Inverse-Chirp Imprint of Gravitational Wave Signals in Scalar Tensor
  Theory
  The scalar tensor theory contains a coupling function connecting the
quantities in the Jordan and Einstein frames, which is constrained to guarantee
a transformation rule between frames. We simulate the supernovae core collapse
with different choices of coupling functions defined over the viable region of
the parameter space and find that a generic inverse-chirp feature of the
gravitational waves in the scalar tensor scenario.
