Speaker
Description
Anisotropic flow parameters $(v_{n})$ are important observables as they provide insight into the collective expansion and transport properties of the medium produced in relativistic heavy-ion collisions. Among these parameters, directed flow ($v_1$) describes the collective sideward motion of produced particles in heavy-ion collisions. It is an important probe to study the in-medium dynamics as it is predicted to be sensitive to the equation of state (EoS) of the produced medium. Minimum in the slope of directed flow ($dv_1/dy$) as a function of collision energy has been proposed as a signature of the first-order phase transition between hadronic matter and Quark-Gluon Plasma (QGP). Triangular flow $(v_3)$ typically arises from the initial state fluctuations and is expected to be uncorrelated with the reaction plane. However, recent measurements at lower collision energies (higher baryon chemical potential ($\mu_{B}$)) of $\sqrt{s_{NN}}$ = 2.4 and 3 GeV, show a correlation between $v_3$ and the first-order event plane angle ($\Psi_{1}$).
In this presentation, we will report the measurements of $\Psi_{1}$ correlated $v_1$ and $v_3$ for $\pi$, K, $p$, net-kaon, net-proton, $d$, $t$, and ${}^{3}He$ in Au+Au collisions at $\sqrt{s_{NN}}$ = 3.2, 3.5, 3.9, and 4.5 GeV taken in fixed-target mode from the second phase of the beam energy scan (BES-II) program at RHIC-STAR. We will show the dependencies of $v_1$ and $v_3$ on rapidity, centrality, and collision energy, and subsequently, discuss their physics implications. The experimental measurements will be compared with the results from the JAM transport model to understand the underlying physics mechanisms at low collision energies.
Details
Sharang Rav Sharma, IISER Tirupati, India, for STAR Collaboration
https://www.iisertirupati.ac.in/
| Internet talk | Yes |
|---|---|
| Is this an abstract from experimental collaboration? | Yes |
| Name of experiment and experimental site | STAR Collaboration at RHIC |
| Is the speaker for that presentation defined? | Yes |
