  We construct and study new giant graviton configurations in the framework of
the non-supersymmetric Schrodinger holography. We confirm in the original
Schrodinger spacetime, the picture discovered previously in the pp-wave limit
of the geometry, namely that it is the giant graviton that becomes the
energetically favored stable configuration compared to the point graviton one.
Furthermore, there is a critical value of the deformation above which the point
graviton disappears from the spectrum. The former fact leads also to the
possibility of tunnelling from the point graviton to the giant graviton
configuration. We calculate, explicitly, the instanton solution and its
corresponding action which gives a measure of the tunnelling probability.
Finally, we evaluate holographically the three-point correlation function of
two giant gravitons and one dilaton mode as a function of the Schrodinger
invariant.
