Class Hierarchy
This inheritance list is sorted roughly, but not completely, alphabetically:
[detail level 1234567]
 Co2scl::eos_baseEquation of state base class
 Co2scl::eos_crustBaym-Pethick-Sutherland equation of state
 Co2scl::eos_had_baseHadronic equation of state [abstract base]
 Co2scl::eos_had_eden_baseA hadronic EOS based on a function of the densities [abstract base]
 Co2scl::eos_had_ddcRelativistic mean field EOS with density dependent couplings
 Co2scl::eos_had_gognyGogny EOS
 Co2scl::eos_had_hlpsSchematic EOS from Hebeler et al
 Co2scl::eos_had_potentialGeneralized potential model equation of state
 Co2scl::eos_had_sym4_mdiA version of eos_had_potential to separate potential and kinetic contributions
 Co2scl::eos_had_schematicSchematic hadronic equation of state
 Co2scl::eos_had_sym4Construct an EOS with an arbitrary choice for the terms in the symmetry energy that are quartic in the isospin asymmetry
 Co2scl::eos_had_tabulatedZero-temperature EOS from a table
 Co2scl::eos_had_pres_baseA hadronic EOS based on a function of the chemical potentials [abstract base]
 Co2scl::eos_had_temp_baseA finite temperature hadronic EOS [abstract base]
 Co2scl::eos_had_temp_eden_baseA hadronic EOS at finite temperature based on a function of the densities [abstract base]
 Co2scl::eos_had_aprEOS from Akmal, Pandharipande, and Ravenhall
 Co2scl::eos_had_sym4_aprA version of eos_had_apr to separate potential and kinetic contributions
 Co2scl::eos_had_skyrmeSkyrme hadronic equation of state
 Co2scl::eos_had_sym4_skyrmeA version of eos_had_skyrme to separate potential and kinetic contributions
 Co2scl::eos_had_temp_pres_baseA hadronic EOS at finite temperature based on a function of the chemical potentials [abstract base]
 Co2scl::eos_crust_virialVirial EOS for neutrons, protons, deuterons, and alpha particles
 Co2scl::eos_had_rmfRelativistic mean field theory EOS
 Co2scl::eos_had_rmf_deltaField-theoretical EOS with scalar-isovector meson, $ \delta $
 Co2scl::eos_had_sym4_rmfA version of eos_had_rmf to separate potential and kinetic contributions
 Co2scl::eos_quarkQuark matter equation of state base
 Co2scl::eos_quark_bagSimple bag model
 Co2scl::eos_quark_njlNambu Jona-Lasinio EOS at zero temperature
 Co2scl::eos_quark_cflNambu Jona-Lasinio model with a schematic CFL di-quark interaction at finite temperature
 Co2scl::eos_quark_cfl6An EOS like eos_quark_cfl but with a color-superconducting 't Hooft interaction
 Co2scl::eos_had_sym4_baseA class to compute quartic contributions to the symmetry energy [abstract base]
 Co2scl::eos_had_sym4_aprA version of eos_had_apr to separate potential and kinetic contributions
 Co2scl::eos_had_sym4_mdiA version of eos_had_potential to separate potential and kinetic contributions
 Co2scl::eos_had_sym4_rmfA version of eos_had_rmf to separate potential and kinetic contributions
 Co2scl::eos_had_sym4_skyrmeA version of eos_had_skyrme to separate potential and kinetic contributions
 Co2scl::eos_nseEquation of state for nuclei in statistical equilibrium
 Co2scl::eos_nse_fullEOS for nuclear statistical equilibrium with interactions
 Co2scl::eos_sn_baseA base class for the supernova EOSs [abstract]
 Co2scl::eos_sn_hfslThe Hempel et al. supernova EOSs
 Co2scl::eos_sn_lsThe Lattimer-Swesty supernova EOS
 Co2scl::eos_sn_ooThe EOS tables from O'Connor and Ott
 Co2scl::eos_sn_shtA class to manipulate the G. Shen et al. EOS
 Co2scl::eos_sn_stosThe H. Shen et al. supernova EOS
 Co2scl::eos_tovA EOS base class for the TOV solver
 Co2scl::eos_nstar_rotAn EOS for nstar_rot
 Co2scl::eos_nstar_rot_interpCreate a tabulated EOS for nstar_rot using interpolation
 Co2scl::eos_nstar_rot_CTabulated EOS for nstar_rot from Bethe74
 Co2scl::eos_nstar_rot_LTabulated EOS for nstar_rot from Pandharipande75
 Co2scl::eos_tov_buchdahlThe Buchdahl EOS for the TOV solver
 Co2scl::eos_tov_interpAn EOS for the TOV solver using simple linear interpolation and an optional crust EOS
 Co2scl::eos_tov_linearLinear EOS $ P = c_s^2 (\varepsilon-\varepsilon_0) $
 Co2scl::eos_tov_polytropeStandard polytropic EOS $ P = K \varepsilon^{1+1/n} $
 Co2scl::eos_tov_vectors< vec_t >Provide an EOS for TOV solvers based on interpolation of user-supplied vectors
 Cex_eos_had_aprCompute the APR EOS with a Gibbs construction and the mass versus radius curve [Example class]
 Cex_eos_had_skyrmeClass to analyze Skyrme EOSs and output the results [Example class]
 Cex_skyrme_dataOutput data for a Skyrme EOS [Example class]
 Co2scl::nucleus_rmf::initial_guessInitial guess structure
 Co2scl::eos_quark_njl::njtp_sA structure for passing parameters to the integrands
 Co2scl::nstar_coldNaive static cold neutron star
 Co2scl::nstar_rotRotating neutron star class based on RNS v1.1d from N. Stergioulas et al
 Co2scl::nucleus_rmfSpherical closed-shell nuclei with a relativistic mean-field model in the Hartree approximation
 Co2scl::nucmass_ibm_shell [external]
 Co2scl::nucmass_frdm_shellMass formula adding simple shell effects to the finite-range liquid droplet model
 Co2scl::nucmass_ldrop_shellLiquid drop model with shell effects
 Co2scl::nucmass_info [external]
 Co2scl::nucmass [external]
 Co2scl::nucmass_fit_base [external]
 Co2scl::nucmass_frdm [external]
 Co2scl::nucmass_frdm_shellMass formula adding simple shell effects to the finite-range liquid droplet model
 Co2scl::nucmass_ldropSimple liquid drop mass formula
 Co2scl::nucmass_ldrop_skinMore advanced liquid drop model
 Co2scl::nucmass_ldrop_pairLiquid drop model with pairing
 Co2scl::nucmass_ldrop_shellLiquid drop model with shell effects
 Co2scl::nucleus_rmf::odparmsA convenient struct for the solution of the Dirac equations
 Co2scl::nstar_rot::polytrope_solveSubclass of nstar_rot which specifies the function to invert a polytropic EOS
 Co2scl::nucleus_rmf::shellA shell of nucleons for nucleus_rmf
 Co2scl::eos_sn_base::sliceA slice of data from eos_sn_base for one index fixed
 Co2scl::tov_loveDetermination of the neutron star Love number
 Co2scl::tov_solveClass to solve the Tolman-Oppenheimer-Volkov equations

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