The RHIC Beam Energy Scan - STAR'S Perspective
Abstract
The first decade of RHIC running has established the existence of a strongly coupled Quark Gluon Plasma (sQGP), a new state of nuclear matter with partonic degrees of freedom. Theory predicts how transitions to this sQGP depend on the baryon chemical potential, mu_B, and temperature, T. At low mu_B and high T a cross-over transition occurs. At high mu_B and low T the transition is of first order. Hence, at intermediate values, a critical point should occur. Experimentally we can vary these initial conditions by altering the beam energy. Thus a beam energy scan (BES) will allow us to explore the QCD phase diagram close to the QGP-hadron gas boundary and locate such key "landmarks" as the critical point. Establishing the existence of this critical point would be a seminal step forwards for QCD physics. I discuss below the physics case for a BES, and explain why RHIC and the STAR experiment are ideally designed for such a program.
Keywords
Cite
@article{arxiv.0906.0305,
title = {The RHIC Beam Energy Scan - STAR'S Perspective},
author = {Helen Caines},
journal= {arXiv preprint arXiv:0906.0305},
year = {2019}
}
Comments
Proceedings for the Rencontres de Moriond 2009 QCD session