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\subsection{Neutrino Physics}  \begin{enumerate}  \item Use three species, $\nu_e$, $\bar{\nu}_e$, and $\nu_x = \{\nu_\mu$ $\bar{\nu}_\mu$, $\nu_\tau$, and $\bar{\nu}_\tau\}$.  \item Use a clearly defined energy bin structure.  \item The SFHo EOS contains light clusters. For this study, all neutrino interactions (both absorption and scattering) on light clusters is ignored.  \item For scattering on free nucleons, use the Breunn (1985) rates. Include weak magnetism and recoil corrections.  \item For scattering on heavy nuclei, use the Breunn (1985) rate, include corrections a la Burrows, Reddy, and Thompson (2006): Ion-ion correlations, electron polarization correction, and a correction for the nuclear form factor.