SpECTRE Documentation Coverage Report
Current view: top level - Evolution/Systems/NewtonianEuler - ConservativeFromPrimitive.hpp Hit Total Coverage
Commit: 9b01d30df5d2e946e7e38cc43c008be18ae9b1d2 Lines: 1 5 20.0 %
Date: 2024-04-23 04:54:49
Legend: Lines: hit not hit

          Line data    Source code
       1           0 : // Distributed under the MIT License.
       2             : // See LICENSE.txt for details.
       3             : 
       4             : #pragma once
       5             : 
       6             : #include <cstddef>
       7             : 
       8             : #include "DataStructures/Tensor/TypeAliases.hpp"
       9             : #include "Evolution/Systems/NewtonianEuler/TagsDeclarations.hpp"
      10             : #include "PointwiseFunctions/Hydro/Tags.hpp"
      11             : #include "Utilities/TMPL.hpp"
      12             : 
      13             : /// \cond
      14             : namespace gsl {
      15             : template <typename T>
      16             : class not_null;
      17             : }  // namespace gsl
      18             : 
      19             : class DataVector;
      20             : /// \endcond
      21             : 
      22             : // IWYU pragma: no_forward_declare Tensor
      23             : 
      24             : namespace NewtonianEuler {
      25             : 
      26             : /*!
      27             :  * \brief Compute the conservative variables from the primitive variables.
      28             :  *
      29             :  * \f{align*}
      30             :  * S^i &= \rho v^i \\
      31             :  * e &= \dfrac{1}{2}\rho v^2 + \rho\epsilon
      32             :  * \f}
      33             :  *
      34             :  * where \f$S^i\f$ is the momentum density, \f$e\f$ is the energy density,
      35             :  * \f$\rho\f$ is the mass density, \f$v^i\f$ is the velocity, \f$v^2\f$ is its
      36             :  * magnitude squared, and \f$\epsilon\f$ is the specific internal energy.
      37             :  * In addition, this method returns the mass density as a conservative.
      38             :  */
      39             : template <size_t Dim>
      40           1 : struct ConservativeFromPrimitive {
      41           0 :   using return_tags =
      42             :       tmpl::list<Tags::MassDensityCons, Tags::MomentumDensity<Dim>,
      43             :                  Tags::EnergyDensity>;
      44             : 
      45           0 :   using argument_tags =
      46             :       tmpl::list<hydro::Tags::RestMassDensity<DataVector>,
      47             :                  hydro::Tags::SpatialVelocity<DataVector, Dim>,
      48             :                  hydro::Tags::SpecificInternalEnergy<DataVector>>;
      49             : 
      50           0 :   static void apply(gsl::not_null<Scalar<DataVector>*> mass_density_cons,
      51             :                     gsl::not_null<tnsr::I<DataVector, Dim>*> momentum_density,
      52             :                     gsl::not_null<Scalar<DataVector>*> energy_density,
      53             :                     const Scalar<DataVector>& mass_density,
      54             :                     const tnsr::I<DataVector, Dim>& velocity,
      55             :                     const Scalar<DataVector>& specific_internal_energy);
      56             : };
      57             : }  // namespace NewtonianEuler

Generated by: LCOV version 1.14