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Aims: We explore the lensing properties of asymmetric matter densitydistributions in Bekenstein's Tensor-Vector-Scalar theory (TeVeS). Methods:Using an iterative Fourier-based solver for the resulting non-linear scalarfield equation, we numerically calculate the total gravitational potential andderive the corresponding TeVeS lensing maps. Results: Considering variations onrather small scales, we show that the lensing properties significantly dependon the lens's extent along the line of sight. Furthermore, all simulated TeVeSconvergence maps strongly track the dominant baryonic components, non-lineareffects, being capable of counteracting this trend, turn out to be very small.Setting up a toy model for the cluster merger 1E0657-558, we infer that TeVeScannot explain observations without assuming an additional dark mass componentin both cluster centers, which is in accordance with previous work.

Asymmetric Gravitational Lenses in TeVeS and Application to the Bullet Cluster