star-fcv-l AT lists.bnl.gov
Subject: STAR Flow, Chirality and Vorticity PWG
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- From: LikeLiu <likeliu AT mails.ccnu.edu.cn>
- To: star-fcv-l AT lists.bnl.gov
- Cc: Nu Xu <nxu AT lbl.gov>, Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>, shiss <shiss AT mail.ccnu.edu.cn>
- Subject: Re: [[Star-fcv-l] ] Paper draft of FXT PID v2
- Date: Sun, 5 Jan 2025 13:58:29 +0100
Dear FCV colleagues,
Apologies for the inconvenience!
This email was delivered to the wrong mailing list and was intended for the
PA internal group.
Please ignore that.
Thanks and best regards,
Li-Ke
> On Jan 5, 2025, at 12:46, LikeLiu (via star-fcv-l Mailing List)
> <star-fcv-l AT lists.bnl.gov> wrote:
>
> Hi Nu and all,
>
> Thanks for your suggestions!
>
> The paper draft of FXT PID v2 has been modified accordingly, mainly on the
> figures and their corresponding textual descriptions.
> Also, for the summary part,
> "suggest an increasing significance of partonic interactions in collisions
> at sNN ≥ 3.5 GeV" -> "4.5 GeV”,
> as a conservative statement, the scaling at 3.5 and 3.9 GeV is not
> explicitly stated.
>
> The model calculations are ongoing, to reduce the v2pt statistical
> fluctuation, especially for 3 GeV.
>
> The diff version has been attached, please let me know if you have any
> comments.
>
> best regards,
> Li-Ke
>
> <paper_draft_diff.pdf>
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[[Star-fcv-l] ] Paper draft of FXT PID v2,
LikeLiu, 01/05/2025
- Re: [[Star-fcv-l] ] Paper draft of FXT PID v2, LikeLiu, 01/05/2025
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