  Due to the recent growth of discoveries of strong gravitational lensing (SGL)
systems, one can statistically study both lens properties and cosmological
parameters from 161 galactic scale SGL systems. We analyze meVSL model with the
velocity dispersion of lenses by adopting the redshift and surface mass density
depending power-law mass model. Analysis shows that meVSL models with various
dark energy models including $\Lambda$CDM, $\omega$CDM, and CPL provide the
negative values of meVSL parameter, $b$ when we put the prior to the $\Omega_{m
0}$ value from Planck. These indicate the faster speed of light and the
stronger gravitational force in the past. However, if we adopt the WMAP prior
on $\Omega_{m0}$, then we obtain the null results on $b$ within 1-$\sigma$ CL
for the different dark energy models.
