Class eos_tov_vectors (o2scl)¶
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template<class vec_t>
class eos_tov_vectors : public o2scl::eos_tov¶ Provide an EOS for TOV solvers based on interpolation of user-supplied vectors.
EOS storage
Interpolators
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interp_vec<vec_t> pe_int¶
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interp_vec<vec_t> pn_int¶
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interp_vec<vec_t> ep_int¶
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interp_vec<vec_t> en_int¶
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interp_vec<vec_t> np_int¶
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interp_vec<vec_t> ne_int¶
Basic EOS functions
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inline virtual double ed_from_pr(double pr)¶
From the pressure, return the energy density.
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inline virtual double pr_from_ed(double ed)¶
From the energy density, return the pressure.
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inline virtual double nb_from_ed(double ed)¶
From the energy density, return the baryon density.
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inline virtual double nb_from_pr(double pr)¶
From the pressure, return the baryon density.
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inline virtual double ed_from_nb(double nb)¶
From the baryon density, return the energy density.
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inline virtual double pr_from_nb(double nb)¶
From the baryon density, return the pressure.
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inline virtual void ed_nb_from_pr(double pr, double &ed, double &nb)¶
Given the pressure, produce the energy and number densities.
The arguments
prandedshould always be in \( M_{\odot}/\mathrm{km}^3 \) . The argument fornbshould be in \( \mathrm{fm}^{-3} \) .If baryon_column is false, then
nbis unmodified.
Public Functions
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inline void read_vectors_swap(size_t user_n, vec_t &user_ed, vec_t &user_pr, vec_t &user_nb)¶
Read the EOS from a set of equal length vectors for energy density, pressure, and baryon density.
In this version, the user-specified vectors are swapped with internal storage.
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inline void read_vectors_swap(size_t user_n, vec_t &user_ed, vec_t &user_pr)¶
Read the EOS from a pair of equal length vectors for energy density and pressure.
In this version, the user-specified vectors are swapped with internal storage.
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interp_vec<vec_t> pe_int¶