Polytropic models represent stars in hydrostatic equilibrium that follow the polytropic equation of state,
for piecewise-constant \(K\) and \(\npoly\). The structure of polytropic models is obtained by solving the Lane-Emden equation; GYRE doesn’t do this itself, but can read structure data from external files created by the build_poly executable (see the Building Polytropic Structure Files appendix for more details).
To use a polytropic model with GYRE, set the
parameter in the :n ml_g:model namelist group to
file parameter to the name of the polytropic