STAR Correlations and Fluctuations PWG

[Mate Csanad <csanad AT bnl.gov>]

Dear Daniel,

Thanks a lot for incorporating the results I mentioned, very kind of you.

Best regards,
Mate

PS: Let me just send one more minor comment relating to it, either for 
mentioning it on the slide or in words, or just FYI (in case questions come up 
during or after the talk): the non-constant trend of alpha(sqrt(sNN)) also means 
that the radius parameter's trend vs sqrt(sNN) is modified, compared to the 
alpha=2 case.


2024. 08. 29. 13:49 keltezéssel, Wielanek Daniel (via star-cf-l Mailing List) 
írta:
> Dear All,
>
> I've uploaded never version of my presentation.
>
>
> Pozdrawiam/Best regards,
>
> Daniel Wielanek
>
> --------------------------------------------------------------------------------
> *Od:* star-cf-l-request AT lists.bnl.gov <star-cf-l-request AT lists.bnl.gov> w 
> imieniu użytkownika Mate Csanad <csanad AT bnl.gov>
> *Wysłane:* środa, 28 sierpnia 2024 10:04:57
> *Do:* star-cf-l AT lists.bnl.gov
> *Temat:* Re: [[Star-cf-l] ] STAR presentation by Daniel Wielanek for NTHEP-2024 
> submitted for review
> 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
>  
> <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/blog/kincses/Pion-interferometry-Levy-stable-sources-STAR-FXT-energies>
> https://drupal.star.bnl.gov/STAR/system/files/alpha0_sqrts_fxt.pdf 
> <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/blog/kincses/Two-particle-interferometry-Levy-stable-sources-sqrtsNN-200-GeV-AuAu-collisions>
> https://drupal.star.bnl.gov/STAR/system/files/alpha0_npart.pdf 
> <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 
> > <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 
> <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