Gravitational waveforms from the quasicircular inspiral of compact
  binaries in massive Brans-Dicke theory
  We study the gravitational waves emitted by an inspiralling compact binary
system in massive Brans-Dicke theory. In addition to the two tensor
polarizations, which have been obtained in the previous work, we calculate
explicitly and analytically the expressions for the time-domain waveforms of
the two scalar polarizations. With the stationary phase approximations, we
obtain the Fourier transforms of the two tensor polarizations. We find that
when the scalar field is light, the waveforms can be mapped to the parametrized
post-Einsteinian (ppE) framework and we identify the ppE parameters. However,
when the scalar field is heavy, the ppE framework is not applicable. We also
obtain the projected constraints on the parameters of this theory by
gravitational wave observations of future ground-based detectors. Finally, we
apply our result to the model proposed by Damour and Esposito-Far\`{e}se,
$f(R)$ gravity, and screened modified gravity.
