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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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Namespaces | |
| namespace | detail |
Classes | |
| struct | Configuration |
| struct | InfinityRows |
| Potential rows replaced by the zero trace at compactified infinity. More... | |
| struct | PreparedSystem |
| struct | SurfaceRows |
| Reduced equation rows whose volume residual is replaced by the selected surface condition. More... | |
Concepts | |
| concept | ReferenceResolvable |
| Check model-provided reference requirements before instantiating numerical preparation. | |
Typedefs | |
| template<typename Selection, typename Coordinates, typename Bound> | |
| using | PlanFor = typename detail::SelectPlan<Selection, Coordinates, Bound>::Type |
| Compile automatic physics-aware rules or retain the user's complete explicit plan. | |
| template<typename Plan> | |
| using | MetricsFor |
| Assemble each metric once even when several state and residual rules share it. | |
Functions | |
| template<typename Options, typename Discretization, typename... Metrics> | |
| auto | make_inputs (std::shared_ptr< const Options > options, const Discretization &discretization, utils::dependencies::KeyList< Metrics... >) |
| Keep the immutable configuration alive and reference metrics separate from candidate coefficients. | |
| template<typename NormalizationPlan, typename Bound, typename Options, typename Layout, typename... Metrics> | |
| auto | make_computations (const Bound &bound, const Options &options, const Layout &layout, utils::dependencies::KeyList< Metrics... >) |
| Compose normalization into the physical graph, including the selected surface row replacement. | |
| template<typename Mass, typename Density, StellarModelType Model> requires detail::ReferenceAvailable<Mass, Model, FixedTotalMass> && std::same_as<Density, dimensions::DensityValue> | |
| auto | resolve_reference (const solver::normalization::LaneEmdenApproximation< Mass, Density > &scheme, const Model &model) |
| Resolve the Lane–Emden reference from explicit inputs or the model's mass target; no model prescribes central density. | |
| template<solver::normalization::ReferenceScheme Scheme, StellarModelType Model> | |
| Scheme | resolve_reference (const Scheme &scheme, const Model &) |
| Explicit or custom reference schemes need no model-specific defaults. | |
| template<typename Options, StellarModelType Model> requires ReferenceResolvable<Options, Model> | |
| auto | resolve_configuration (Options options, const Model &model) |
| Freeze resolved reference choices while retaining the deduced coordinate and plan types. | |
| using serif::model::normalization::MetricsFor |
Assemble each metric once even when several state and residual rules share it.
| using serif::model::normalization::PlanFor = typename detail::SelectPlan<Selection, Coordinates, Bound>::Type |
Compile automatic physics-aware rules or retain the user's complete explicit plan.
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nodiscard |
Compose normalization into the physical graph, including the selected surface row replacement.
|
nodiscard |
Keep the immutable configuration alive and reference metrics separate from candidate coefficients.
|
nodiscard |
Freeze resolved reference choices while retaining the deduced coordinate and plan types.
|
nodiscard |
Explicit or custom reference schemes need no model-specific defaults.
|
nodiscard |
Resolve the Lane–Emden reference from explicit inputs or the model's mass target; no model prescribes central density.