A starburst induced by a galaxy merger may create a relatively thin central stellar disk at radius \leq 100 pc .
We calculate the rate of tidal disruption events ( TDEs ) by the inspiraling secondary supermassive black ( SMBH ) through the disk .
With a small enough stellar velocity dispersion ( \sigma / v _ { c } \leq 0.1 ) in the disk , it is shown that 10 ^ { 5 } -10 ^ { 6 } TDEs of solar-type main sequence stars per post-starburst galaxy ( PSB ) can be produced to explain their dominance in producing observed TDEs .
Although the time it takes to bring the secondary SMBH to the disk apparently varies in the range of \sim 0.1 - 1 Gyr since the starburst , depending on its landing location and subsequently due to dynamical friction with stars exterior to the central stellar disk in question , the vast majority of TDEs by the secondary SMBH in any individual PSB occurs within a space of time shorter than \sim 30 Myr .
Five unique testable predictions of this model are suggested .