Key points are not available for this paper at this time.
It is pointed out that the Brans-Dicke theory predicts a transverse spin-0 component of the O (r^-1) radiative Riemann tensor. Unlike the conventional spin-2 radiative Riemann tensor, monopole oscillations may serve as a source. Under favorable conditions, neutron star formation within our galaxy will be detectable by Weber's gravitational-wave receiver.
Robinson et al. (Mon,) studied this question.