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--- the_lumberjacks [2014/06/11 15:40]
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+++ the_lumberjacks [2014/06/11 15:47] (current)
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 \end{equation}
-The free parameters in these trajectories are the initial temperatures and densities as well as the electron fraction.
+The free parameters in these trajectories are the initial temperatures and densities as well as the electron fraction.  The initial temperature of 37Gk and initial density of $1\times 10^{9}$ g/cm${^3}$. The electron fraction was given values of 0.42, 0.44, 0.46, 0.48, and 0.50.
+We started the network calculation when the temperature reaches 10GK.  This is a safe approximation since above this temperature, the material will be in Nuclear Statistical Equilibrium and the evolution of the abundances will not be set by the thermal history.  We used a network of 4510 isotopes, ranging from free nucleons to fermium (Z=100).
 ===== References =====

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