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  Low-frequency gravitational-wave science with eLISA/NGO

Amaro-Seoane, P., Aoudia, S., Babak, S., Binetruy, P., Berti, E., Bohé, A., et al. (2012). Low-frequency gravitational-wave science with eLISA/NGO. Classical and quantum gravity, 29(12): 124016.

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 Creators:
Amaro-Seoane, Pau1, Author           
Aoudia, Sofiane1, Author           
Babak, Stanislav1, Author           
Binetruy, Pierre, Author
Berti, Emanuele, Author
Bohé, Alejandro2, Author           
Caprini, Chiara, Author
Colpi, Monica, Author
Cornish, Neil J., Author
Danzmann, Karsten3, Author           
Dufaux, Jean-Francois, Author
Gair, Jonathan, Author
Jennrich, Oliver, Author
Jetzer, Philippe, Author
Klein, Antoine, Author
Lang, Ryan N., Author
Lobo, Alberto, Author
Littenberg, Tyson, Author
McWilliams, Sean T., Author
Nelemans, Gijs, Author
Petiteau, Antoine1, Author           Porter, Edward K., AuthorSchutz, Bernard F.1, Author           Sesana, Alberto1, Author           Stebbins, Robin, AuthorSumner, Tim, AuthorVallisneri, Michele, AuthorVitale, Stefano, AuthorVolonteri, Marta, AuthorWard, Henry, Author more..
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              
2Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_1933290              
3Laser Interferometry & Gravitational Wave Astronomy, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_24010              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO, Astrophysics, Galaxy Astrophysics, astro-ph.GA
 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.

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 Dates: 2012-02-032012
 Publication Status: Issued
 Pages: 20 pages, 8 figures, proceedings of the 9th Amaldi Conference on Gravitational Waves. For a longer exposition of the eLISA science case, see http://arxiv.org/abs/1201.3621
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: arXiv: 1202.0839
DOI: 10.1088/0264-9381/29/12/124016
 Degree: -

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Title: 9th Edoardo Amaldi Meeting and the 2011 Numerical Relativity and Data Analysis Meeting (AMALDI 9/NRDA 2011)
Place of Event: Cardiff University
Start-/End Date: 2011-07-10 - 2011-07-15

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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics
Pages: - Volume / Issue: 29 (12) Sequence Number: 124016 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: https://pure.mpg.de/cone/journals/resource/954925513480_1