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Classical and Quantum Gravity 29 (2012) 4016
Low-frequency gravitational-wave science with eLISA/NGO
Pau Amaro-Seoane, Sofiane Aoudia, Stanislav Babak, P. Binétruy1, Emanuele Berti, A. Bohé2, C. Caprini3, Monica Colpi, Neil J. Cornish, Karsten Danzmann, J.-F. Dufaux1, Jonathan Gair, Oliver Jennrich, Philippe Jetzer, Antoine Klein, Ryan N. Lang, Alberto Lobo, Tyson Littenberg, Sean T. Mcwilliams, Gijs Nelemans, A. Petiteau1, 4, E.K. Porter1, Bernard F. Schutz, Alberto Sesana, Robin Stebbins, Tim Sumner, Michele Vallisneri, Stefano Vitale, Marta Volonteri, Henry Ward
eLISA/NGO Collaboration(s)

We review the expected science performance of the New Gravitational-Wave Observatory (NGO, a.k.a. eLISA), a mission under study by the European Space Agency for launch in the early 2020s. eLISA will survey the low-frequency gravitational-wave sky (from 0.1 mHz to 1 Hz), detecting and characterizing a broad variety of systems and events throughout the Universe, including the coalescences of massive black holes brought together by galaxy mergers; the inspirals of stellar-mass black holes and compact stars into central galactic black holes; several millions of ultra-compact binaries, both detached and mass transferring, in the Galaxy; and possibly unforeseen sources such as the relic gravitational-wave radiation from the early Universe. eLISA's high signal-to-noise measurements will provide new insight into the structure and history of the Universe, and they will test general relativity in its strong-field dynamical regime.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
2 :  IAP - Institut d'Astrophysique de Paris
3 :  IPHT - Institut de Physique Théorique (ex SPhT)
4 :  Max-Planck-Institut für Gravitationsphysik ( Albert-Einstein-Institut )
Physique/Relativité Générale et Cosmologie Quantique

Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique
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