Class ex_eos_had_skyrme ()¶

O2scl : Class List

class ex_eos_had_skyrme¶

Class to analyze Skyrme EOSs and output the results [Example class].

Public Functions

inline ex_eos_had_skyrme()¶

inline void compare_neut_nstar()¶: Generate a table comparing neutron matter and neutron star matter.

inline int check_pressure()¶: Check if the pressure of neutron matter is positive.

inline int low_neutron_mat()¶

Check low-density neutron matter.

I’m not sure where the data originally came from, but it was based on something similar to the left panel of Fig. 1 in Gandolfi et al. (2015).

Todo:: AWS 12/21/2020: I need to document here what “quality” values are reasonable. I should probably make this optional as well, as many Skyrme interactions are not intended to be used at this density.

inline int saturation_prop()¶: Test saturation density.

inline int mvsr()¶: Compute the M vs. R curve.

inline int json(vector<string> &sv, bool itive_com)¶: Summarize the results of one model.

inline int summary(vector<string> &sv, bool itive_com)¶: Summarize the results of one model.

inline int test(vector<string> &sv, bool itive_com)¶: Test the code.

inline int store(vector<string> &sv, bool itive_com)¶: Write to a file.

inline int unedf(vector<string> &sv, bool itive_com)¶: Create data files for the UNEDF forces.

inline int load(vector<string> &sv, bool itive_com)¶: Load internally stored model.

inline int run_all(vector<string> &sv, bool itive_com)¶: Run all the models.

Public Members

eos_had_skyrme sk¶: Base EOS model.

string name¶: Model name.

double t0hc¶: Parameter t0 in MeV.

double t1hc¶: Parameter t1 in MeV.

double t2hc¶: Parameter t2 in MeV.

double t3hc¶: Parameter t3 in MeV.

double W0hc¶: Parameter W0 in MeV.

double b4hc¶: Parameter b4.

double b4phc¶: Parameter b4p.

int verbose¶: Verbose parameter.

bool output_files¶: If true, create output files for individual EOSs.

string file_prefix¶: Prefix for output files.

bool json_mode¶: If true, output JSON.

Protected Attributes

nstar_cold nst¶: To compute cold neutron stars.

nstar_hot nh¶: To compute hot neutron stars.

fermion n¶: Neutron.

fermion p¶: Proton.

fermion_deriv nd¶: Neutron.

fermion_deriv pd¶: Proton.

thermo th¶: Thermodynamics.

hdf_file hf¶: File for I/O.

ex_skyrme_data res¶: Results.

format_float fd¶: Formatting output.

table_units tneut¶: Neutron matter.

table_units tneut2¶: Neutron matter.