Class nstar_hot (o2scl)

O2scl : Class List

class nstar_hot : public o2scl::nstar_cold

Neutron stars at finite temperature and entropy.

Public Functions

inline nstar_hot()

inline void set_eos_T(eos_had_temp_base &he)

Set the finite-temperature hadronic EOS.

int calc_eos_T(double T, double np_0 = 0.0)

Compute the EOS in betq-equilibrium at finite temperature.

int calc_eos_point_beta_T(double nb, double T, double &np, thermo &hb)

Compute the EOS in betq-equilibrium at finite temperature at a particular density.

int calc_eos_point_beta_s(double nb, double sonb, double &np, thermo &hb)

Compute the EOS in betq-equilibrium at finite entropy per baryon.

int calc_eos_s(double s, double np_0 = 0.0)

Compute the EOS in betq-equilibrium at fixed entropy per baryon.

int calc_eos_s_YLe(double s, double YLe, double np_0 = 0.0)

Compute the EOS in betq-equilibrium at fixed entropy per baryon at a fixed number of electron-type leptons per baryon.

Protected Types

typedef boost::numeric::ublas::vector<double> ubvector

Protected Functions

int solve_fun_T(size_t nv, const ubvector &x, ubvector &y, thermo &hb, double T, double n_B)

Solve for beta equilibrium at finite temperature.

int solve_fun_s(size_t nv, const ubvector &x, ubvector &y, thermo &hb, double sonb, double n_B)

Solve for beta equilibrium at finite entropy per baryon.

int solve_fun_s_YLe(size_t nv, const ubvector &x, ubvector &y, thermo &hb, double s, double YLe, double n_B)

Solve for beta equilibrium at finite temperature.

Protected Attributes

eos_had_temp_base *hepT

A pointer to the finite temperature equation of state.

fermion_rel ft

Fermion thermodynamics (for the leptons)

bool eos_T_set

If true, then the hadronic EOS has been set.