Evolutionary Models¶
Supported Formats¶
Evolutionary models are read from a file created by a separate stellar
evolution code. The format of this file is specified by the
file_format
parameter of the &model
namelist group
(see the Stellar Model Parameters section). Possible choices are summarized
in the table below.
|
Description |
---|---|
|
Binary file describing an evolutionary model in AMDL format, as reverse engineered from the ADIPLS stellar oscillation code (Christensen-Dalsgaard, 2008) |
|
HDF5 file describing an evolutionary model in B3 format. This format is for testing purposes only, and will eventually be superseded and/or removed |
|
Text file describing an evolutionary model in FAMDL format, as
specified in the |
|
Text file describing an evolutionary model in FGONG format, as
specified in the updated |
|
HDF5 file describing an evolutionary model in GYRE Stellar Model (GSM) format, as specified in the GSM File Format section |
|
Text file describing an evolutionary model in MESA format, as specified in the MESA File Format section |
|
Text file describing an evolutionary model in the revised LOSC format |
|
Text file describing an evolutionary model in OSC format, as
specified in the |
|
Text file describing an evolutionary model in WDEC format, as specified in Bischoff-Kim & Montgomery (2018) |
Interpolation¶
Cubic spline interpolation is used to evaluate data between model grid
points. The deriv_type
parameter in the &model
namelist group controls how the spline derivatives are set up.
Double Points¶
If a model contains a pair of adjacent points with the same radial coordinate \(r\), this pair is treated as a double point representing a discontinuity in the density and some other thermodynamic quantities (but not the pressure or temperature). GYRE does not attempt to interpolate across double points, but does handle them properly when solving the oscillation equations through the use of jump conditions.