star-fcv-l AT lists.bnl.gov
Subject: STAR Flow, Chirality and Vorticity PWG
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[Star-fcv-l] suggestion to your photo-nuclear flow measurement.
- From: Jiangyong Jia <jiangyong.jia AT stonybrook.edu>
- To: Prithwish Tribedy <prithwish2005 AT gmail.com>, star-fcv-l AT lists.bnl.gov
- Subject: [Star-fcv-l] suggestion to your photo-nuclear flow measurement.
- Date: Wed, 12 May 2021 11:43:16 -0400
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
-
[Star-fcv-l] suggestion to your photo-nuclear flow measurement.,
Jiangyong Jia, 05/12/2021
- Re: [Star-fcv-l] suggestion to your photo-nuclear flow measurement., Prithwish Tribedy, 05/12/2021
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