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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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#include "serif/solver/continuation/family.hpp"#include "serif/solver/continuation/stellar_parameters.hpp"Classes | |
| class | serif::solver::continuation::PreservePressureAtReferenceDensity |
| Vary K with n to preserve pressure at one explicitly selected physical reference density. More... | |
Namespaces | |
| namespace | serif |
| namespace | serif::solver |
| namespace | serif::solver::continuation |
Functions | |
| auto | serif::solver::continuation::preserve_pressure_at_reference_density (dimensions::DensityValue density) |
| Choose a pressure-preserving physical EOS family, independently of numerical normalization. | |