Fix the primitive variables to an atmosphere in low density regions. More...

#include <FixToAtmosphere.hpp>

Classes
struct	DensityCutoff
	Rest mass density at which to impose the atmosphere. Should be greater than or equal to the density of the atmosphere. More...

struct	DensityOfAtmosphere
	Rest mass density of the atmosphere. More...

struct	KappaLimiting
	If set then we apply a limiting precodure on the temperature near the atmosphere based on essentially limiting the polytropic constant in a Gamma-law equation of state. More...

struct	KappaLimitingOptions
	Options for limiting the temperature in the atmosphere by effectively limiting the polytropic constant, with a generalization for finite temperature equations of state. More...

struct	VelocityLimiting

struct	VelocityLimitingOptions
	Limit the velocity in and near the atmosphere. More...

Public Types
using	options = tmpl::list< DensityOfAtmosphere, DensityCutoff, VelocityLimiting, KappaLimiting >

using	return_tags = tmpl::list< hydro::Tags::RestMassDensity< DataVector >, hydro::Tags::SpecificInternalEnergy< DataVector >, hydro::Tags::SpatialVelocity< DataVector, Dim >, hydro::Tags::LorentzFactor< DataVector >, hydro::Tags::Pressure< DataVector >, hydro::Tags::Temperature< DataVector > >

using	argument_tags = tmpl::list< hydro::Tags::ElectronFraction< DataVector >, gr::Tags::SpatialMetric< DataVector, Dim >, hydro::Tags::GrmhdEquationOfState >

Public Member Functions
	FixToAtmosphere (double density_of_atmosphere, double density_cutoff, std::optional< VelocityLimitingOptions > velocity_limiting, std::optional< KappaLimitingOptions > kappa_limiting, const Options::Context &context={})

	FixToAtmosphere (const FixToAtmosphere &)=default

FixToAtmosphere &	operator= (const FixToAtmosphere &)=default

	FixToAtmosphere (FixToAtmosphere &&)=default

FixToAtmosphere &	operator= (FixToAtmosphere &&)=default

void	pup (PUP::er &p)

template<size_t ThermodynamicDim>
void	operator() (gsl::not_null< Scalar< DataVector > * > rest_mass_density, gsl::not_null< Scalar< DataVector > * > specific_internal_energy, gsl::not_null< tnsr::I< DataVector, Dim, Frame::Inertial > * > spatial_velocity, gsl::not_null< Scalar< DataVector > * > lorentz_factor, gsl::not_null< Scalar< DataVector > * > pressure, gsl::not_null< Scalar< DataVector > * > temperature, const Scalar< DataVector > &electron_fraction, const tnsr::ii< DataVector, Dim, Frame::Inertial > &spatial_metric, const EquationsOfState::EquationOfState< true, ThermodynamicDim > &equation_of_state) const


double	density_of_atmosphere () const
	Other algorithmic decisions may depend on the atmosphere treatment so provide access to the values.

double	density_cutoff () const
	Other algorithmic decisions may depend on the atmosphere treatment so provide access to the values.

const std::optional< VelocityLimitingOptions > &	velocity_limiting () const
	Other algorithmic decisions may depend on the atmosphere treatment so provide access to the values.

const std::optional< KappaLimitingOptions > &	kappa_limiting () const
	Other algorithmic decisions may depend on the atmosphere treatment so provide access to the values.

Static Public Attributes
static constexpr Options::String	help

Friends
template<size_t SpatialDim>
bool	operator== (const FixToAtmosphere< SpatialDim > &lhs, const FixToAtmosphere< SpatialDim > &rhs)

Detailed Description

template<size_t Dim>
class VariableFixing::FixToAtmosphere< Dim >

Fix the primitive variables to an atmosphere in low density regions.

If the rest mass density is below \(\rho_{\textrm{cutoff}}\) (DensityCutoff), it is set to \(\rho_{\textrm{atm}}\) (DensityOfAtmosphere), and the pressure, and specific internal energy (for one-dimensional equations of state) are adjusted to satisfy the equation of state. For a two-dimensional equation of state, the specific internal energy is set to zero.

Member Data Documentation

◆ help

template<size_t Dim>

constexpr Options::String VariableFixing::FixToAtmosphere< Dim >::help

staticconstexpr

Initial value:

= {
      "If the rest mass density is below DensityCutoff, it is set\n"
      "to DensityOfAtmosphere, and the pressure, and specific internal energy\n"
      "(for one-dimensional equations of state) are\n"
      "adjusted to satisfy the equation of state. For a two-dimensional\n"
      "equation of state, the specific internal energy is set to zero.\n"
      "In addition, the spatial velocity is set to zero, and the Lorentz\n"
      "factor is set to one.\n"}

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

src/Evolution/VariableFixing/FixToAtmosphere.hpp

Classes

Public Types

Public Member Functions

Static Public Attributes

Friends

Detailed Description

Member Data Documentation

◆ help