equations.hpp File Reference

#include "serif/utils/serialize/physics.hpp"
#include "serif/equations/equations.hpp"
#include "serif/equations/registry.hpp"

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Classes
struct	serif::utils::serialize::Serializer< equations::BarycenterConstraint< Axis, Row > >
struct	serif::utils::serialize::Serializer< equations::PointMassCompanion >
struct	serif::utils::serialize::Serializer< equations::BarotropicDensityBalance< EOS > >
struct	serif::utils::serialize::Serializer< equations::PrimalPoissonBalance >
struct	serif::utils::serialize::Serializer< equations::SurfacePotentialBalance >
struct	serif::utils::serialize::Serializer< equations::MassNormalization >
struct	serif::utils::serialize::Serializer< equations::AngularMomentumConstraint >
struct	serif::utils::serialize::Serializer< equations::EquationRegistry< Equations... > >

Namespaces
namespace	serif
namespace	serif::utils
namespace	serif::utils::serialize
namespace	serif::utils::serialize::detail

Functions
Result< std::optional< equations::PointMassCompanion > >	serif::utils::serialize::detail::read_companion (const Node &node)
	Archives written before companions existed have no companion field; a single star stays one.
Node	serif::utils::serialize::detail::with_companion (Node node, const std::optional< equations::PointMassCompanion > &companion)
	Record the companion only when there is one, so single-star archives keep their schema.