SpECTRE Documentation Coverage Report
Current view: top level - PointwiseFunctions/Hydro/EquationsOfState - Equilibrium3D.hpp Coverage Total Hit
Commit: 0d1d717af84a81fb1284a20c4013708fe85cc2f0 Lines: 39.5 % 38 15
Test Date: 2026-10-22 17:29:42
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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/Tensor.hpp"
      19              : #include "DataStructures/Tensor/TypeAliases.hpp"
      20              : #include "Options/String.hpp"
      21              : #include "PointwiseFunctions/Hydro/EquationsOfState/EquationOfState.hpp"
      22              : #include "PointwiseFunctions/Hydro/Units.hpp"
      23              : #include "Utilities/Serialization/CharmPupable.hpp"
      24              : #include "Utilities/TMPL.hpp"
      25              : 
      26              : namespace EquationsOfState {
      27              : /*!
      28              :  * \ingroup EquationsOfStateGroup
      29              :  * \brief A 3D equation of state representing a fluid in compositional
      30              :  * equalibrium.
      31              :  *
      32              :  *
      33              :  * The equation of state takes the form
      34              :  *
      35              :  * \f[
      36              :  * p = p (T, rho, Y_e) = p(T, rho, Y_e= Y_{e, \beta})
      37              :  * \f]
      38              :  *
      39              :  * where \f$\rho\f$ is the rest mass density and  \f$T\f$ is the
      40              :  * temperaturee;   \f$Y_e\f$  the electron fraction,  is not
      41              :  * used, and therefore this evaluating this EoS at any arbtirary
      42              :  * electron fraction is equivalent to evaluating it  in beta equalibrium
      43              :  *
      44              :  */
      45              : template <typename EquilEos>
      46            1 : class Equilibrium3D : public EquationOfState<EquilEos::is_relativistic, 3> {
      47              :  public:
      48            0 :   static constexpr size_t thermodynamic_dim = 3;
      49            0 :   static constexpr bool is_relativistic = EquilEos::is_relativistic;
      50            0 :   static std::string name() {
      51              :     return "Equilibrium3D(" + pretty_type::name<EquilEos>() + ")";
      52              :   }
      53            0 :   static constexpr Options::String help = {
      54              :       "An 3D EoS which is independent of electron fraction. "
      55              :       "Contains an underlying 2D EoS which is dependent only "
      56              :       "on rest mass density and temperature/internal energy."};
      57              : 
      58            0 :   struct UnderlyingEos {
      59            0 :     using type = EquilEos;
      60            0 :     static std::string name() { return pretty_type::short_name<EquilEos>(); }
      61            0 :     static constexpr Options::String help{
      62              :         "The underlying Eos which is being represented as a "
      63              :         "3D Eos.  Must be a 2D EoS"};
      64              :   };
      65              : 
      66            0 :   using options = tmpl::list<UnderlyingEos>;
      67              : 
      68            0 :   Equilibrium3D() = default;
      69            0 :   Equilibrium3D(const Equilibrium3D&) = default;
      70            0 :   Equilibrium3D& operator=(const Equilibrium3D&) = default;
      71            0 :   Equilibrium3D(Equilibrium3D&&) = default;
      72            0 :   Equilibrium3D& operator=(Equilibrium3D&&) = default;
      73            0 :   ~Equilibrium3D() override = default;
      74              : 
      75            0 :   explicit Equilibrium3D(const EquilEos& underlying_eos)
      76              :       : underlying_eos_(underlying_eos){};
      77              : 
      78              :   EQUATION_OF_STATE_FORWARD_DECLARE_MEMBERS(Equilibrium3D, 3)
      79              : 
      80            0 :   std::unique_ptr<EquationOfState<EquilEos::is_relativistic, 3>> get_clone()
      81              :       const override;
      82              : 
      83            0 :   bool is_equal(
      84              :       const EquationOfState<EquilEos::is_relativistic, 3>& rhs) const override;
      85              : 
      86              :   /// \brief Returns `true` if the EOS is barotropic
      87            1 :   bool is_barotropic() const override { return false; }
      88              : 
      89              :   /// \brief Returns `true` if the EOS is in beta-equilibrium
      90            1 :   bool is_equilibrium() const override { return true; }
      91              : 
      92            0 :   bool operator==(const Equilibrium3D<EquilEos>& rhs) const;
      93              : 
      94            0 :   bool operator!=(const Equilibrium3D<EquilEos>& rhs) const;
      95              :   /// @{
      96              :   /*!
      97              :    * Computes the electron fraction in beta-equilibrium \f$Y_e^{\rm eq}\f$ from
      98              :    * the rest mass density \f$\rho\f$ and the temperature \f$T\f$.
      99              :    */
     100            1 :   Scalar<double> equilibrium_electron_fraction_from_density_temperature(
     101              :       const Scalar<double>& rest_mass_density,
     102              :       const Scalar<double>& temperature) const override{
     103              :     return underlying_eos_
     104              :         .equilibrium_electron_fraction_from_density_temperature(
     105              :             rest_mass_density, temperature);
     106              :   }
     107              : 
     108            1 :   Scalar<DataVector> equilibrium_electron_fraction_from_density_temperature(
     109              :       const Scalar<DataVector>& rest_mass_density,
     110              :       const Scalar<DataVector>& temperature) const override {
     111              :     return underlying_eos_
     112              :         .equilibrium_electron_fraction_from_density_temperature(
     113              :             rest_mass_density, temperature);
     114              :   }
     115              :   /// @}
     116              :   //
     117              : 
     118            0 :   WRAPPED_PUPable_decl_base_template(  // NOLINT
     119              :       SINGLE_ARG(EquationOfState<EquilEos::is_relativistic, 3>), Equilibrium3D);
     120              : 
     121              :   /// The lower bound of the electron fraction that is valid for this EOS
     122            1 :   double electron_fraction_lower_bound() const override { return 0.0; }
     123              : 
     124              :   /// The upper bound of the electron fraction that is valid for this EOS
     125            1 :   double electron_fraction_upper_bound() const override { return 1.0; }
     126              : 
     127              :   /// The lower bound of the rest mass density that is valid for this EOS
     128            1 :   double rest_mass_density_lower_bound() const override {
     129              :     return underlying_eos_.rest_mass_density_lower_bound();
     130              :   }
     131              : 
     132              :   /// The upper bound of the rest mass density that is valid for this EOS
     133            1 :   double rest_mass_density_upper_bound() const override {
     134              :     return underlying_eos_.rest_mass_density_upper_bound();
     135              :   }
     136              : 
     137              :   /// The lower bound of the temperature that is valid for this EOS
     138            1 :   double temperature_lower_bound() const override {
     139              :     return underlying_eos_.temperature_lower_bound();
     140              :   }
     141              : 
     142              :   /// The upper bound of the temperature that is valid for this EOS
     143            1 :   double temperature_upper_bound() const override {
     144              :     return underlying_eos_.temperature_upper_bound();
     145              :   }
     146              : 
     147              :   /// The lower bound of the specific internal energy that is valid for this EOS
     148              :   /// at the given rest mass density \f$\rho\f$ and electron fraction \f$Y_e\f$
     149            1 :   double specific_internal_energy_lower_bound(
     150              :       const double rest_mass_density,
     151              :       const double /*electron_fraction*/) const override {
     152              :     return underlying_eos_.specific_internal_energy_lower_bound(
     153              :         rest_mass_density);
     154              :   }
     155              : 
     156              :   /// The upper bound of the specific internal energy that is valid for this EOS
     157              :   /// at the given rest mass density \f$\rho\f$
     158            1 :   double specific_internal_energy_upper_bound(
     159              :       const double rest_mass_density,
     160              :       const double /*electron_fraction*/) const override {
     161              :     return underlying_eos_.specific_internal_energy_upper_bound(
     162              :         rest_mass_density);
     163              :   }
     164              : 
     165              :   /// The lower bound of the specific enthalpy that is valid for this EOS
     166            1 :   double specific_enthalpy_lower_bound() const override {
     167              :     return underlying_eos_.specific_enthalpy_lower_bound();
     168              :   }
     169              : 
     170              :   /// The baryon mass for this EoS
     171            1 :   double baryon_mass() const override { return underlying_eos_.baryon_mass(); }
     172              : 
     173              :  private:
     174              :   EQUATION_OF_STATE_FORWARD_DECLARE_MEMBER_IMPLS(3)
     175            0 :   EquilEos underlying_eos_;
     176              : };
     177              : /// \cond
     178              : template <typename EquilEos>
     179              : PUP::able::PUP_ID EquationsOfState::Equilibrium3D<EquilEos>::my_PUP_ID = 0;
     180              : /// \endcond
     181              : }  // namespace EquationsOfState
        

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