Crust ===== A code for computing the structure of a neutron star crust. This documentation was generated from git commit .. include:: commit.rst Based partially on work in [Steiner08]_, this code was written for use in [Steiner12]_ and then used again in [Deibel14]_ (which was itself based on [Steiner09]_ ). Basic call stack ---------------- Full equilibrium crust (T=0): - :cpp:func:`crust::crust_driver::full_eq()` * :cpp:func:`crust::crust_driver::compute_sna()` - :cpp:func:`crust::crust_driver::delta_ZN()` - Minimize :cpp:func:`crust::sna_thermo::free_energy_sna_neut::operator()` * crust::sna_thermo::free_energy_sna_fix_nb_nn() * crust::sna_thermo::baryon_density_sna() * crust::sna_thermo::free_energy_sna() Accreted crust: - :cpp:func:`crust::crust_driver::acc()` * :cpp:func:`crust::rxns::emit_neutron()` * :cpp:func:`crust::dist_thermo::gibbs_energy_per_baryon_cell()` * :cpp:func:`crust::rxns::elec_capture()` * :cpp:func:`crust::rxns::beta_decay()` * :cpp:func:`crust::rxns::pyc_fusion()` * :cpp:func:`crust::dist_thermo::free_energy_dist()` * :cpp:func:`crust::dist_thermo::gibbs_energy_dist()` .. toctree:: :maxdepth: 2 classdoc bib * :ref:`genindex` * :ref:`modindex` * :ref:`search`