This test case checks the implementation of GYRE in MESA for a cooling 0.85 Msun white dwarf model.
This test case has 1 part.
- Part 1 (
inlist_pulse_wd) loads a pre-built 0.85 Msun white dwarf model and evolves the model until the effective temperature drops below log10(Teff/K) = 4. During the evolution the
run_star_extras.f90calls GYRE, processes the GYRE output, and searches for a non-radial g-mode frequency of 2.2e-3 Hz (period of 454 s). Close matches to this target frequency are reported in the terminal:
model order freq (Hz) P (sec) P (day) 1292 -8 0.2204E-02 0.0000 0.0000 matched target frequency 1292 -7 0.2374E-02 0.0000 0.0000 ... model order freq (Hz) P (sec) P (day) 1296 -8 0.2163E-02 0.0000 0.0000 matched target frequency 1296 -7 0.2348E-02 0.0000 0.0000
Last-Updated: 11Jun2021 (MESA 5be9e57) by fxt.