A 0.55875 solar Mass VLTP model

A very late thermal pulse model made by MESA r22.11.1, We take the example of a $2.3M_{\odot}$ progenitor star with a metallicity of $Z=0.02$ and a helium abundance of $Y=0.28$. 
The progenitor star evolves from the pre-main sequence phase, passes through the main sequence and red giant branch (RGB) phases, and undergoes a total of 9 thermal pulses in the thermally pulsing asymptotic giant branch (TP-AGB) phase.\

Evolution after application of the ``relax\_mass'' function marks the beginning of the Very Late Thermal Pulse process we are attempting to model.
For the VLTP model, $\texttt{Total\_mass} = M = 0.55875\Msun$ (the mass after mass loss), $\texttt{H\_mass} = 0.000145 \Msun$ (mass of H envelope), and $\texttt{core\_mass} \equiv \texttt{CO\_mass} + \texttt{He\_mass} = M_{\rm c} = 0.55864\Msun$ (the mass of star without hydrogen envelope).

It from a draft prepared to publish, will add the link after published.