SpECTRE Documentation Coverage Report
Current view: top level - PointwiseFunctions/Hydro/EquationsOfState - Equilibrium3D.hpp Hit Total Coverage
Commit: 8f6d7ed2ad592dd78354983fd8e5ec2be7abb468 Lines: 14 37 37.8 %
Date: 2024-05-02 15:57:06
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          Line data    Source code
       1           0 : // Distributed under the MIT License.
       2             : // See LICENSE.txt for details.
       3             : 
       4             : #pragma once
       5             : 
       6             : #include <boost/preprocessor/arithmetic/dec.hpp>
       7             : #include <boost/preprocessor/arithmetic/inc.hpp>
       8             : #include <boost/preprocessor/control/expr_iif.hpp>
       9             : #include <boost/preprocessor/list/adt.hpp>
      10             : #include <boost/preprocessor/repetition/for.hpp>
      11             : #include <boost/preprocessor/repetition/repeat.hpp>
      12             : #include <boost/preprocessor/tuple/to_list.hpp>
      13             : #include <cstddef>
      14             : #include <limits>
      15             : #include <memory>
      16             : #include <pup.h>
      17             : 
      18             : #include "DataStructures/Tensor/TypeAliases.hpp"
      19             : #include "Options/String.hpp"
      20             : #include "PointwiseFunctions/Hydro/EquationsOfState/EquationOfState.hpp"
      21             : #include "PointwiseFunctions/Hydro/Units.hpp"
      22             : #include "Utilities/Serialization/CharmPupable.hpp"
      23             : #include "Utilities/TMPL.hpp"
      24             : 
      25             : namespace EquationsOfState {
      26             : /*!
      27             :  * \ingroup EquationsOfStateGroup
      28             :  * \brief A 3D equation of state representing a fluid in compositional
      29             :  * equalibrium.
      30             :  *
      31             :  *
      32             :  * The equation of state takes the form
      33             :  *
      34             :  * \f[
      35             :  * p = p (T, rho, Y_e) = p(T, rho, Y_e= Y_{e, \beta})
      36             :  * \f]
      37             :  *
      38             :  * where \f$\rho\f$ is the rest mass density and  \f$T\f$ is the
      39             :  * temperaturee;   \f$Y_e\f$  the electron fraction,  is not
      40             :  * used, and therefore this evaluating this EoS at any arbtirary
      41             :  * electron fraction is equivalent to evaluating it  in beta equalibrium
      42             :  *
      43             :  */
      44             : template <typename EquilEos>
      45           1 : class Equilibrium3D : public EquationOfState<EquilEos::is_relativistic, 3> {
      46             :  public:
      47           0 :   static constexpr size_t thermodynamic_dim = 3;
      48           0 :   static constexpr bool is_relativistic = EquilEos::is_relativistic;
      49           0 :   static std::string name() {
      50             :     return "Equilibrium3D(" + pretty_type::name<EquilEos>() + ")";
      51             :   }
      52           0 :   static constexpr Options::String help = {
      53             :       "An 3D EoS which is independent of electron fraction. "
      54             :       "Contains an underlying 2D EoS which is dependent only "
      55             :       "on rest mass density and temperature/internal energy."};
      56             : 
      57           0 :   struct UnderlyingEos {
      58           0 :     using type = EquilEos;
      59           0 :     static std::string name() { return pretty_type::short_name<EquilEos>(); }
      60           0 :     static constexpr Options::String help{
      61             :         "The underlying Eos which is being represented as a "
      62             :         "3D Eos.  Must be a 2D EoS"};
      63             :   };
      64             : 
      65           0 :   using options = tmpl::list<UnderlyingEos>;
      66             : 
      67           0 :   Equilibrium3D() = default;
      68           0 :   Equilibrium3D(const Equilibrium3D&) = default;
      69           0 :   Equilibrium3D& operator=(const Equilibrium3D&) = default;
      70           0 :   Equilibrium3D(Equilibrium3D&&) = default;
      71           0 :   Equilibrium3D& operator=(Equilibrium3D&&) = default;
      72           0 :   ~Equilibrium3D() override = default;
      73             : 
      74           0 :   explicit Equilibrium3D(const EquilEos& underlying_eos)
      75             :       : underlying_eos_(underlying_eos){};
      76             : 
      77             :   EQUATION_OF_STATE_FORWARD_DECLARE_MEMBERS(Equilibrium3D, 3)
      78             : 
      79           0 :   std::unique_ptr<EquationOfState<EquilEos::is_relativistic, 3>> get_clone()
      80             :       const override;
      81             : 
      82           0 :   bool is_equal(
      83             :       const EquationOfState<EquilEos::is_relativistic, 3>& rhs) const override;
      84             : 
      85             :   /// \brief Returns `true` if the EOS is barotropic
      86           1 :   bool is_barotropic() const override { return false; }
      87             : 
      88           0 :   bool operator==(const Equilibrium3D<EquilEos>& rhs) const;
      89             : 
      90           0 :   bool operator!=(const Equilibrium3D<EquilEos>& rhs) const;
      91             :   /// @{
      92             :   /*!
      93             :    * Computes the electron fraction in beta-equilibrium \f$Y_e^{\rm eq}\f$ from
      94             :    * the rest mass density \f$\rho\f$ and the temperature \f$T\f$.
      95             :    */
      96           1 :   Scalar<double> equilibrium_electron_fraction_from_density_temperature(
      97             :       const Scalar<double>& rest_mass_density,
      98             :       const Scalar<double>& temperature) const {
      99             :     return underlying_eos_
     100             :         .equilibrium_electron_fraction_from_density_temperature(
     101             :             rest_mass_density, temperature);
     102             :   }
     103             : 
     104           1 :   Scalar<DataVector> equilibrium_electron_fraction_from_density_temperature(
     105             :       const Scalar<DataVector>& rest_mass_density,
     106             :       const Scalar<DataVector>& temperature) const {
     107             :     return underlying_eos_
     108             :         .equilibrium_electron_fraction_from_density_temperature(
     109             :             rest_mass_density, temperature);
     110             :   }
     111             :   /// @}
     112             :   //
     113             : 
     114           0 :   WRAPPED_PUPable_decl_base_template(  // NOLINT
     115             :       SINGLE_ARG(EquationOfState<EquilEos::is_relativistic, 3>), Equilibrium3D);
     116             : 
     117             :   /// The lower bound of the electron fraction that is valid for this EOS
     118           1 :   double electron_fraction_lower_bound() const override { return 0.0; }
     119             : 
     120             :   /// The upper bound of the electron fraction that is valid for this EOS
     121           1 :   double electron_fraction_upper_bound() const override { return 1.0; }
     122             : 
     123             :   /// The lower bound of the rest mass density that is valid for this EOS
     124           1 :   double rest_mass_density_lower_bound() const override {
     125             :     return underlying_eos_.rest_mass_density_lower_bound();
     126             :   }
     127             : 
     128             :   /// The upper bound of the rest mass density that is valid for this EOS
     129           1 :   double rest_mass_density_upper_bound() const override {
     130             :     return underlying_eos_.rest_mass_density_upper_bound();
     131             :   }
     132             : 
     133             :   /// The lower bound of the temperature that is valid for this EOS
     134           1 :   double temperature_lower_bound() const override {
     135             :     return underlying_eos_.temperature_lower_bound();
     136             :   }
     137             : 
     138             :   /// The upper bound of the temperature that is valid for this EOS
     139           1 :   double temperature_upper_bound() const override {
     140             :     return underlying_eos_.temperature_upper_bound();
     141             :   }
     142             : 
     143             :   /// The lower bound of the specific internal energy that is valid for this EOS
     144             :   /// at the given rest mass density \f$\rho\f$ and electron fraction \f$Y_e\f$
     145           1 :   double specific_internal_energy_lower_bound(
     146             :       const double rest_mass_density,
     147             :       const double /*electron_fraction*/) const override {
     148             :     return underlying_eos_.specific_internal_energy_lower_bound(
     149             :         rest_mass_density);
     150             :   }
     151             : 
     152             :   /// The upper bound of the specific internal energy that is valid for this EOS
     153             :   /// at the given rest mass density \f$\rho\f$
     154           1 :   double specific_internal_energy_upper_bound(
     155             :       const double rest_mass_density,
     156             :       const double /*electron_fraction*/) const override {
     157             :     return underlying_eos_.specific_internal_energy_upper_bound(
     158             :         rest_mass_density);
     159             :   }
     160             : 
     161             :   /// The lower bound of the specific enthalpy that is valid for this EOS
     162           1 :   double specific_enthalpy_lower_bound() const override {
     163             :     return underlying_eos_.specific_enthalpy_lower_bound();
     164             :   }
     165             : 
     166             :   /// The baryon mass for this EoS
     167           1 :   double baryon_mass() const override { return underlying_eos_.baryon_mass(); }
     168             : 
     169             :  private:
     170             :   EQUATION_OF_STATE_FORWARD_DECLARE_MEMBER_IMPLS(3)
     171           0 :   EquilEos underlying_eos_;
     172             : };
     173             : /// \cond
     174             : template <typename EquilEos>
     175             : PUP::able::PUP_ID EquationsOfState::Equilibrium3D<EquilEos>::my_PUP_ID = 0;
     176             : /// \endcond
     177             : }  // namespace EquationsOfState

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