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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. | |
Public Member Functions inherited from o2scl::nstar_cold | |
| 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 | |
Data Fields inherited from o2scl::nstar_cold | |
| 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 |
Protected Member Functions inherited from o2scl::nstar_cold | |
| double | solve_fun (double x) |
Protected Attributes inherited from o2scl::nstar_cold | |
| 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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