|
SpECTRE
v2026.04.01
|
The flux of \(U\) is \(\frac{1}{2} U^2\). More...
#include <Fluxes.hpp>
Public Types | |
| using | argument_tags = tmpl::list<Tags::U> |
| using | return_tags |
Static Public Member Functions | |
| static void | apply (gsl::not_null< tnsr::I< DataVector, 1 > * > flux, const Scalar< DataVector > &u) |
The flux of \(U\) is \(\frac{1}{2} U^2\).
| using Burgers::Fluxes::return_tags |