Azimuthal anisotropy measurement of (multi-)strange hadrons in Au+Au collisions at $\sqrt{s_{\text{NN}}}$ = 54.4 GeV
STAR Collaboration: M. S. Abdallah, B. E. Aboona, J. Adam, L., Adamczyk, J. R. Adams, J. K. Adkins, I. Aggarwal, M. M. Aggarwal, Z. Ahammed,, D. M. Anderson, E. C. Aschenauer, J. Atchison, V. Bairathi, W. Baker, J. G., Ball Cap, K. Barish, R. Bellwied, P. Bhagat, A. Bhasin

TL;DR
This paper measures azimuthal anisotropies ($v_2$ and $v_3$) of various strange hadrons in Au+Au collisions at 54.4 GeV, revealing insights into the collective behavior and energy dependence of the medium created.
Contribution
It provides the first detailed measurement of $v_2$ and $v_3$ for multiple strange hadrons at this energy, highlighting the energy dependence and quark number scaling in heavy-ion collisions.
Findings
$v_3$ is more sensitive to energy changes than $v_2$.
Quark number scaling holds for $v_2$ within 10%.
Differences observed between baryons and anti-baryons in flow measurements.
Abstract
Azimuthal anisotropy of produced particles is one of the most important observables used to access the collective properties of the expanding medium created in relativistic heavy-ion collisions. In this paper, we present second () and third () order azimuthal anisotropies of , , , and at mid-rapidity (1) in Au+Au collisions at = 54.4 GeV measured by the STAR detector. The and are measured as a function of transverse momentum and centrality. Their energy dependence is also studied. is found to be more sensitive to the change in the center-of-mass energy than . Scaling by constituent quark number is found to hold for within 10%. This observation could be evidence for the development of partonic collectivity in 54.4 GeV Au+Au collisions. Differences in and…
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