This field holds the effective potential level on the stellar isobar. The level is solved together with the fixed total mass. The barotropic_constant name is retained as an internal coordinate identity. In the density formulation its value is Us, the gravitational potential minus the centrifugal potential on the surface; it is not the polytropic EOS constant K.
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#include <fields.hpp>
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| struct | mass_normalization |
| | 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...
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This field holds the effective potential level on the stellar isobar. The level is solved together with the fixed total mass. The barotropic_constant name is retained as an internal coordinate identity. In the density formulation its value is Us, the gravitational potential minus the centrifugal potential on the surface; it is not the polytropic EOS constant K.
◆ Terms
Type list of terms for compile time reflection and iteration over the terms of the field.
◆ mass_normalization_term
| mass_normalization serif::discretization::blocks::barotropic_constant::mass_normalization_term {} |
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staticconstexpr |
Static constexpr instance of the mass_normalization term. This is used to access the term in the discretization.
◆ name
Compile time reflected name of the field.
The documentation for this struct was generated from the following file:
- src/include/serif/discretization/blocks/fields.hpp