SpECTRE
v2024.05.11
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The magnetic field \(B^i = n_\mu {}^\star\!F^{i \mu}\) measured by an Eulerian observer, where \(n_\mu\) is the normal to the spatial hypersurface and \({}^\star\!F^{\mu \nu}\) is the dual of the Faraday tensor. Note that \(B^i\) is purely spatial, and it can be lowered using the spatial metric. More...
#include <Tags.hpp>
Public Types | |
using | type = tnsr::I< DataType, Dim, Fr > |
Static Public Member Functions | |
static std::string | name () |
The magnetic field \(B^i = n_\mu {}^\star\!F^{i \mu}\) measured by an Eulerian observer, where \(n_\mu\) is the normal to the spatial hypersurface and \({}^\star\!F^{\mu \nu}\) is the dual of the Faraday tensor. Note that \(B^i\) is purely spatial, and it can be lowered using the spatial metric.