Gravitational Radiation from Post-Newtonian Sources and Inspiralling Compact Binaries
To be observed and analyzed by the network of gravitational wave detectors on ground (LIGO, VIRGO, etc.) and by the future detectors in space (eLISA, etc.), inspiralling compact binaries -- binary star systems composed of neutron stars and/or black holes in their late stage of evolution -- require h...
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| Formato: | Artigo |
| Idioma: | English |
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SpringerOpen
2014-02-01
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| coleção: | Living Reviews in Relativity |
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| Acesso em linha: | http://www.livingreviews.org/lrr-2014-2 |