STAR Flow, Chirality and Vorticity PWG

[niseem <niseem AT rcf.rhic.bnl.gov>]

Hi Jiangyong,

Please find the updated abstract at this link,


https://drupal.star.bnl.gov/STAR/system/files/Niseem_IS1_21_0.pdf


Thanks,
Niseem


On 2020-09-21 06:45, Jiangyong Jia via Star-fcv-l wrote:
> Hi, Niseem,
>
> The abstract looks very good. My only suggestion is to try align the
> physics better with initial state of the Heavy ion collisions.
>
> Right now you mainly talk about the final state, but I believe jet
> tomography also constrains initial geometry (via the scaling 
> relations) 
>
> You might want to mention something about the scaling aspect and what
> one can learn by comparing with LHC.
>
> Other than this, I sign off.
>
> Jiangyong
>
> > On 2020-09-15 20:19, niseem via Star-fcv-l wrote:
> > > Dear Prithwish and ShinIchi,
> > >
> > > Please find the updated abstract at this link,
> > >
> > > https://drupal.star.bnl.gov/STAR/system/files/Niseem_IS1_21_0.pdf
> > >
> > >
> > > For your comments,
> > >
> > > (1) ShinIchi comments,
> > >
> > > 1- I thought you would be also focusing various different ways of
> > > non-flow subtractions, which you do not mention here at all, while 
> > > you
> > > do mention about the different ways of centrality definition only for
> > > UU?
> > > > > There is no different centrality definition I rephrased the
> > > > > sentence to give a better understanding
> > >
> > > 2- I would say you might like to focus on the most important
> > > topics/point that you would like to
> > > present, like energy dependence, system size dependence, centrality
> > > determination and/or non-flow subtraction etc…
> > > > > Abstract updated
> > >
> > > 3-some more words on how this measurement would be related to the
> > > small system vn? where we do not see clear quenching effect at least
> > > on RAA...
> > > > > I agree with you, p+Au got removed
> > >
> > > (2) Prithwish comments
> > > i- Comments on the abstract :
> > > -using the STAR experiment —> from the STAR experiment
> > > -Au+At at 200 —> Au+Au at 200
> > > -“The measurements scaling features”   sounds a bit ambiguous, pls. 
> > > be
> > > specific and revise this sentence.
> > > -constraints for—> constraints on
> > > -upcoming O+O and p+Au runs at RHIC—>anticipated O+O run at RHIC in
> > > the year 2021
> > > > > All comments are considered
> > >
> > >
> > > -Do you want to mention p+Au here ? A p+Au run at STAR/RHIC is going
> > > to take a while, also we already have p+Au data which might create a
> > > confusion.
> > > > > I agree with you, p+Au got removed
> > >
> > > -Along the line of ShinIchi's comments: adding a line on the novel
> > > subtraction method that you use can strengthen your abstract, 
> > > however,
> > > I leave this to you.
> > > > > I agree with you, the sentence has been updated
> > >
> > >
> > > ii-Comments on analysis and preliminary approval:
> > > 1. We find out what would be our policy on promising isobar data in 
> > > an
> > > abstract. If PAC’s recommendation on not showing isobar data at any
> > > conference was specific to CME analysis, this won’t be a problem. 
> > > But,
> > > you don't have to worry -- we will clarify this from management 
> > > before
> > > the abstract is submitted.
> > >
> > > > > Please note that the meeting will be in January and we started the
> > > > > production I’m hoping to have final results before that. Also, as
> > > > > you stated these only flow measurements.
> > >
> > > 2. In your last presentation you mentioned about ongoing 27 GeV
> > > analysis :
> > > https://www.star.bnl.gov/protected/bulkcorr/niseem/pwg_2020/High_PT_3.pdf
> > >
> > > However, in this abstract you mentioned about 54 GeV. Do you have
> > > plans to show/include both 27 and 54 GeV ?
> > >
> > > > > 27 GeV added to the abstract I’m working on it now.
> > >
> > >
> > >
> > > Thanks,
> > > Niseem
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