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\section{Stellar evolution calculations}  We use the Modules for Experiments in Stellar Evolution (MESA) to evolve low-mass stars from the pre main sequence to the cooling WD sequence \citep{http://adsabs.harvard.edu/abs/2011ApJS..192....3P}. \citep{http://adsabs.harvard.edu/abs/2011ApJS..192....3P}.This code includes the physics of rotation and dynamo-generated magnetic fields in radiation zones \citep{Paxtonr:2013}     Rotation is implemented The details of the implementation of angular momentum transport