O2scl_eos Data Structures

Here are the data structures with brief descriptions:
apr4_eosA version of apr_eos to separate potential and kinetic contributions
apr_eosEOS from Akmal, Pandharipande, and Raveno2scll (zero temperature)
bag_eosNaive bag model EOS
bps_eosBaym-Pethick-Sutherland equation of state
cfl6_eosCFL NJL EOS with a color-superconducting 't Hooft interaction
cfl_njl_eosNambu Jona-Lasinio model with a schematic CFL di-quark interaction at finite temperature
cold_nstarNaive static cold neutron star
ddc_eosRelativistic mean field EOS with density dependent couplings
eosEquation of state base
eos_iocSetup I/O objects for equation of state classes
gen_potential_eosGeneralized potential model equation of state
had_gibbs_nseosCreate a Gibbs phase transition between two hadronic EOSs to create neutron star matter
had_gibbs_nseos::chipar_sUseful structure for parameters to had_gibbs_nseos::fixed_chi_eqs() [protected]
had_gibbs_nseos::solvepar_sUseful structure for parameters to phase1_eqs(), phase2_eqs(), and gibbs_eqs() [protected]
hadronic_eosHadronic equation of state
hadronic_eos::denpar_sDensity parameters [protected]
hadronic_eos::mupar_sChemical potential parameters [protected]
mdi4_eosA version of gen_potential_eos to separate potential and kinetic contributions
nambujl_eosNambu Jona-Lasinio EOS at zero temperature
nambujl_eos::njtp_sA structure for passing parameters to the integrands [protected]
quark_eosQuark matter equation of state base
rmf4_eosA version of rmf_eos to separate potential and kinetic contributions
rmf_delta_eosField-theoretical EOS with scalar-isovector meson,
rmf_eosRelativistic mean field theory EOS
schematic_eosSchematic hadronic equation of state
skyrme4_eosA version of skyrme_eos to separate potential and kinetic contributions
skyrme_eosSkyrme hadronic equation of state at zero temperature
sym4_eosConstruct an EOS with an arbitrary choice for the terms in the symmetry energy that are quartic in the isospin asymmetry
sym4_eos_baseA class to compute quartic contributions to the symmetry energy
tabulated_eosEOS from a table
tov_buchdahl_eosThe Buchdahl EOS for the TOV solver
tov_eosA EOS base class for the TOV solver
tov_interp_eosAn EOS for the TOV solver using simple linear interpolation and a default low-density EOS
tov_polytrope_eosStandard polytropic EOS $ p = K \rho^{1+1/n} $
tov_solveClass to solve the Tolman-Oppenheimer-Volkov equations

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