Abstract
In order to examine the rotational effect around neutron star in tensor-vector-scalar (TeVeS) theory, we consider the slowly rotating relativistic stars with a uniform angular velocity. As a result, we find that similar to the case in general relativity (GR), the angular momentum is proportional to the angular velocity and one could possibly distinguish the gravitational theory in the strong field regime even in the case that the value of the coupling constant K is quite small.
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