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Currently the RHIC Beam Energy Scan is exploring a new region of the QuantumChromodynamic phase diagram at large baryon densities that approaches nuclearastrophysics regimes. This provides an opportunity to study relativistichydrodynamics in a regime where the net conserved charges of baryon number,strangeness, and electric charge play a role, which will significantly changethe theoretical approach to simulating the baryon-dense Quark-Gluon Plasma.Here we detail many of the important changes needed to adapt both initialconditions and the medium to baryon-rich matter. Then, we make baselinepredictions for the elliptical flow and fluctuations based on extrapolating thephysics at LHC and top RHIC energies to support future analyses of where andhow the new baryon-dense physics causes these extrapolations to break down.First we compare eccentricities across beam energies, exploring theirunderlying assumptions; we find the the extrapolated initial state is predictedto be nearly identical to that at AuAu $\sqrt{s_{NN}}=200$ GeV. Then the finalflow harmonic predictions are based on linear+cubic response. We discusspreliminary STAR results in order to determine the implications that they havefor linear+cubic response coefficients at the lowest beam energy of AuAu$\sqrt{s_{NN}}=7$ GeV.

Baseline predictions of elliptic flow and fluctuations at the RHIC Beam Energy Scan using response coefficients