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Fig. 7

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Schematic representation of a single time step in our dynamic code. In this chart ρ0 is the initial crust density, Ye,0 is the initial electron fraction, Y(Z0) is the initial chemical abundance of the crust, T0 is the initial temperature, Z0 is the initial atomic number and n0 is the initial particle density of the crust. The neutron density (nn) is first found using the secant method and then reaction network is solved using the Crank-Nicholson method. After solving the reaction network evolution of the density (ρ(t)), heating due to β and neutron decay and nuclear fission is calculated. The neutron density is then re-evaluated and finally the maximal temperature change criterion is checked before moving on to the next time step.

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