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MeanField_SERiF/docs/man/man3/models.hpp.3

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.TH "src/include/serif/geometry/deformation/models.hpp" 3 "Version v0.0.1a" "SERiF" \" -*- nroff -*-
.ad l
.nh
.SH NAME
src/include/serif/geometry/deformation/models.hpp
.SH SYNOPSIS
.br
.PP
\fR#include <array>\fP
.br
\fR#include <optional>\fP
.br
.SS "Classes"
.in +1c
.ti -1c
.RI "struct \fBserif::geometry::deformation::NodalRadialSurface\fP"
.br
.RI "Give each surface node an independent radial displacement, measured in physical length\&. "
.ti -1c
.RI "struct \fBserif::geometry::deformation::SphericalHarmonicSurface\fP"
.br
.RI "Represent radial displacement lengths with normalized real spherical harmonics on the reference surface\&. "
.ti -1c
.RI "struct \fBserif::geometry::deformation::PowerLawRadialExtension\fP"
.br
.RI "Extend surface motion toward a fixed stellar center using a power of logical reference radius\&. "
.ti -1c
.RI "struct \fBserif::geometry::deformation::FixedInfinityRadialExtension\fP"
.br
.RI "Reduce surface motion linearly to zero at reference infinity in logical reference radius\&. "
.ti -1c
.RI "struct \fBserif::geometry::deformation::DomainDeformation< SurfaceT, InteriorT, VacuumT >\fP"
.br
.RI "State how the stellar surface moves and how that motion extends into the two surrounding regions\&. "
.in -1c
.SS "Namespaces"
.in +1c
.ti -1c
.RI "namespace \fBserif\fP"
.br
.ti -1c
.RI "namespace \fBserif::geometry\fP"
.br
.ti -1c
.RI "namespace \fBserif::geometry::deformation\fP"
.br
.in -1c
.SH "Author"
.PP
Generated automatically by Doxygen for SERiF from the source code\&.