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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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#include <cmath>#include <optional>#include <string_view>#include <utility>#include "serif/dimensions/type_alias.hpp"#include "serif/discretization/blocks/fields.hpp"#include "serif/eos/evaluation.hpp"#include "serif/eos/exceptions.hpp"#include "serif/eos/relations/relations.hpp"#include "serif/equations/companion.hpp"#include "serif/equations/contributions.hpp"#include "serif/equations/point.hpp"#include "serif/equations/rigid_rotation.hpp"#include "serif/utils/error/errors.hpp"Classes | |
| class | serif::equations::BarotropicDensityBalance< EOS > |
| Enforce A(rho) - A(rho_surface) + Phi - Omega^2 Psi - U_surface = 0 using density test values. This closure assumes a connected barotrope in rigid rotation. More... | |
Namespaces | |
| namespace | serif |
| namespace | serif::equations |