Reproduction Package for the Paper "Dark Matter-Induced Stellar Oscillations"

Authors

Jeremy Sakstein (sakstein@hawaii.edu)
Ippocratis Saltas (saltas@fzu.cz)

Software

MESA version 15140 (http://mesa.sourceforge.net)
MESASDK version 20200325 (http://www.astro.wisc.edu/~townsend/static.php?ref=mesasdk)
GFORTRAN GCC version 9.2.0
GYRE version 7.0
Python 3.7.3
Jupyter Notebook version 6.4.12

MESA Files

MESA_inlist: MESA inlist used to produce the equilibrium solar model. Should be placed in $MESA_DIR/star/test_suit/simplex_solar_calibration.

late_pre_zams_1.0M.mod: Pre-main-sequence model loaded by MESA_inlist. Should be placed in $MESA_DIR/star/test_suit/simplex_solar_calibration.

solar_ref_mesa.mesa: Pulse data for the equilibrium solar model.

GYRE Files

GYRE_inlist.in: GYRE inlist used to produce the eigenfrequencies of the equilibrium solar model.

summary_mesa.txt: GYRE summary file.

detail.l1.n+N.h5: Tabulated eigenfunctions for the mode with n=1 n=N.

Python Files

V_rms_computation.ipynb: Jupyter notebook that computes the RMS velocity.

GS98_OPAL_CALIBR.txt: Equilibrium solar model. See V_rms_computation.ipynb.

Citation Policy

If you use any part of this reproduction package for independent work we recommend you cite this paper.