2000/05/19 by Francesco Fucito, F. Fucito, Fucito, F.
Earth and Planetary Sciences · Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astronomical interferometer #Astrophysics #Binary number #Classical mechanics #Detector #FOS: Physical sciences #General Relativity and Quantum Cosmology (gr-qc) #Geometry #Geophysics and Gravity Measurements #Gravitation #Gravitational wave #Gravitational-wave observatory #High Energy Physics - Theory (hep-th) #Interferometry #LIGO #Optics #Physics #Pulsars and Gravitational Waves Research #Scalar (mathematics) #Theoretical physics #gr-qc #hep-th
paper · pdf · doi:10.48550/arxiv.gr-qc/0005089
published in arXiv (Cornell University) (Cornell University) · 23 pages, talk delivered at the 2nd SIGRAV school on gravity, como italy, iopconf.sty needed
arxiv created 2000/05/19 · openalex publication_date 2000/05/19 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
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.