deletions | additions       diff --git a/Initial Conditions.tex b/Initial Conditions.tex  index 720cc09..165f326 100644  --- a/Initial Conditions.tex  +++ b/Initial Conditions.tex 
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\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 \cite{Bruenn_1985} rates. Include weak magnetism and recoil corrections via \cite{Horowitz_2002}.  \item For scattering on heavy nuclei, use the \cite{Bruenn_1985} rate, includecorrections via \cite{Burrows_2006}:  Ion-ion correlations, correlations via \cite{Horowitz_1997},  electron polarization correction, correction (??),  and a correction for the nuclear form factor. factor via \cite{Bruenn_1997,Rampp_2002}.  \item Include inelastic neutrino-electron scattering only in 1D simulations. This will include inelastic scattering during the collapse phase of 2D simulations as up to 15ms postbounce will be done in 1D.  \item For pair processes, include electron-positron annihilation to neutrino pairs (and the reverse). Ignore all other pair processes, nucleon-nucleon Bremsstrahlung and neutrino pair conversion to other neutrino pairs.  \item Use \cite{Bruenn_1985} rates for absorption rates (on nucleons and nuclei). Include weak magnetism and recoil corrections for nucleon rates. Do not include any nucleon potentials.