A w - M phantom transition at zt<0.1 as a resolution of the Hubble tension
This is the repository that contains the Mathematica code as well as useful comments that reproduce the figures of arxiv:2012.13932.
A rapid phantom transition of the dark energy equation of state parameter
Citing the paper
If you use any of the above codes or the figures in a published work please cite the following paper:
A w - M phantom transition at zt<0.1 as an approach to the Hubble tension
George Alestas, Lavrentios Kazantzidis and Leandros Perivolaropoulos, arxiv:2012.13932
Any further questions/comments are welcome.