Editing Appendix/Ramblings/PatrickMotl (section)

==December 22, 2020 (from Patrick)== 

<table border="1" cellpadding="10" width="60%" align="center"><tr><td align="left">
I added several simulations to [http://www.patrickmotl.net  my web page]; these are version 12 of the n = 5 pressure truncated polytropes.

I had the code compute the mass profile of the star during the run and plotted Joel’s function x versus enclosed mass as a proxy for the 
perturbation to the star. I also added plots of the frequency spectrum of the central density perturbation. I plotted the frequency spectrum 
where time is measured in units of the free fall time.

It appears to me that the eigenfrequencies are all evenly spaced which is not what I expected.
</td></tr></table>