Base class for equations of state which need two independent thermodynamic variables in order to determine the pressure. More...

#include <EquationOfState.hpp>

Public Types
using	creatable_classes = typename detail::DerivedClasses< IsRelativistic, 2 >::type

Public Member Functions
	EquationOfState (const EquationOfState &)=default

EquationOfState &	operator= (const EquationOfState &)=default

	EquationOfState (EquationOfState &&)=default

EquationOfState &	operator= (EquationOfState &&)=default

	EquationOfState (CkMigrateMessage *msg)

	WRAPPED_PUPable_abstract (EquationOfState)

virtual std::unique_ptr< EquationOfState< IsRelativistic, 2 > >	get_clone () const =0

virtual bool	is_equal (const EquationOfState< IsRelativistic, 2 > &rhs) const =0

virtual std::unique_ptr< EquationOfState< IsRelativistic, 3 > >	promote_to_3d_eos () const =0

virtual double	electron_fraction_lower_bound () const
	The lower bound of the electron fraction that is valid for this EOS.

virtual double	electron_fraction_upper_bound () const
	The upper bound of the electron fraction that is valid for this EOS.

virtual double	rest_mass_density_lower_bound () const =0
	The lower bound of the rest mass density that is valid for this EOS. More...

virtual double	rest_mass_density_upper_bound () const =0
	The upper bound of the rest mass density that is valid for this EOS. More...

virtual double	specific_internal_energy_lower_bound (const double rest_mass_density) const =0
	The lower bound of the specific internal energy that is valid for this EOS at the given rest mass density \(\rho\). More...

virtual double	specific_internal_energy_upper_bound (const double rest_mass_density) const =0
	The upper bound of the specific internal energy that is valid for this EOS at the given rest mass density \(\rho\). More...

virtual double	temperature_lower_bound () const
	The lower bound of the temperature that is valid for this EOS.

virtual double	temperature_upper_bound () const
	The upper bound of the temperature that is valid for this EOS.

virtual double	specific_enthalpy_lower_bound () const =0
	The lower bound of the specific enthalpy that is valid for this EOS. More...

virtual double	baryon_mass () const
	The vacuum mass of a baryon for this EOS. More...


virtual Scalar< double >	equilibrium_electron_fraction_from_density_temperature (const Scalar< double > &rest_mass_density, const Scalar< double > &) const

virtual Scalar< DataVector >	equilibrium_electron_fraction_from_density_temperature (const Scalar< DataVector > &rest_mass_density, const Scalar< DataVector > &) const


virtual Scalar< double >	pressure_from_density_and_energy (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	pressure_from_density_and_energy (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	pressure_from_density_and_enthalpy (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	pressure_from_density_and_enthalpy (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	specific_internal_energy_from_density_and_pressure (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	specific_internal_energy_from_density_and_pressure (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	temperature_from_density_and_energy (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	temperature_from_density_and_energy (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	specific_internal_energy_from_density_and_temperature (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	specific_internal_energy_from_density_and_temperature (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	chi_from_density_and_energy (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	chi_from_density_and_energy (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0


virtual Scalar< double >	kappa_times_p_over_rho_squared_from_density_and_energy (const Scalar< double > &, const Scalar< double > &) const =0

virtual Scalar< DataVector >	kappa_times_p_over_rho_squared_from_density_and_energy (const Scalar< DataVector > &, const Scalar< DataVector > &) const =0

Static Public Attributes
static constexpr bool	is_relativistic = IsRelativistic

static constexpr size_t	thermodynamic_dim = 2

Detailed Description

template<bool IsRelativistic>
class EquationsOfState::EquationOfState< IsRelativistic, 2 >

Base class for equations of state which need two independent thermodynamic variables in order to determine the pressure.

The template parameter IsRelativistic is true for relativistic equations of state and false for non-relativistic equations of state.

Member Function Documentation

◆ baryon_mass()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::baryon_mass ( ) const

inlinevirtual

The vacuum mass of a baryon for this EOS.

Reimplemented in EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ chi_from_density_and_energy() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::chi_from_density_and_energy	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes \(\chi=\partial p / \partial \rho |_{\epsilon}\) from the \(\rho\) and \(\epsilon\), where \(p\) is the pressure, \(\rho\) is the rest mass density, and \(\epsilon\) is the specific internal energy.

◆ chi_from_density_and_energy() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::chi_from_density_and_energy	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes \(\chi=\partial p / \partial \rho |_{\epsilon}\) from the \(\rho\) and \(\epsilon\), where \(p\) is the pressure, \(\rho\) is the rest mass density, and \(\epsilon\) is the specific internal energy.

◆ equilibrium_electron_fraction_from_density_temperature() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::equilibrium_electron_fraction_from_density_temperature	(	const Scalar< DataVector > &	rest_mass_density,
		const Scalar< DataVector > &
	)		const

inlinevirtual

Computes the electron fraction in beta-equilibrium \(Y_e^{\rm eq}\) from the rest mass density \(\rho\) and the temperature \(T\).

◆ equilibrium_electron_fraction_from_density_temperature() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::equilibrium_electron_fraction_from_density_temperature	(	const Scalar< double > &	rest_mass_density,
		const Scalar< double > &
	)		const

inlinevirtual

Computes the electron fraction in beta-equilibrium \(Y_e^{\rm eq}\) from the rest mass density \(\rho\) and the temperature \(T\).

◆ kappa_times_p_over_rho_squared_from_density_and_energy() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::kappa_times_p_over_rho_squared_from_density_and_energy	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes \(\kappa p/\rho^2=(p/\rho^2)\partial p / \partial \epsilon |_{\rho}\) from \(\rho\) and \(\epsilon\), where \(p\) is the pressure, \(\rho\) is the rest mass density, and \(\epsilon\) is the specific internal energy.

The reason for not returning just \(\kappa=\partial p / \partial \epsilon\) is to avoid division by zero for small values of \(\rho\) when assembling the speed of sound with some equations of state.

◆ kappa_times_p_over_rho_squared_from_density_and_energy() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::kappa_times_p_over_rho_squared_from_density_and_energy	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes \(\kappa p/\rho^2=(p/\rho^2)\partial p / \partial \epsilon |_{\rho}\) from \(\rho\) and \(\epsilon\), where \(p\) is the pressure, \(\rho\) is the rest mass density, and \(\epsilon\) is the specific internal energy.

The reason for not returning just \(\kappa=\partial p / \partial \epsilon\) is to avoid division by zero for small values of \(\rho\) when assembling the speed of sound with some equations of state.

◆ pressure_from_density_and_energy() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::pressure_from_density_and_energy	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes the pressure \(p\) from the rest mass density \(\rho\) and the specific internal energy \(\epsilon\).

◆ pressure_from_density_and_energy() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::pressure_from_density_and_energy	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes the pressure \(p\) from the rest mass density \(\rho\) and the specific internal energy \(\epsilon\).

◆ pressure_from_density_and_enthalpy() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::pressure_from_density_and_enthalpy	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes the pressure \(p\) from the rest mass density \(\rho\) and the specific enthalpy \(h\).

◆ pressure_from_density_and_enthalpy() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::pressure_from_density_and_enthalpy	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes the pressure \(p\) from the rest mass density \(\rho\) and the specific enthalpy \(h\).

◆ rest_mass_density_lower_bound()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::rest_mass_density_lower_bound ( ) const

pure virtual

The lower bound of the rest mass density that is valid for this EOS.

Implemented in EquationsOfState::DarkEnergyFluid< IsRelativistic >, EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ rest_mass_density_upper_bound()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::rest_mass_density_upper_bound ( ) const

pure virtual

The upper bound of the rest mass density that is valid for this EOS.

Implemented in EquationsOfState::DarkEnergyFluid< IsRelativistic >, EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ specific_enthalpy_lower_bound()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_enthalpy_lower_bound ( ) const

pure virtual

The lower bound of the specific enthalpy that is valid for this EOS.

Implemented in EquationsOfState::DarkEnergyFluid< IsRelativistic >, EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ specific_internal_energy_from_density_and_pressure() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_from_density_and_pressure	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes the specific internal energy \(\epsilon\) from the rest mass density \(\rho\) and the pressure \(p\).

◆ specific_internal_energy_from_density_and_pressure() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_from_density_and_pressure	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes the specific internal energy \(\epsilon\) from the rest mass density \(\rho\) and the pressure \(p\).

◆ specific_internal_energy_from_density_and_temperature() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_from_density_and_temperature	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes the specific internal energy \(\epsilon\) from the rest mass density \(\rho\) and the temperature \(T\).

◆ specific_internal_energy_from_density_and_temperature() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_from_density_and_temperature	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes the specific internal energy \(\epsilon\) from the rest mass density \(\rho\) and the temperature \(T\).

◆ specific_internal_energy_lower_bound()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_lower_bound ( const double rest_mass_density ) const

pure virtual

The lower bound of the specific internal energy that is valid for this EOS at the given rest mass density \(\rho\).

Implemented in EquationsOfState::DarkEnergyFluid< IsRelativistic >, EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ specific_internal_energy_upper_bound()

template<bool IsRelativistic>

virtual double EquationsOfState::EquationOfState< IsRelativistic, 2 >::specific_internal_energy_upper_bound ( const double rest_mass_density ) const

pure virtual

The upper bound of the specific internal energy that is valid for this EOS at the given rest mass density \(\rho\).

Implemented in EquationsOfState::DarkEnergyFluid< IsRelativistic >, EquationsOfState::IdealFluid< IsRelativistic >, EquationsOfState::IdealFluid< false >, and EquationsOfState::IdealFluid< true >.

◆ temperature_from_density_and_energy() [1/2]

template<bool IsRelativistic>

virtual Scalar< DataVector > EquationsOfState::EquationOfState< IsRelativistic, 2 >::temperature_from_density_and_energy	(	const Scalar< DataVector > &	,
		const Scalar< DataVector > &
	)		const

pure virtual

Computes the temperature \(T\) from the rest mass density \(\rho\) and the specific internal energy \(\epsilon\).

◆ temperature_from_density_and_energy() [2/2]

template<bool IsRelativistic>

virtual Scalar< double > EquationsOfState::EquationOfState< IsRelativistic, 2 >::temperature_from_density_and_energy	(	const Scalar< double > &	,
		const Scalar< double > &
	)		const

pure virtual

Computes the temperature \(T\) from the rest mass density \(\rho\) and the specific internal energy \(\epsilon\).

The documentation for this class was generated from the following file:

src/PointwiseFunctions/Hydro/EquationsOfState/EquationOfState.hpp

Public Types

Public Member Functions

Static Public Attributes

Detailed Description

Member Function Documentation

◆ baryon_mass()

◆ chi_from_density_and_energy() [1/2]

◆ chi_from_density_and_energy() [2/2]

◆ equilibrium_electron_fraction_from_density_temperature() [1/2]

◆ equilibrium_electron_fraction_from_density_temperature() [2/2]

◆ kappa_times_p_over_rho_squared_from_density_and_energy() [1/2]

◆ kappa_times_p_over_rho_squared_from_density_and_energy() [2/2]

◆ pressure_from_density_and_energy() [1/2]

◆ pressure_from_density_and_energy() [2/2]

◆ pressure_from_density_and_enthalpy() [1/2]

◆ pressure_from_density_and_enthalpy() [2/2]

◆ rest_mass_density_lower_bound()

◆ rest_mass_density_upper_bound()

◆ specific_enthalpy_lower_bound()

◆ specific_internal_energy_from_density_and_pressure() [1/2]

◆ specific_internal_energy_from_density_and_pressure() [2/2]

◆ specific_internal_energy_from_density_and_temperature() [1/2]

◆ specific_internal_energy_from_density_and_temperature() [2/2]

◆ specific_internal_energy_lower_bound()

◆ specific_internal_energy_upper_bound()

◆ temperature_from_density_and_energy() [1/2]

◆ temperature_from_density_and_energy() [2/2]