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: Nu Xu <nxu AT lbl.gov>, Sooraj Radhakrishnan <skradhakrishnan AT lbl.gov>, shiss <shiss AT mail.ccnu.edu.cn>, Xin Dong <xdong AT lbl.gov>
- Cc: Xing Wu <star-fcv-l AT lists.bnl.gov>, Zuowen Liu <liuzw AT mails.ccnu.edu.cn>, gpwang <gpwang AT mails.ccnu.edu.cn>
- Subject: [[Star-fcv-l] ] Paper draft of FXT PID v2
- Date: Sun, 5 Jan 2025 12:46:44 +0100
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
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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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