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star-fcv-l - Re: [Star-fcv-l] today's PWG discussion on nonflow in U/Au paper

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Subject: STAR Flow, Chirality and Vorticity PWG

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  • From: subhash <subhash AT rcf.rhic.bnl.gov>
  • To: "STAR Flow, Chirality and Vorticity PWG" <star-fcv-l AT lists.bnl.gov>
  • Subject: Re: [Star-fcv-l] today's PWG discussion on nonflow in U/Au paper
  • Date: Thu, 25 Jan 2024 13:28:20 +0800

Dear Sergei,

Thank you for your email. While I acknowledge that the meeting could have been more productive, I believe that valuable points were raised by both groups, and there was a mutual understanding, despite some disagreements. I see this as a positive starting point. The nonflow is not only important to this specific analysis but holds general relevance across various other analyses as well. I think we should organize more focused discussions on nonflow in the coming days within our working group and beyond.

Thanks and regards,
Subhash



On 2024-01-25 12:21 PM, Sergei Voloshin via Star-fcv-l wrote:
Hi all,

There was a rather interesting discussion at today's meeting (thanks
to Fuqiang and Jianyong for preparing the presentations!), though I
had to leave after 2.5 hours... I have a few comments (not in any
particular order) below.

- The discussion could be much more productive, if somebody would
chair the session. It could be better if during the presentation only
short questions were allowed, and longer discussions delayed for
later. Especially when it is clear that people agree to disagree (but
not only).

- I agree with Fuqiang that a clear estimate of nonflow should be
made, e.g.for reported v_2, but for other quantities as well.

- For the nonlfow estimate HIJING can be used, though the data might
be preferable. From my point of view, using pp data would be the best
if used <uQ*>, AA-pp method. One can use peripheral collisions, as
tried by Jianyong, including even the scaling presented (though again
much better would be <UQ*> approach). Even better would be to compare
different estimates.

- The statements were made that it is not really possible to define
nonflow. Very strange - what do we report then? Let us define what we
want to measure, e.g. the correlation with the participant plane
(another possibility would be the correlation with the reaction
plane), then what is extra in e.g. measurements with two-particle
correlations would be non-flow.

- Again, if we report v_2, let us define what we mean by that and
report a realistic estimate of "non-flow" in that measurement. The
values around a few percent for (ultra)central collisions look very
unrealistic, to say the least.

- The paper mentions "standard" and subevent methods, but neither is
defined (unless I missed that).

- The effect of nonflow for AuAu and UU collisions is likely rather
similar, and the effect on the ratios should be calculated taking this
into account. (This is probably what Jianyong meant by "difference" in
nonflow)

- Statement that "surface emission" is not flow, is incorrect (unless
I misunderstood what was said) at least for the definition of flow I
used above, but it indeed depends on the definition of flow.

- The statement that quenching reduces nonflow is (likely) incorrect,
in fact it could increase it. The result of quenching is that instead
of one high(er) pt particle we have several low pt. But those still
have azimuthal angle strongly correlated with "jet" - then the
contribution to nonflow would only increase.

- "hot spots" effect (mentioned in relation to 2-particle CF) is
non-flow (again I could have misunderstood it) -- this is incorrect.
More exactly it again depends on the definition of flow used. If it is
correlations relative to the reaction plane, the statement is correct,
if it is relative to the participant plane, the hot spots effect is
already included in geometry/flow plane fluctuations.

Best regards,
Sergei

-

--

======================================
Sergei A. Voloshin

Distinguished Professor,

Department of Physics and Astronomy,
Wayne State University,
666 W. Hancock, Detroit, Michigan, 48201
e-mail: sergei.voloshin AT wayne.edu
======================================
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