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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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Vary K with n to preserve pressure at one explicitly selected physical reference density. More...
#include <polytropic.hpp>
Public Types | |
| using | OutputParameter = PolytropicConstant |
| using | DependencyParameters = ParameterList<PolytropicIndex> |
Public Member Functions | |
| PreservePressureAtReferenceDensity (dimensions::DensityValue density) | |
| Validate a positive finite thermodynamic pressure anchor. | |
| template<model::StellarModelType Model> requires Model::template | |
| contains_specification< eos::models::Polytrope > auto | bind (const Model &target) const |
| Freeze target values into an owning law whose exact endpoint retains the original K. | |
Private Attributes | |
| dimensions::DensityValue | m_density |
Vary K with n to preserve pressure at one explicitly selected physical reference density.
| using serif::solver::continuation::PreservePressureAtReferenceDensity::DependencyParameters = ParameterList<PolytropicIndex> |
| using serif::solver::continuation::PreservePressureAtReferenceDensity::OutputParameter = PolytropicConstant |
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inlineexplicit |
Validate a positive finite thermodynamic pressure anchor.
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inlinenodiscard |
Freeze target values into an owning law whose exact endpoint retains the original K.
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private |