SpECTRE Documentation Coverage Report
Current view: top level - Evolution/Systems/GrMhd/ValenciaDivClean - NewmanHamlin.hpp Coverage Total Hit
Commit: 0d1d717af84a81fb1284a20c4013708fe85cc2f0 Lines: 16.7 % 6 1
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 <cstddef>
       7              : #include <optional>
       8              : #include <string>
       9              : 
      10              : #include "Evolution/Systems/GrMhd/ValenciaDivClean/PrimitiveRecoveryData.hpp"
      11              : 
      12              : /// \cond
      13              : namespace EquationsOfState {
      14              : template <bool, size_t>
      15              : class EquationOfState;
      16              : }  // namespace EquationsOfState
      17              : namespace grmhd::ValenciaDivClean {
      18              : class PrimitiveFromConservativeOptions;
      19              : }  // namespace grmhd::ValenciaDivClean
      20              : /// \endcond
      21              : 
      22              : namespace grmhd::ValenciaDivClean::PrimitiveRecoverySchemes {
      23              : 
      24              : /*!
      25              :  * \brief Compute the primitive variables from the conservative variables using
      26              :  * the scheme of [Newman and Hamlin, SIAM J. Sci. Comput., 36(4)
      27              :  * B661-B683 (2014)](https://epubs.siam.org/doi/10.1137/140956749).
      28              :  *
      29              :  * In the Newman and Hamlin paper, `tau` is \f$e - \rho W\f$,
      30              :  * `momentum_density_squared` is\f${\cal M}^2\f$,
      31              :  * `momentum_density_dot_magnetic_field` is \f${\cal T}\f$,
      32              :  * `magnetic_field_squared` is \f${\cal B}^2\f$, and
      33              :  * `rest_mass_density_times_lorentz_factor` is \f${\tilde \rho}\f$.
      34              :  * Furthermore, the returned `PrimitiveRecoveryData.rho_h_w_squared` is \f${\cal
      35              :  * L}\f$.
      36              :  *
      37              :  * In terms of the conservative variables (in our notation):
      38              :  * \f{align}
      39              :  * e = & \frac{{\tilde D} + {\tilde \tau}}{\sqrt{\gamma}} \\
      40              :  * {\cal M}^2 = & \frac{\gamma^{mn} {\tilde S}_m {\tilde S}_n}{\gamma} \\
      41              :  * {\cal T} = & \frac{{\tilde B}^m {\tilde S}_m}{\gamma} \\
      42              :  * {\cal B}^2 = & \frac{\gamma_{mn} {\tilde B}^m {\tilde B}^n}{\gamma} \\
      43              :  * {\tilde \rho} = & \frac{\tilde D}{\sqrt{\gamma}}
      44              :  * \f}
      45              :  *
      46              :  * where the conserved variables \f${\tilde D}\f$, \f${\tilde S}_i\f$,
      47              :  * \f${\tilde \tau}\f$, and \f${\tilde B}^i\f$ are a generalized mass-energy
      48              :  * density, momentum density, specific internal energy density, and magnetic
      49              :  * field, and \f$\gamma\f$ and \f$\gamma^{mn}\f$ are the determinant and inverse
      50              :  * of the spatial metric \f$\gamma_{mn}\f$.
      51              :  */
      52            1 : class NewmanHamlin {
      53              :  public:
      54              :   template <bool EnforcePhysicality, typename EosType>
      55            0 :   static std::optional<PrimitiveRecoveryData> apply(
      56              :       double initial_guess_for_pressure, double tau,
      57              :       double momentum_density_squared,
      58              :       double momentum_density_dot_magnetic_field, double magnetic_field_squared,
      59              :       double rest_mass_density_times_lorentz_factor, double electron_fraction,
      60              :       const EosType& equation_of_state,
      61              :       const grmhd::ValenciaDivClean::PrimitiveFromConservativeOptions&
      62              :           primitive_from_conservative_options);
      63              : 
      64            0 :   static const std::string name() { return "Newman Hamlin"; }
      65              : 
      66              :  private:
      67            0 :   static constexpr size_t max_iterations_ = 50;
      68            0 :   static constexpr double relative_tolerance_ = 1.e-10;
      69              : };
      70              : }  // namespace grmhd::ValenciaDivClean::PrimitiveRecoverySchemes
        

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