Beam Energy Dependence of the Third Harmonic of Azimuthal Correlations in Au+Au Collisions at RHIC
STAR Collaboration: L. Adamczyk, J. K. Adkins, G. Agakishiev, M. M., Aggarwal, Z. Ahammed, I. Alekseev, A. Aparin, D. Arkhipkin, E. C. Aschenauer,, A. Attri, G. S. Averichev, X. Bai, V. Bairathi, R. Bellwied, A. Bhasin, A. K., Bhati, P. Bhattarai, J. Bielcik, J. Bielcikova

TL;DR
This study analyzes the third harmonic of azimuthal correlations in Au+Au collisions across a range of energies, revealing insights into the presence of quark-gluon plasma and its properties at different collision energies.
Contribution
It provides the first systematic measurement of the third harmonic $v_3^2 ext{(2)}$ over a wide energy range, highlighting its persistence at low energies and its scaling behavior.
Findings
$v_3^2 ext{(2)}$ persists down to 7.7 GeV in central collisions.
$v_3^2 ext{(2)}$ is consistent with zero in peripheral collisions at low energies.
A minimum in scaled $v_3^2 ext{(2)}$$ occurs near 20 GeV.
Abstract
We present results from a harmonic decomposition of two-particle azimuthal correlations measured with the STAR detector in Au+Au collisions for energies ranging from GeV to 200 GeV. The third harmonic , where is the angular difference in azimuth, is studied as a function of the pseudorapidity difference between particle pairs . Non-zero {\vthree} is directly related to the previously observed large- narrow- ridge correlations and has been shown in models to be sensitive to the existence of a low viscosity Quark Gluon Plasma (QGP) phase. For sufficiently central collisions, persist down to an energy of 7.7 GeV suggesting that QGP may be created even in these low energy collisions. In peripheral collisions at these low energies however,…
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