SpECTRE Documentation Coverage Report
Current view: top level - Evolution/Systems/GeneralizedHarmonic - SphericalShellPowerMonitor.hpp Hit Total Coverage
Commit: ecb8a275e1aebab77dcce48a5e098ed4e486ab4b Lines: 4 12 33.3 %
Date: 2026-08-22 01:05:40
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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 <array>
       7             : #include <cstddef>
       8             : #include <optional>
       9             : 
      10             : #include "DataStructures/DataVector.hpp"
      11             : #include "DataStructures/SimpleSparseMatrix.hpp"
      12             : #include "DataStructures/Tensor/TypeAliases.hpp"
      13             : #include "DataStructures/Variables.hpp"
      14             : #include "Evolution/Systems/GeneralizedHarmonic/ApplyTensorYlmFilter.hpp"
      15             : #include "NumericalAlgorithms/Spectral/Mesh.hpp"
      16             : #include "Utilities/Gsl.hpp"
      17             : 
      18             : /// \cond
      19             : class DataVector;
      20             : namespace ylm {
      21             : class Spherepack;
      22             : }  // namespace ylm
      23             : /// \endcond
      24             : 
      25             : namespace gh::power_monitor {
      26             : 
      27             : /// Holds separate GH shell power monitors for each evolved GH variable.
      28           1 : struct GhShellPowerMonitors {
      29           0 :   std::array<DataVector, 2> spacetime_metric{};
      30           0 :   std::array<DataVector, 2> pi{};
      31           0 :   std::array<DataVector, 2> phi{};
      32             : };
      33             : 
      34             : /// Sparse matrices for Cartesian-component to TensorYlm-basis transforms.
      35           1 : struct CartToSphereMatrices {
      36           0 :   std::optional<SimpleSparseMatrix> i{};
      37           0 :   std::optional<SimpleSparseMatrix> ii{};
      38           0 :   std::optional<SimpleSparseMatrix> ij{};
      39           0 :   std::optional<SimpleSparseMatrix> ijj{};
      40             : };
      41             : 
      42             : /// Fill any missing Cartesian-to-TensorYlm sparse matrices with Spherepack
      43             : /// normalization.
      44           1 : void fill_cart_to_sphere_matrices(gsl::not_null<CartToSphereMatrices*> matrices,
      45             :                                   size_t ell_max);
      46             : 
      47             : /*!
      48             :  * \brief Compute radial and angular power monitors for the evolved GH
      49             :  * variables on a spherical shell.
      50             :  *
      51             :  * Each monitor is an array containing the radial monitor at index 0 and the
      52             :  * angular monitor at index 1. Radial monitors are computed from the original
      53             :  * GH variables, matching SpEC's shell radial power monitor behavior. Angular
      54             :  * monitors are computed after transforming the GH variables to TensorYlm
      55             :  * coefficients. The Cartesian-to-TensorYlm matrices are filled on first use
      56             :  * and reused on subsequent calls.
      57             :  */
      58           1 : GhShellPowerMonitors gh_shell_power_monitors(
      59             :     gsl::not_null<CartToSphereMatrices*> cart_to_sphere_matrices,
      60             :     const Variables<ylm::TensorYlm::filter_detail::gh_spacetime_vars_list>&
      61             :         gh_vars,
      62             :     const Mesh<3>& mesh,
      63             :     const InverseJacobian<DataVector, 3, Frame::Inertial, Frame::Grid>&
      64             :         jac_inertial_to_grid);
      65             : 
      66             : }  // namespace gh::power_monitor

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