\documentclass[12pt]{article} %,aps,longbibliography]{article}
\usepackage{geometry}
\geometry{a4paper,inner=22mm,outer=22mm,top=26mm,bottom=26mm,}
\usepackage{authblk}
\usepackage{nopageno}
\usepackage{lineno}
\usepackage[utf8]{inputenc} 
\linenumbers 

\usepackage{hyperref}

\bibliographystyle{apsrev4-1}

\begin{document}

\begin{center}


{\large \bf Search for the chiral effect using isobar collisions and BES-II data from STAR}\\

\bigskip
the STAR Collaboration\\

\bigskip

\end{center}
\begin{abstract}
Quantum Chromodynamics allows for the formation of parity-odd domains inside the medium produced in heavy-ion collisions associated with a net chirality of the quarks. As a consequence, the Chiral Magnetic Effect (CME) and Chiral Vortical Effect (CVE) are phenomena predicted to occur and cause electric-charge and baryonic-charge separation along the direction of the magnetic field and vorticity created in heavy-ion collisions, respectively. 
%
Recently, the STAR experiment has performed a precision measurement of the possible difference in charge separation along the magnetic field direction between isobar systems $^{96}_{44}{\rm Ru}+^{96}_{44}{\rm Ru}$ and $^{96}_{40}{\rm Zr}+^{96}_{40}{\rm Zr}$ at $\sqrt{s_{\rm NN}}=200$ GeV. % 
%
In this talk, we will present the findings from the isobar blind analysis.
%
While the isobar blind analyses were dedicated towards CME searches at the top RHIC energy, the RHIC BES-II program provides a unique opportunity and advantages at lower energies, where the magnetic field lifetime may be longer than those at the higher energy collisions. 
%
We will also present the latest results on the search for CME and CVE at 27 GeV Au+Au collisions with the unique capabilities of the STAR Event Plane Detector.  
\end{abstract}

\end{document}