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  Prospects for observing extreme-mass-ratio inspirals with LISA

Gair, J. R., Babak, S., Sesana, A., Amaro-Seoane, P., Barausse, E., Berry, C. P. L., et al. (2017). Prospects for observing extreme-mass-ratio inspirals with LISA. Journal of Physics: Conference Series, 840(1): 012021.

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Datensatz-Permalink: http://hdl.handle.net/11858/00-001M-0000-002D-46D4-C Versions-Permalink: http://hdl.handle.net/11858/00-001M-0000-002E-0958-A
Genre: Konferenzbeitrag

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1704.00009.pdf (Preprint), 669KB
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JPCS_840_012021.pdf (Verlagsversion), 630KB
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Urheber

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 Urheber:
Gair, Jonathan R, Autor
Babak, Stanislav1, Autor              
Sesana, Alberto2, Autor              
Amaro-Seoane, Pau1, Autor              
Barausse, Enrico, Autor
Berry, Christopher P L, Autor
Berti, Emanuele, Autor
Sopuerta, Carlos, Autor
Affiliations:
1Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:1933290              
2Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, escidoc:24013              

Inhalt

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Schlagwörter: Astrophysics, Galaxy Astrophysics, astro-ph.GA,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO,General Relativity and Quantum Cosmology, gr-qc
 Zusammenfassung: One of the key astrophysical sources for the Laser Interferometer Space Antenna (LISA) are the inspirals of stellar-origin compact objects into massive black holes in the centres of galaxies. These extreme-mass-ratio inspirals (EMRIs) have great potential for astrophysics, cosmology and fundamental physics. In this paper we describe the likely numbers and properties of EMRI events that LISA will observe. We present the first results computed for the 2.5 Gm interferometer that was the new baseline mission submitted in January 2017 in response to the ESA L3 mission call. In addition, we attempt to quantify the astrophysical uncertainties in EMRI event rate estimates by considering a range of different models for the astrophysical population. We present both likely event rates and estimates for the precision with which the parameters of the observed sources could be measured. We finish by discussing the implications of these results for science using EMRIs.

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 Datum: 2017-03-312017
 Publikationsstatus: Im Druck publiziert
 Seiten: 12 pages, 3 figures, 5 tables. These proceedings are a summary of the results presented in arXiv:1703.09722
 Ort, Verlag, Ausgabe: -
 Inhaltsverzeichnis: -
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 Identifikatoren: arXiv: 1704.00009
URI: http://arxiv.org/abs/1704.00009
DOI: 10.1088/1742-6596/840/1/012021
 Art des Abschluß: -

Veranstaltung

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Titel: 11th International LISA Symposium
Veranstaltungsort: Zürich, Switzerland
Start-/Enddatum: 2016-09-05 - 2016-09-09

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Titel: Journal of Physics: Conference Series
Genre der Quelle: Zeitschrift
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Ort, Verlag, Ausgabe: Bristol : IOP Publishing
Seiten: - Band / Heft: 840 (1) Artikelnummer: 012021 Start- / Endseite: - Identifikator: ISSN: 1742-6588
CoNE: http://pubman.mpdl.mpg.de/cone/journals/resource/111097776606042