Class eos_had_tabulated (o2scl)¶
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class eos_had_tabulated : public o2scl::eos_had_eden_base¶
Zero-temperature EOS from a table.
This assumes a symmetry energy which depends quadratically on the isospin asymmetry in order to construct an EOS from a table of baryon density and energy per baryon for both nuclear and pure neutron matter.
Note: If using a tabulated EOS to compute derivatives (like the compressibility which effectively requires a second derivative), it is important to tabulated the EOS precisely enough to ensure that the derivatives are accurate. In the case of ensuring that the compressibility at saturation density is reproduced to within 3 significant figures, the EOS should be specified with at least 6 digits of precision on a grid at least as small as 0.002 \( \mathrm{fm}^{-3} \).
- Idea for Future:
Storage in a o2scl::table object isn’t necessary, and storing in a vector object is more efficient.
Allow the pressure to be specified to make the EOS more accurate?
The EOS tables
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bool one_table¶
If true, then tnuc and tneut point to the same table.
Strings for the column names
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std::string srho_nuc¶
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std::string srho_neut¶
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std::string snuc¶
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std::string sneut¶
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inline void free_table()¶
Free the table memory.
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inline virtual int calc_temp_f_gen(double nB, double nQ, double nS, double T, thermo &th)¶
Equation of state as a function of baryon, charge, and strangeness density at finite temperature.
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inline eos_had_tabulated()¶
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inline virtual ~eos_had_tabulated()¶
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inline virtual int calc_e(fermion &ne, fermion &pr, thermo &th)¶
Equation of state as a function of density.
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template<class vec_t>
inline int set_eos(size_t n, vec_t &rho, vec_t &Enuc, vec_t &Eneut)¶ Set the EOS through vectors specifying the densities and energies.
Protected Attributes
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bool table_alloc¶
True if the table has been allocated.