\documentclass[12pt]{article} \usepackage{geometry} \geometry{a4paper,inner=18mm,outer=18mm,top=26mm,bottom=26mm,} \usepackage{authblk} \usepackage{nopageno} \usepackage{lineno} \usepackage{hyperref} \begin{document} \begin{center} {\large \bf Search for the Chiral Magnetic Effect with the BES-II data aided by the Event Plane Detector at STAR} \bigskip Yu Hu \\ Fudan University, Brookhaven National Laboratory \\ Zhiwan Xu \\University of California Los Angeles\\ (for the STAR collaboration)\\ \bigskip \end{center} \linenumbers \begin{abstract} % The Quark-Gluon Plasma droplets produced in relativistic heavy-ion collisions have been conjectured to exhibit a spontaneous electric-charge separation in the direction of strong magnetic field through a phenomenon known as the Chiral Magnetic Effect (CME). Recently, STAR experiment has performed a precision measurement of charge separation difference between Ru+Ru and Zr+Zr collisions at $\sqrt{s_{\rm NN}}=200$ GeV, and showed that the magnitude of possible difference in the charge separation attributable to the different magnetic fields in the two systems is much smaller than previously expected \cite{STAR:2021mii}. We present results of the CME search from the RHIC BES-II data, where the magnetic field may last longer than those at the high energy collisions and the non-flow related background is expected to be smaller. For the BES-II program, the Event Plane Detector (EPD) installed in the year 2018 at STAR provides a unique capability for the CME search. The EPD can determine the event plane angles at forward/backward rapidity. With the reconstructed EPD plane, this opens up new event shape selection capabilities, to enhance the sensitivity for the CME search with the BES-II data recently collected by STAR. In this poster, We will present the CME search results at STAR using the EPD from Au+Au collisions at $\sqrt{s_{\rm NN}} =$ 27 GeV, 19 GeV, and 14.5 GeV. % \end{abstract} \begin{thebibliography}{99} \bibitem{STAR:2021mii} J. Adam, et al. {STAR Collaboration}, {Search for the Chiral Magnetic Effect with Isobar Collisions at $\sqrt{s_{NN}}$ = 200 GeV by the STAR Collaboration at RHIC}, (2021), \href{https://arxiv.org/abs/2109.00131}{arXiv:2109.00131[nucl-ex]}. \end{thebibliography} \end{document}