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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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The density field used to represent the distribution of mass in the system. This is a scalar field that is associated with the mass density of the system. The density field is used to enforce the mass conservation condition in the weak form. More...
#include <fields.hpp>
Classes | |
| struct | mass |
| The mass density term for the system. Note that the naming here could be a bit confusing as FEM also uses the term "mass" to represent the canonical mass matrix. This is a more standard physics reading of what is going on here. We define that this space is a third order scalar H1 space. This gives density a continuous surface trace and a weak spatial gradient. More... | |
Public Types | |
| using | Terms = utils::types::TypeList<mass> |
| Type list of terms for compile time reflection and iteration over the terms of the field. | |
Static Public Attributes | |
| static constexpr std::string_view | name = meta::type_name<density>() |
| Compile time reflected name of the field. | |
| static constexpr mass | mass_density_term {} |
| Static constexpr instance of the mass term. This is used to access the term in the discretization. | |
The density field used to represent the distribution of mass in the system. This is a scalar field that is associated with the mass density of the system. The density field is used to enforce the mass conservation condition in the weak form.
Type list of terms for compile time reflection and iteration over the terms of the field.
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staticconstexpr |
Static constexpr instance of the mass term. This is used to access the term in the discretization.
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staticconstexpr |
Compile time reflected name of the field.