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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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1202.0839 (Preprint), 2MB
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1202.0839
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 Urheber:
Amaro-Seoane, Pau1, Autor           
Aoudia, Sofiane1, Autor           
Babak, Stanislav1, Autor           
Binetruy, Pierre, Autor
Berti, Emanuele, Autor
Bohé, Alejandro2, Autor           
Caprini, Chiara, Autor
Colpi, Monica, Autor
Cornish, Neil J., Autor
Danzmann, Karsten3, Autor           
Dufaux, Jean-Francois, Autor
Gair, Jonathan, Autor
Jennrich, Oliver, Autor
Jetzer, Philippe, Autor
Klein, Antoine, Autor
Lang, Ryan N., Autor
Lobo, Alberto, Autor
Littenberg, Tyson, Autor
McWilliams, Sean T., Autor
Nelemans, Gijs, Autor
Petiteau, Antoine1, Autor           Porter, Edward K., AutorSchutz, Bernard F.1, Autor           Sesana, Alberto1, Autor           Stebbins, Robin, AutorSumner, Tim, AutorVallisneri, Michele, AutorVitale, Stefano, AutorVolonteri, Marta, AutorWard, Henry, Autor mehr..
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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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO, Astrophysics, Galaxy Astrophysics, astro-ph.GA
 Zusammenfassung: 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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 Datum: 2012-02-032012
 Publikationsstatus: Erschienen
 Seiten: 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
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
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 Identifikatoren: arXiv: 1202.0839
DOI: 10.1088/0264-9381/29/12/124016
 Art des Abschluß: -

Veranstaltung

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Titel: 9th Edoardo Amaldi Meeting and the 2011 Numerical Relativity and Data Analysis Meeting (AMALDI 9/NRDA 2011)
Veranstaltungsort: Cardiff University
Start-/Enddatum: 2011-07-10 - 2011-07-15

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Titel: Classical and quantum gravity
Genre der Quelle: Zeitschrift
 Urheber:
Affiliations:
Ort, Verlag, Ausgabe: Bristol, U.K. : Institute of Physics
Seiten: - Band / Heft: 29 (12) Artikelnummer: 124016 Start- / Endseite: - Identifikator: ISSN: 0264-9381
CoNE: https://pure.mpg.de/cone/journals/resource/954925513480_1