Gravitational waves - A new astronomy

Details Gravitational waves - A new astronomy Gravitational waves - A new astronomy

Mar 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976mmsai..47...11p&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 47, Mar. 1976, p. 11-22. In Italian.

Astronomy and Astrophysics

Astronomy

Astronomy, Cosmic Rays, Gravitational Waves, Antenna Design, Binary Stars, Black Holes (Astronomy), Neutron Stars, Relativity, Supernovae

Scientific paper

Possible sources of gravitational waves, techniques for perceiving gravitational waves (GW), and noise sources interfering with precise GW measurements are discussed. Supernovae giving rise to pulsars and/or asymmetric mass distributions rotating vigorously, markedly asymmetric binary systems, binary systems comprising a neutron star and a black hole, or massive black holes are contemplated as plausible sources of detectible gravitational radiation. The Weber gravitational antenna, experiments conducted to date along these lines, and proposals for a second generation of GW antennas or GW sensors are described.

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