SpECTRE
v2025.03.17
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The Irrotational Bns equations From Baumgarte and Shapiro Chapter 15 formulated as a set of coupled first-order PDEs. More...
#include <FirstOrderSystem.hpp>
Public Types | |
using | primal_fields = implementation defined |
using | primal_fluxes = implementation defined |
using | background_fields = implementation defined |
using | inv_metric_tag = gr::Tags::InverseSpatialMetric< DataVector, 3 > |
using | fluxes_computer = Fluxes |
using | sources_computer = Sources |
using | boundary_conditions_base = elliptic::BoundaryConditions::BoundaryCondition< 3 > |
using | modify_boundary_data = void |
Static Public Attributes | |
static constexpr size_t | volume_dim = 3 |
The Irrotational Bns equations From Baumgarte and Shapiro Chapter 15 formulated as a set of coupled first-order PDEs.
This system formulates the Irrotational Bns Hydrostatic Equilibrium equations for the velocity potential
The system can be formulated in terms of these fluxes and sources (see elliptic::protocols::FirstOrderSystem
):