2000/12/06 by J. A. de Freitas Pacheco, Pacheco, J. A. de Freitas
Engineering · Physics and Astronomy · #Astronomical Observations and Instrumentation #Astrophysics (astro-ph) #FOS: Physical sciences #Geophysics and Sensor Technology #Pulsars and Gravitational Waves Research #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0012128
Paper presented at the 6$^{th}$ International Workshop on Relativistic Aspects of Nuclear Physics - Tabatinga - Brazil - October 2000
arxiv created 2000/12/06 · openalex publication_date 2000/12/06 · arxiv updated 2009/12/01 · openalex created_date 2024/04/11 · openalex updated_date 2026/07/28
The properties of potential gravitational wave sources like neutron stars,\nblack holes and binary systems are reviewed, as well as the different\ncontributions (stochastic and continuous) to the gravitational wave background.\nThe detectability of these sources by the present generation of laser beam\ninterferometers, which will be fully operational around 2002, is also\nconsidered.\n