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Right now, the equation of state classes depend on the user to input the correct value of non_interacting
for the particle inputs. This is not very graceful...
Class apr_eos
There might be room to improve the testing of the finite temperature part a bit.
Class apr_eos
There is some repetition between calc_e() and calc_temp_e() that possibly could be removed.
Class bps_eos
Can the pressure be made to match more closely?
Class bps_eos
Convert to a hadronic_eos object and offer an associated interface?
Class cfl_njl_eos
This class internally mixes ovector, omatrix, gsl_vector and gsl_matrix objects in a confusing and non-optimal way. Fix this.
Class cfl_njl_eos
Allow user to change derivative object? This isn't possible right now because the stepsize parameter of the derivative object is used.
Class cold_nstar
Convert tables to table_units
Class cold_nstar
Ensure that the adiabatic index of the central density is greater than 4/3
Class cold_nstar
Warn if the EOS becomes pure neutron matter.
Class ddc_eos
Implement the finite temperature EOS properly.
Class gen_potential_eos
Calculate the chemical potentials analytically
Class hadronic_eos
Could write a function to compute the "symmetry free energy" or the "symmetry entropy"
Class nse_eos
Right now calc_density() needs a very good guess. This could be fixed, probably by solving for the log(mu/T) instead of mu.
Class rmf_delta_eos
Finish the finite temperature EOS
Class rmf_eos
It might be nice to remove explicit reference to the meson masses in functions which only compute nuclear matter since they are unnecessary. This might, however, demand redefining some of the couplings. Fix calc_p() to be better at guessing The number of couplings is getting large, maybe new organization is required. Overload hadronic_eos::fcomp() with an exact version
Global rmf_eos::calc_e (fermion &ne, fermion &pr, thermo <h)
Improve the operation of this function when the proton density is zero.
Global rmf_eos::calc_e_fields (fermion &ne, fermion &pr, thermo <h, double &sig, double &ome, double &rho)
Improve the operation of this function when the proton density is zero.
Class tov_buchdahl_eos
Figure out what to do with the buchfun() function
Global tov_solve::bio
Is this really required?
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