (including FXT):
> - onset on deconfinemet,
> - 1st order phase transition
> - Critical Point
>
> S14: Star Detector -> BES program
> You can show also here the QCD phase diagram from S5 (as it nicely illustrates 
> the coverage of the collision energies)
>
> S18: I suggest to remove the last bullet, but putting a reference that this 
> figure is taken from CPOD’23
> Increase font size of text please
>
> S19: as here you have only 2 bullets, I suggest to add them to the previous 
> slide
>
> S22: define \epsilon_F with a formula
> It will be good to add a conclusion from this slide, e.g. that no phase 
> transition indicated, and that these results are consistent with the scenario of 
> cross-over transition
> Increase the font size please
>
> S23: CP?-> critical behavior? (Since the location of the CP here is 
> questionable)
>
> S24: add reference to the figure and add references to EoS included in these 
> calculations
> Except sensitivity to the EoS, please mention that all results are closer to the 
> cross-over EoS.
> This figure is usually shown for identical particles that you can not 
> distinguish, I suggest you can use any other future that is applicable for all 
> particles species.
>
> S29: not contaminated -> less contaminated
> I suggest to remove the last bullet, instead to keep a reference to the figure: 
> CPOD’23 (as you did)
> Please separate a bit the text and the figure, they overall each other
>
> S30: plays -> play
> Pleae define all symbols mentioned here
> Instead of mentioning of properties  of resonances, you can mention that this 
> analysis helps to disctiguise whether a_0 is a tetraquark ro not (but here you 
> need to add title bit more details regarding extracting parameters from Diana)
> Add a reference to LL model
>
> S32, instead of the last sentence, please add a reference to the SQM’24 
> conference
>
> S33: Title: Femtoscopy - baryons -> Baryon femtoscopy
> Remove the repetition: Baryon femtoscopy
> Remove „generally"
> By measuring the CF’s with knows sources we can probe the interactions: -> 
> Assuming known source function, possible to probe interactions:
> Are they repel or attract themselves? -> Do the particle attract or repeal each 
> other?
>
> S34: Title: Femtoscopy - baryons -> Baryon femtoscopy
>
> S33, 34: you may consider adding some graphics
>
> S34: d_0,f_0 -> d_0, f_0 (add a space)
>
> S35: deuteron lambda -> deuteron-lambda
> General comment: if you use greek symbols, do this in your all slides, so lambda 
> -> \Lambda, etc..
> Rewrite the numerical values in the math mode, eg. 2.32^{+0.12}_{-0.11} fm
>
> S38:
> Chosen results… -> STAR highlights on fluctuations and correlations were shown
>
> I hope this helps, I will go through your slides once more when you implement my 
> comments,
>
> Thanks,
> Hanna
>
>
> Prof.*Hanna Zbroszczyk*,PhD, DSc, Eng.
> *E-mail*: hanna.zbroszczyk AT pw.edu.pl <mailto: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 AT star.bnl.gov w dniu 20.08.2024, o godz. 
> > 21:13:
> >
> > Dear star-cf-l AT lists.bnl.gov members,
> >
> > Daniel Wielanek (daniel.wielanek AT pw.edu.pl) has submitted a material for a
> > review, please have a look:
> > https://drupal.star.bnl.gov/STAR/node/68615
> >
> > Deadline: 2024-09-02
> > ---
> > If you have any problems with the review process, please contact
> > webmaster AT www.star.bnl.gov