Bayesian Analysis of Neutron Star Mass and Radius Observations
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A simplified version of nstar_cold. More...
This simplified version only computes the energy density and pressure rather than the O2scl version which computes several extra quantities. This class is part of bamr::model.
Definition at line 50 of file nstar_cold2.h.
#include <nstar_cold2.h>
Public Member Functions | |
int | calc_eos (double np_0=0.0) |
Compute the core EOS. | |
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void | set_eos (eos_had_base &he) |
void | calc_eos (double np_0=0.0) |
double | calc_urca (double np_0=0.0) |
void | calc_nstar () |
void | fixed (double target_mass) |
void | set_eos (eos_had_base &he) |
void | calc_eos (double np_0=0.0) |
double | calc_urca (double np_0=0.0) |
void | calc_nstar () |
void | fixed (double target_mass) |
o2_shared_ptr< table_units<> >::type | get_eos_results () |
o2_shared_ptr< table_units<> >::type | get_tov_results () |
int | set_n_and_p (fermion &n, fermion &p) |
int | set_root (root<> &rf) |
int | set_tov (tov_solve &ts) |
Additional Inherited Members | |
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fermion | def_n |
fermion | def_p |
fermion_zerot | fzt |
tov_solve | def_tov |
root_cern | def_root |
eos_tov_interp | def_eos_tov |
bool | solver_success |
bool | well_formed |
double | pressure_flat |
double | allow_urca |
double | deny_urca |
double | acausal |
double | acausal_pr |
double | acausal_ed |
double | solver_tol |
int | verbose |
double | nb_start |
double | nb_end |
double | dnb |
bool | include_muons |
bool | err_nonconv |
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double | solve_fun (double x) |
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bool | eos_set |
fermion | e |
fermion | mu |
eos_had_base * | hep |
fermion * | np |
fermion * | pp |
tov_solve * | tp |
root * | rp |
o2_shared_ptr< table_units<> >::type | eost |
double | barn |
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