The RHIC Beam Energy Scan - STAR'S Perspective
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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.
[1] F. T. Collaboration,et al. First results from Au+Au collisions at \sqrt{s_{\rm NN}} = 9.2\,{\rm GeV} in STAR , 2008, 0812.4099.