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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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The value of this global scalar is the effective surface-potential level Us. Its paired residual enforces the prescribed total mass. The surface equation supplies the dependence on Us, while the mass equation integrates the density over the star. More...
#include <fields.hpp>
Public Types | |
| using | Support = domain::StellarDomains |
| The support of the mass normalization term is the stellar domains since we only want to enforce the mass normalization condition in the stellar domains. | |
| using | Quantity = dimensions::GravitationalPotential |
| Physical units of the solved effective potential level, distinct from the mass residual units. | |
Public Types inherited from serif::discretization::blocks::term< barotropic_constant > | |
| using | field_type |
Static Public Attributes | |
| static constexpr std::string_view | name = meta::type_name<mass_normalization>() |
| Compile time reflected name of the term. | |
| static constexpr std::string_view | symbol = "Us" |
| Compile time symbol for the effective surface-potential level. | |
The value of this global scalar is the effective surface-potential level Us. Its paired residual enforces the prescribed total mass. The surface equation supplies the dependence on Us, while the mass equation integrates the density over the star.
| using serif::discretization::blocks::barotropic_constant::mass_normalization::Quantity = dimensions::GravitationalPotential |
Physical units of the solved effective potential level, distinct from the mass residual units.
| using serif::discretization::blocks::barotropic_constant::mass_normalization::Support = domain::StellarDomains |
The support of the mass normalization term is the stellar domains since we only want to enforce the mass normalization condition in the stellar domains.
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staticconstexpr |
Compile time reflected name of the term.
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staticconstexpr |
Compile time symbol for the effective surface-potential level.