We use a self-consistent chiral-hydrodynamic formalism which combines the linear $sigma$ model with second-order hydrodynamics in 2+1 dimensions to compute the spectrum of thermal photons produced in Au+Au collisions at $sqrt{s_{NN}}=200$ GeV. The temperature-dependent shear viscosity of the model, $eta$, is calculated from the linearized Boltzmann equation. We compare the results obtained in the chiral-hydrodynamic model to those obtained in the second-order theory with a Lattice QCD equation of state and a temperature-independent value of $eta/s$. We find that the thermal photon production is significantly larger in the latter model due to a slower evolution and larger dissipative effects.
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