STAR Flow, Chirality and Vorticity PWG

[Prithwish Tribedy <ptribedy AT rcf.rhic.bnl.gov>]

Thanks a lot for the suggestions. We'll see what we can do. Please note 
that d+Au and p+Au data are from a different energy (200 GeV). We're 
studying Au+Au 54 GeV data which is more like 2(\gamma)+27(Au) 
collisions.

Best,
Prithwish


On 2021-05-12 11:43, Jiangyong Jia via Star-fcv-l wrote:
> My suggested checks for your interesting analysis
>
> 1) hadronic event generator HIJING/uRQMD and look at the Gap
> distribution with and with out your cut in ZDC and BBC
>
> This will allow to look at the background contamination
>
> 2) RUN Pythia gamma-p and DPMjet gamma-A collisions and see how they
> survives3)  your analysis cut and any possible biases on your 
> distributions
>
> 3) produce similar distribution for dAu for which the gamma-Au
> cross-section should be much smaller (almost negliable), check what
> kinds of distribution you get after applying your cut
>
> 4) compare your v2 signal with pAu and dAu from shengli. (ATLAS results
> show that the v2 for gamma-A is much smaller than pPb).
>
> Jiangyong
>
>
>
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