4–10 Apr 2022
Auditorium Maximum UJ
Europe/Warsaw timezone
Proceedings submission deadline extended to September 11, 2022

Probing the nuclear deformation effects in Au+Au and U+U collisions from STAR experiment

6 Apr 2022, 18:34
4m
Poster Initial state physics and approach to thermal equilibrium Poster Session 2 T01

Speaker

Jiangyong Jia (Stony Brook University (US))

Description

Nuclear deformation is an ubiqutous phenomenon for most atomic nuclei, reflecting collective motion induced by interaction between valance nucleons and shell structure. In most cases, the deformation has a quadrupole shape that is charactorized by overall strength $\beta_2$ and triaxiality $\gamma$ (prolate $\gamma=0$, obolate $\gamma=\pi/3$ and triaxial otherwise). Collisions of deformed nuclei lead to large shape and size fluctuations in the initial state geometry, which after collective expansion, lead to enhanced fluctuation of elliptic flow $v_2$ and event-by-event mean transverse momentum $[p_{\mathrm{T}}]$. Therefore, detailed study of the $v_2$, and $[p_{\mathrm{T}}]$ and correlations beween them can constrain the deformation parameters $(\beta_2,\gamma)$. A comparion of $(\beta_2,\gamma)$ with those measured from nuclear structure experiment could then be used to constrain the hydrodynamic responses of heavy-ion collisions. In this poster, we present results of $v_2$, $[p_{\mathrm{T}}]$ fluctuations and $v_2^2-[p_{\mathrm{T}}]$ correlation for harmonics $n=2,3,4$ in modestly-deformed $^{197}$Au+$^{197}$Au collisions at 200 GeV and highly-deformed $^{238}$U+$^{238}$U collisions at 193 GeV. Significant differences for mean, variance $c_2$ and skewness $c_3$ of $[p_{\mathrm{T}}]$ fluctuations, are observed between the two systems as a function of centrality. The $v_2^2-[p_{\mathrm{T}}]$ results remain positive over the full centrality in Au+Au collisions, while they change sign in 0-5\% central U+U collisions. The ratio of $v_2$ and $c_2$ between U+U and Au+Au in ultra-central collisions (UCC) are used to constrain the value of $\beta_2$, which leads to an estimate of $\beta_{2Au}\sim0.18$. On the other hand, the value of $\gamma$ can be constrained from the ratios of $v_2^2-[p_{\mathrm{T}}]$ and $c_3$ between U+U and Au+Au. The enhancement of $c_3$ and the suppression of $v_2^2-[p_{\mathrm{T}}]$ in UCC confirm that Uranum is prolate deformed with $\gamma\sim0$. Comparison with state-of-art model calculations is discussed.

Authors

Jiangyong Jia (Stony Brook University (US)) STAR Collaboration

Presentation materials