Crust

A code for computing the structure of a neutron star crust.

This documentation was generated from git commit

608fe58a13fd79997e1e31894d7c528ee75f47fa

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):

• crust::crust_driver::full_eq()
  • crust::crust_driver::compute_sna()
• crust::crust_driver::delta_ZN()
• Minimize 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:

• crust::crust_driver::acc()
  • crust::rxns::emit_neutron()
  • crust::dist_thermo::gibbs_energy_per_baryon_cell()
  • crust::rxns::elec_capture()
  • crust::rxns::beta_decay()
  • crust::rxns::pyc_fusion()
  • crust::dist_thermo::free_energy_dist()
  • crust::dist_thermo::gibbs_energy_dist()

• Class Documentation
  • sna_thermo
  • dist_thermo
  • multi_zone
  • pyc_rates
  • crust_driver
  • rxns
  • shear_eigen
  • tov_shear
  • table3d_eos
• Bibliography

• Index
• Module Index
• Search Page