PaperFlowindAuandOORun21
Title: Measurements of Multiplicity Dependent v2 and v3 in O+O and d+Au Collisions
PA:
Shengli Huang(1), Jinhui Chen(2), Roy Lacey(1), Jiangyong Jia(1), Prithwish Tribedy(3), Zaining Wang(2), Zhengxi Yan(1), ChunjianZhang(2)
1.SBU 2.Fudan 3. BNL
Analysis note:
https://drupal.star.bnl.gov/STAR/starnotes/private/PSN0863
paper draft:
1)PWGC: drupal.star.bnl.gov/STAR/system/files/OOPaper-7.pdf
2)GPC Request: https://drupal.star.bnl.gov/STAR/system/files/OOPaper-3.pdf
Target Journal: PRL
PWGC review:
drupal.star.bnl.gov/STAR/blog/slhuang/PWGC-Slide-OO-and-dAu-flow-paper
PWG presentation:
•For O+O:
•https://drupal.star.bnl.gov/STAR/blog/slhuang/OO-Glauber-Update
•https://drupal.star.bnl.gov/STAR/blog/slhuang/di-hadron-correlation-OO
•https://drupal.star.bnl.gov/STAR/system/files/OOnewpreliminary.pdf
•https://drupal.star.bnl.gov/STAR/blog/slhuang/Qm2023-preliminary
•https://drupal.star.bnl.gov/STAR/system/files/OOPWGMay-17-2023-Shengli.pdf
•https://drupal.star.bnl.gov/STAR/system/files/OOPWGMay10-2023-Shengli.pdf
•For d+Au:
•https://drupal.star.bnl.gov/STAR/blog/slhuang/PWGJune112024
•https://drupal.star.bnl.gov/STAR/blog/slhuang/PWGJun182024
Abstract:
In this paper, the elliptic and triangular flow harmonics ($v_2$ and $v_3$) are measured as a function of multiplicity in first-ever $^{16}$O+$^{16}$O and $d$+Au collisions at $\sqrtsNN$ = 200 GeV. The elliptic flow harmonic ($v_2\{2\}$ and $v_{2}\{4\}$), obtained via two- and four-particle correlations, respectively, exhibit a strong system dependence, whereas the triangular flow harmonic ($v_{3}\{2\}$) is nearly system-independent. The ratio $v_{n}\{2\}/\varepsilon_{n}\{2\}$ is found system-independent for eccentricity $\varepsilon_{n}\{2\}$ with sub-nucleon fluctuations. Moreover, $v_{2}\{4\}/v_{2}\{2\}$ is consistent with $\varepsilon_{2}\{4\}/\varepsilon_{2}\{2\}$ in central $d$+Au collisions, while is lower than $\varepsilon_{2}\{4\}/\varepsilon_{2}\{2\}$ in central $^{16}$O+$^{16}$O collisions. These findings provide critical insights into the origin of collectivity in small systems and enhance our understanding of nucleon-nucleon correlations and alpha cluster structure in high-energy nuclear collisions.
Figure 1:
The $c_n\{2\}$ values (for $n=2,3$) as a function of charged-particle multiplicity ($N_\text{ch}$) in \oo and \dau collisions at $\sqrt{s_{NN}}$ = 200 GeV. Left panels (a,c) show results before nonflow subtraction, while right panels (b,d) present values after nonflow subtraction using the $c_1$ method. Substantial nonflow contributions are evident at low multiplicities. After subtraction, $c_2\{2\}$ in \dau increases with $N_\text{ch}$, while in \oo it shows a weaker dependence, consistent with the spherical geometry of the $^{16}$O nucleus. In contrast, $c_3\{2\}$ values remain similar between the two systems after subtraction, indicating that triangularity is primarily driven by initial-state fluctuations.
Figure 2:
Panels (a) and (d) show the $v_n\{2\}$ values (for $n=2,3$) after nonflow subtraction as a function of $N_{\text{ch}}$ for \dau and \oo collisions. Panels (b), (c), (e), and (f) present the ratios $v_n\{2\}/\varepsilon_n\{2\}$, where $\varepsilon_n\{2\}$ is calculated from Glauber model simulations with and without sub-nucleon fluctuations, for $n=2$ and $n=3$, respectively. The results indicate that the linear scaling relation between flow coefficients and initial eccentricities holds for both $v_2$ and $v_3$, with notably better agreement when sub-nucleon fluctuations are included, especially for $v_3$.
Figure3:
Panels (a) and (b) show the $v_2\{2\}(\rm{subtr.})$ and $v_2\{4\}$ values as a function of $N_{\rm{ch}}$ in \dau and \oo collisions. (c) and (d) show the ratio $v_2\{4\}/v_2\{2\}(\rm{subtr.})$ compared with the corresponding initial-state eccentricity ratio $\varepsilon_2\{4\}/\varepsilon_2\{2\}$ from PHOBOS Glauber model including sub-nucleon fluctuations. The $^{16}$O configurations is based on NLEFT models that include nucleon-nucleon correlations and possible $\alpha$-clustering. In \dau collisions, the ratio remains near 0.9 with weak multiplicity dependence, consistent with the deuteron-driven initial geometry. In contrast, \oo collisions exhibit a significant decrease in $v_2\{4\}/v_2\{2\}(\rm{subtr.})$ at high $N_{\rm{ch}}$, suggesting enhanced flow fluctuations not fully captured by current initial-state models.
Summary:
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