  We calculate the strong lensing probability as a function of the
image-separation $\Delta\theta$ in TeVeS (tensor-vector-scalar) cosmology,
which is a relativistic version of MOND (MOdified Newtonian Dynamics). The
lens, often an elliptical galaxy, is modeled by the Hernquist profile. We
assume a flat cosmology with $\Omega_b=1-\Omega_\Lambda=0.04$ and the simplest
interpolating function $\mu(x)={\rm min}(1,x)$. For comparison, we recalculated
the probabilities for lenses by Singular Isothermal Sphere (SIS) galaxy halos
in LCDM with Schechter-fit velocity function. The amplification bias is
calculated based on the magnification of the second bright image rather than
the total of the two brighter images. Our calculations show that the Hernquist
model predicts insufficient but acceptable probabilities in flat TeVeS
cosmology compared with the results of the well defined combined sample of
Cosmic Lens All-Sky Survey (CLASS) and Jodrell Bank/Very Large Array
Astrometric Survey (JVAS); at the same time, it predicts higher probabilities
than SIS model in LCDM at small image separations.
