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Accession Number N20120012980
Title Low-Frequency Gravitational-Wave Science with eLISA/ NGO.
Publication Date Jul 2011
Media Count 20p
Personal Author A. Bohe A. Klein A. Lobo A. Petiteau B. F. Schutz C. Caprini E. Berti E. K. Porter G. Nelemans J. Gair J. F. Dufaux K. Danzmann M. Colpi M. Vallisneri N. J. Cornish O. Jennrich P. Amaro-Seoane P. Binetruy P. Jetzer R. Stebbins R. N. Lang S. Aoudia S. Babak S. T. McWilliams T. Littenberg
Abstract 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 ultracompact 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.
Keywords Cosmology
Detection
European space agency
Gravitational waves
Low frequencies
Mission planning
Relativity
Signal to noise ratios
Stellar mass
Universe

 
Source Agency National Aeronautics and Space Administration
NTIS Subject Category 54C - Astrophysics
Corporate Author Goddard Space Flight Center, Greenbelt, MD.
Document Type Journal article
Title Note N/A
NTIS Issue Number 1303
Contract Number N/A

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