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SERiF v0.0.1a
Stellar Evolution and Rotation in Four Dimensions
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Integrate grad(v) dot grad(Phi) throughout the star and vacuum. More...
#include <primal_gravity.hpp>
Public Types | |
| using | Operands = utils::types::TypeList<PotentialGradient> |
Public Types inherited from serif::equations::Contribution< PotentialGradient > | |
| using | Test |
| The test type of the contribution. | |
| using | TestOperand |
| The operand type of the contribution (associating a test function and a term) | |
| using | Support |
| The domain support of the contribution (which then boils down to the dofs which are supported by the term on that test function) | |
Static Public Member Functions | |
| static PointLinearization< Operands, discretization::forms::VectorValue > | evaluate (const EquationPoint< Operands > &point) |
| The potential flux and its derivative are grad(Phi) and identity. | |
| static int | additional_order (PotentialGradient, int) |
| A linear flux introduces no additional coefficient degree. | |
Integrate grad(v) dot grad(Phi) throughout the star and vacuum.
| using serif::equations::PrimalPoissonBalance::PotentialFlux::Operands = utils::types::TypeList<PotentialGradient> |
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inlinestaticnodiscard |
A linear flux introduces no additional coefficient degree.
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inlinestaticnodiscard |
The potential flux and its derivative are grad(Phi) and identity.