SpECTRE
v2025.01.30
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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 = tmpl::list<::Tags::Flux< Tags::U, tmpl::size_t< 1 >, Frame::Inertial > > |
Static Public Member Functions | |
static void | apply (gsl::not_null< tnsr::I< DataVector, 1 > * > flux, const Scalar< DataVector > &u) |
The flux of \(U\) is \(\frac{1}{2} U^2\).