Radiation Hydrodynamics: References

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Inverse transport theory and applications (2009, background): “The transport equation may be derived either phenomenologically [39, 60, 83, 110] or from first principles as a high frequency limit of (classical or quantum) waves propagating in highly heterogeneous media; see e.”
RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR COLLAPSE: PROTOSTELLAR CORE FORMATION (2012, unknown): “To avoid numerical difficulties due to strong nonlinearity in the flux limiter and the opacities and to achieve stable integration, we adopt the time-lagged opacities and flux limiter (Castor 2004).”
THE EARLY UV/OPTICAL EMISSION FROM CORE-COLLAPSE SUPERNOVAE (2010, unknown): “6.9 of Castor 2004), is beyond the scope of the present manuscript.”
Equations and Algorithms for Mixed-frame Flux-limited Diffusion Radiation Hydrodynamics (2006, unknown): “In contrast, several authors have analyzed the radiation hydrodynamic equations in the general case to beyond first order in v/c (e.g. Mihalas & Weibel-Mihalas 1999; Castor 2004, and references therein).”
Two-Dimensional Multiangle, Multigroup Neutrino Radiation-Hydrodynamic Simulations of Postbounce Supernova Cores (2008, unknown): “At radii outside∼200 km, the typical striping pattern of Sn (Castor 2004) becomes visible, though not yet dominant.”