STAR Flow, Chirality and Vorticity PWG

[Yicheng Feng <feng216 AT purdue.edu>]

Hi Yu,

Very nice slides!

I have a minor suggestion on your slide 15.

I noticed that a screenshot of my poster is attached on the lower right of that page, which, however, is an old version.

Due to the requirements and comments, I have switched to the 5-slides format with updates as follows:

https://drupal.star.bnl.gov/STAR/system/files/QM2022PosterSlides_YichengFeng_v26.pdf

To avoid possible confusion, I think it might be better to remove that screenshot.

Sincerely,

Yicheng

---

From: Hu, Yu <yuhu AT bnl.gov>
Sent: Sunday, April 3, 2022 2:50 AM
To: Star-cme-focusgroup-l AT lists.bnl.gov <star-cme-focusgroup-l AT lists.bnl.gov>; Star-fcv-l AT lists.bnl.gov <star-fcv-l AT lists.bnl.gov>
Cc: Wang, Fuqiang <fqwang AT purdue.edu>; Tribedy, Prithwish <ptribedy AT bnl.gov>; Yicheng Feng <feng216 AT purdue.edu>; zhiwanxu AT physics.ucla.edu <zhiwanxu AT physics.ucla.edu>; Tang, Aihong <aihong AT bnl.gov>; Evan Finch <levanfinch AT gmail.com>
Subject: Fw: STAR presentation by Yu Hu for Quark Matter 2022 submitted for review

 

Dear All,

Please find my slides for QM22 from the link below, thanks for the comments during my rehearsals.

https://drupal.star.bnl.gov/STAR/system/files/QM22_Apr07_YuHu_ChiralEffect_v7.pdf

I was trying to include all the comments I got over the weeks, my apologies if I miss any comments unintentionally. 

Further comments and suggestions are welcome!

Thank you.

Best,

Yu

---

From: Star-talks-l <star-talks-l-bounces AT lists.bnl.gov> on behalf of star-talks-l-request AT lists.bnl.gov <star-talks-l-request AT lists.bnl.gov>
Sent: Sunday, April 3, 2022 0:52
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Subject: Star-talks-l Digest, Vol 36, Issue 12

 

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Today's Topics:

   1. STAR presentation by Raghav Kunnawalkam Elayavalli        for Quark
      Matter 2022 submitted for review (webmaster AT star.bnl.gov)
   2. Re: STAR presentation by Benjamin Kimelman for Quark Matter
      2022 submitted for review (Rongrong Ma)
   3. STAR presentation by Rishabh Sharma for Quark Matter      2022 got
      commented by Grazyna Odyniec (webmaster AT star.bnl.gov)
   4. STAR presentation by Haojie Xu for Quark Matter 2022
      submitted for review (webmaster AT star.bnl.gov)
   5. STAR presentation by Ashik Ikbal Sheikh for Quark Matter 2022
      submitted for review (webmaster AT star.bnl.gov)
   6. STAR presentation by Gaoguo Yan for Quark Matter  2022
      submitted for review (webmaster AT star.bnl.gov)
   7. STAR presentation by Joseph Adams for Quark Matter        2022
      submitted for review (webmaster AT star.bnl.gov)
   8. D
   9. Re: STAR presentation by Yue-Hang Leung for Quark Matter 2022
      submitted for review (Rongrong Ma)
  10. STAR presentation by Prabhupada Dixit for Quark   Matter 2022
      got commented by Fuqiang Wang (webmaster AT star.bnl.gov)
  11. Re: STAR presentation by Zaochen Ye for Quark Matter 2022
      submitted for review (Rongrong Ma)
  12. Re: STAR presentation by Nihar Sahoo for Quark Matter 2022
      got commented by Sevil Salur (Nihar Sahoo)


----------------------------------------------------------------------

Message: 1
Date: Sat, 2 Apr 2022 20:04:31 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Raghav Kunnawalkam
        Elayavalli      for Quark Matter 2022 submitted for review
Message-ID: <202204030004.23304V16013705 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Raghav  Kunnawalkam Elayavalli (kunnawalkamraghav AT gmail.com) has submitted a 
material for a review, please have a look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Exploiting-jet-topological-differences-pp-and-AuAu-collisions-snn-20

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 2
Date: Sat, 2 Apr 2022 20:41:14 -0400
From: Rongrong Ma <marr AT rcf.rhic.bnl.gov>
To: star-talks-l AT lists.bnl.gov
Subject: Re: [Star-talks-l] STAR presentation by Benjamin Kimelman for
        Quark Matter 2022 submitted for review
Message-ID: <8D683883-C59C-4B6D-AE3E-C4490DEBF6FC AT rcf.rhic.bnl.gov>
Content-Type: text/plain;       charset=us-ascii

Hello Ben

I have some comments to your nice slides:

s3
- baryon density maximum -> maximum baryon density
- remove "Central" and add "in central collisions" before "have been measured"
- indicate a constant rapidity loss

s6
- centrality -> centrality bins
- add definition of Z above the PID figure

s7
- make the last bullet a sub-bullet of the second bullet

s8
- low m_T-m_0 acceptance -> low m_T-m_0 reach

s9
- Just to check: is it true that proton is extracted based on m2 while pion and kaon on 1/beta?
- Proton spectra described well near midrapidity -> Proton spectra near midrapidity described well

s10
- from Blast-wave fit
- Left figure: x-axis and y-axis titles are too small to see
- highest -> largest
- shows geometric effect of size of overlap region -> shows the size of overlapping region
- With large rapidity acceptance, will -> Will

s11
- obtained from spectra and integration of fits -> obtained from spectrum integration and fits

s12
- obtained from spectra and integration of fits -> obtained from spectrum integration and fits
- a lesser degree of -> less

s14
- are very susceptible -> are susceptible
- Right figure: legend is very hard to see

s15
- Title: "Correlation of Coulomb Potential with Proton Yield"
- smaller -> less
- assumptions -> expectations
- as spherical potential -> as a spherical source

s16
- RHIC -> STAR BES-I
- shows importance of -> is affected by
- Do you mean changes in mu_b will change mu_s and suppress K-/K+ ratio? If so, could you elaborate? Do we have any measurement of mu_B and mu_S at 3 GeV?

s17
- Protons rapidity density -> Proton rapidity density
- each participating nucleon has -> each participating nucleon takes part

s20
- Full rapidity -> Rapidity
- from stopped baryons -> from stopped protons
- a non-spherical potential from stopped protons -> a non-spherical source
- shows the importance of -> is affected by

s23
- are minimal effect -> of minimal effect

s25
- indicates -> indicate


Best
Rongrong

> On Apr 2, 2022, at 12:02 PM, webmaster--- via Star-talks-l <star-talks-l AT lists.bnl.gov> wrote:
>
> Dear star-talks-l AT lists.bnl.gov members,
>
> Benjamin Kimelman (BKIMELMAN AT UCDAVIS.EDU ) has submitted a material for a 
> review, please have a look:
> https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Baryon-Stopping-and-Associated-Production-Mesons-AuAu-Collisions-s-0
>
> ---
> If you have any problems with the review process, please contact 
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-talks-l mailing list
> Star-talks-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-talks-l



------------------------------

Message: 3
Date: Sat, 2 Apr 2022 21:33:47 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Rishabh Sharma for Quark
        Matter  2022 got commented by Grazyna Odyniec
Message-ID: <202204030133.2331Xlor022625 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Grazyna Odyniec ( g_odyniec AT lbl.gov ) has commented on a material originally 
submitted by Rishabh Sharma ( rishabhsharma AT students.iisertirupati.ac.in ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Elliptic-flow-light-nuclei-AuAu-collisions-%E2%88%9AsNN-27-and-544-GeV

Comment:
p.s. Rishabh, I see your point. So, you do not need to do any changes. Very 
well prepared poster.

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 4
Date: Sat, 2 Apr 2022 23:11:01 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Haojie Xu for Quark
        Matter 2022     submitted for review
Message-ID: <202204030311.2333B142031965 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Haojie Xu (haojiexu AT zjhu.edu.cn) has submitted a material for a review, 
please have a look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Constraints-neutron-skin-thickness-and-nuclear-deformations-using--0

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 5
Date: Sat, 2 Apr 2022 23:11:43 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Ashik Ikbal Sheikh for
        Quark   Matter 2022 submitted for review
Message-ID: <202204030311.2333BhgA032089 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Ashik Ikbal Sheikh (ashikhep AT gmail.com) has submitted a material for a 
review, please have a look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/splitting-directed-flow-identified-light-hadrons-pi-K-and-p-and-st-0

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 6
Date: Sat, 2 Apr 2022 23:11:37 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Gaoguo Yan for Quark
        Matter  2022 submitted for review
Message-ID: <202204030311.2333BbHA032058 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Gaoguo Yan (gaoguo.yan AT Outlook.com) has submitted a material for a review, 
please have a look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Probe-initial-and-final-state-effects-heavy-ion-collisions-STAR-expe

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 7
Date: Sat, 2 Apr 2022 23:11:49 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Joseph Adams for Quark
        Matter  2022 submitted for review
Message-ID: <202204030311.2333Bnfj032122 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Joseph Adams (adams.1940 AT buckeyemail.osu.edu) has submitted a material for a 
review, please have a look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Measurements-hyperon-polarization-heavy-ion-collisions-%E2%88%9AsNN-3-%E2%88%92200-0

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 8
Date: Sat, 2 Apr 2022 23:11:56 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Yu Hu for Quark Matter
        2022    submitted for review
Message-ID: <202204030311.2333BuxS032156 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Yu Hu (yuhu AT bnl.gov) has submitted a material for a review, please have a 
look:
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Search-chiral-effect-using-isobar-collisions-and-BES-II-data-STAR-0

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 9
Date: Sat, 2 Apr 2022 23:23:26 -0400
From: Rongrong Ma <marr AT rcf.rhic.bnl.gov>
To: star-talks-l AT lists.bnl.gov
Subject: Re: [Star-talks-l] STAR presentation by Yue-Hang Leung for
        Quark Matter 2022 submitted for review
Message-ID: <A8C9E4E2-AD73-4035-9469-97A157727681 AT rcf.rhic.bnl.gov>
Content-Type: text/plain;       charset=us-ascii

Hello Yue-Hang

I have some comments to your nice slides:

s2
- are not well understood -> is not well understood

s3
- If not done yet, please double check your numbers with Dan's table: https://drupal.star.bnl.gov/STAR/system/files/BES-IIFXT_event_counts_fromDan.pdf
- in heavy-ion collision experiments -> in heavy-ion experiments

s4
- Backgrounds -> Background
- rotated pion tracks -> rotating pion tracks

s8
- For the bullet "Hypernuclei deviate from exponential trend", are you referring to H3L and H4L? In terms of significance, deviation of 4He is larger than H3L, but this is not mentioned

s9
- perfectly -> quantitatively
- Why put Thermal model as a separate bullet, while others as sub-bullets? All the models are discussed except for JAM. why?

s10
- remain -> remains
- B_A of light -> B_A of light nuclei

s11
- remove "Au+Au collisions"
- Right figure
-- remove "Data"
-- Increase the size of legend of the label "STAR preliminary"

s12
- Does not depend -> Does not depend on
- predict different models -> predict different trends
- remove the comma after "dynamical stage"
- describe the S3 data well -> describe the S3 data quantitatively

s13
- seems like the resolution for the left figure is poorer than the right one

s14
- are not the final calibrations -> are not with the final calibrations
- remove ", hence results and conclusions may change after final calibrations are preformed". I think this half sentence is the implication of the first half sentence. We do not need to write it down on the slide, which casts doubts on the results shown.

s15
- Stronger -> Strong
- in tension with thermal model -> in tension with model calculations (coalescence model calculations do not describe data either)

Best
Rongrong

> On Apr 2, 2022, at 12:02 PM, webmaster--- via Star-talks-l <star-talks-l AT lists.bnl.gov> wrote:
>
> Dear star-talks-l AT lists.bnl.gov members,
>
> Yue-Hang Leung (YHLeung AT lbl.gov) has submitted a material for a review, 
> please have a look:
> https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Recent-Hypernuclei-Measurements-High-Baryon-Density-Region-STAR-Expe
>
> ---
> If you have any problems with the review process, please contact 
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-talks-l mailing list
> Star-talks-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-talks-l



------------------------------

Message: 10
Date: Sat, 2 Apr 2022 23:41:07 -0400
From: webmaster AT star.bnl.gov
To: star-talks-l AT lists.bnl.gov
Subject: [Star-talks-l] STAR presentation by Prabhupada Dixit for
        Quark   Matter 2022 got commented by Fuqiang Wang
Message-ID: <202204030341.2333f7Q2002270 AT sun.star.bnl.gov>

Dear star-talks-l AT lists.bnl.gov members,

Fuqiang Wang ( fqwang AT purdue.edu ) has commented on a material originally 
submitted by Prabhupada Dixit ( prabhupadad AT iiserbpr.ac.in ) at
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Elliptic-flow-strange-and-multi-strange-hadrons-AuAu-collisions-%E2%88%9AsNN

Comment:
Prabhupada,

I was asked to review your poster. Please find my comments below.

Number the slides.

Add author names (presumably STAR) in refs.

p.2
make any conclusion -> make firm conclusion

p.3:
remove the extra open space at bottom of the second text box.

p.4
Axis labels and values are too small. The texts on the plots are also too 
small. Y-label -> "Counts/MeV".
Info is needed on whether the phi v2 is done with full event or sub-events. 
If full event, then your resolution correction would be incorrect.
The text is cut off at bottom of the page.

p.5
high pT reach -> has a higher pT reach

---
If you have any problems with the review process, please contact 
webmaster AT www.star.bnl.gov


------------------------------

Message: 11
Date: Sun, 3 Apr 2022 00:25:46 -0400
From: Rongrong Ma <marr AT rcf.rhic.bnl.gov>
To: star-talks-l AT lists.bnl.gov
Subject: Re: [Star-talks-l] STAR presentation by Zaochen Ye for Quark
        Matter 2022 submitted for review
Message-ID: <D4E9840F-B04A-4407-A9BB-E0DB5405B78C AT rcf.rhic.bnl.gov>
Content-Type: text/plain;       charset=us-ascii

Hello Zaochen

I have some comments to your nice slides:

s2
- Temperature, as one of key properties of medium, still poorly known

s4-5
- remove "original"

s8-9
- Physics background -> Physical background (three places)
- be determined in -> be determined using

s11-12
- 27 GeV Au+Au -> 27 GeV Au+Au collisions
- T is similar between STAR and NA60 despite

s13-15
- 54 GeV -> 54.4 GeV
- T are higher ->T is higher
- indicate that the emission are -> indicating that emission is

s18
- I suggest to add mass ranges for IMR and LMR in the legend of the figure. Otherwise, it is hard to know without context.
- are close -> is close
- there are two empty spaces before "temperature (T_pc)"
- are higher than what in LMR -> is higher than that in LMR

s19-21
- you have compared to T_pc all along in your slides. why switch to T_ch here?
- phase transition region -> phase transition

s22-23
- collision systems -> collision system

s24
- Second bullet: "Search for significant enhancement in thermal dilepton yield, which could point to a potential critical point."

s26
- please update
- figures need "STAR Preliminary" label

s28
- Add content or remove it

Best
Rongrong


> On Apr 2, 2022, at 1:25 PM, webmaster--- via Star-talks-l <star-talks-l AT lists.bnl.gov> wrote:
>
> Dear star-talks-l AT lists.bnl.gov members,
>
> Zaochen Ye (zaochen.ye.2017 AT gmail.com) has submitted a material for a review, 
> please have a look:
> https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Temperature-measurement-thermal-dileptons-AuAu-collisions-27-and-5-0
>
> ---
> If you have any problems with the review process, please contact 
> webmaster AT www.star.bnl.gov
> _______________________________________________
> Star-talks-l mailing list
> Star-talks-l AT lists.bnl.gov
> https://lists.bnl.gov/mailman/listinfo/star-talks-l



------------------------------

Message: 12
Date: Sun, 03 Apr 2022 10:22:51 +0530
From: Nihar Sahoo <nihar AT rcf.rhic.bnl.gov>
To: webmaster AT star.bnl.gov, star-talks-l AT lists.bnl.gov
Subject: Re: [Star-talks-l] STAR presentation by Nihar Sahoo for Quark
        Matter 2022 got commented by Sevil Salur
Message-ID: <47e0af2236196e5b9b3b5be0e14e7e79 AT rcf.rhic.bnl.gov>
Content-Type: text/plain; charset=US-ASCII; format=flowed

Dear Sevil,

the same version v5.
https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Search-large-angle-jet-deflection-using-semi-inclusive-direct-photon

> The Pythia curves in slide 4 are dashed but the legend in the plots are
> solid. Could you please fix that?
Now fixed.

> What is the reason of crossover for these Pythia curves around 2.5?
Possible reasons could be due to i) pi0 phi (trigger phi which may not
exactly be the same as the near side jet) vs photon trigger phi and/or,
ii) recoil jet pT spectral shapes are different for pi0 and gamma
trigger.
  When we will do both pi0+jet and gamma+jet delta phi measurement using
our upcoming high lumi pp data, then we can study on it in data.
Thank you for this good question.

Regards,
Nihar





On 2022-04-02 23:56, webmaster--- via Star-talks-l wrote:
> Dear star-talks-l AT lists.bnl.gov members,
>
> Sevil Salur ( salur AT physics.rutgers.edu ) has commented on a material
> originally submitted by Nihar Sahoo ( nihar AT rcf.rhic.bnl.gov ) at
> https://drupal.star.bnl.gov/STAR/presentations/Quark-Matter-2022/Search-large-angle-jet-deflection-using-semi-inclusive-direct-photon
>
> Comment:
> Thank you Nihar. 1 more remaining issue that I see and one question for
> my
> own education.
> The Pythia curves in slide 4 are dashed but the legend in the plots are
> solid. Could you please fix that?
> What is the reason of crossover for these Pythia curves around 2.5?
>
>
> ---
> If you have any problems with the review process, please contact
> webmaster AT www.star.bnl.gov
> _______________________________________________
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