  We present results obtained using the magnetic Dartmouth stellar evolution
code that address the possibility that magnetic fields are inflating low-mass
stars in detached eclipsing binaries. While it seems plausible that magnetic
fields are inflating stars with radiative cores, the level of inflation
observed among fully convective stars appears too large to be explained by
magnetic fields. We provide an alternative explanation, stellar metallicity,
and propose observations that can help further constrain stellar models.
