Detection of Scalar Gravitational Waves
arXiv:gr-qc/0005089
Abstract
In this talk I review recent progresses in the detection of scalar gravitational waves. Furthermore, in the framework of the Jordan-Brans-Dicke theory, I compute the signal to noise ratio for a resonant mass detector of spherical shape and for binary sources and collapsing stars. Finally I compare these results with those obtained from laser interferometers and from Einsteinian gravity.
23 pages, talk delivered at the 2nd SIGRAV school on gravity, como italy, iopconf.sty needed