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Status: Bibliographieeintrag
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Verfasst von:Alfradique, Viviane [VerfasserIn]   i
 Quartin, Miguel [VerfasserIn]   i
 Amendola, Luca [VerfasserIn]   i
 Castro, Tiago [VerfasserIn]   i
 Toubiana, Alexandre [VerfasserIn]   i
Titel:The lure of sirens
Titelzusatz:joint distance and velocity measurements with third generation detectors
Verf.angabe:Viviane Alfradique, Miguel Quartin, Luca Amendola, Tiago Castro, and Alexandre Toubiana
E-Jahr:2022
Jahr:27 May 2022
Umfang:14 S.
Fussnoten:Gesehen am 21.09.2022
Titel Quelle:Enthalten in: De.arxiv.org
Ort Quelle:[S.l.] : Arxiv.org, 1991
Jahr Quelle:2022
Band/Heft Quelle:(2022), Artikel-ID 2205.14034, Seite 1-14
Abstract:The next generation of detectors will detect gravitational waves from binary neutron stars at cosmological distances, for which around a thousand electromagnetic follow-ups may be observed per year. So far, most work devoted to the expected cosmological impact of these standard sirens employed them only as distance indicators. Only recently their use as tracers of clustering, similar to what already proposed for supernovae, has been studied. Focusing on the expected specifications of the Einstein Telescope (ET), we forecast here the performance on cosmological parameters of future standard sirens as both distance and density indicators, with emphasis on the linear perturbation growth index and on spatial curvature. We improve upon previous studies in a number of ways: a more detailed analysis of available telescope time, the inclusion of more cosmological and nuisance parameters, the Alcock-Paczynski correction, the use of sirens also as both velocity and density tracers, and a more accurate estimation of the distance posterior. We find that the analysis of the clustering of sirens improves the constraints on $H_0$ by 30% and on $\Omega_{k0}$ by over an order of magnitude, with respect to their use merely as distance indicators. With 5 years of joint ET and Rubin Observatory follow-ups we could reach precision of 0.1 km/s/Mpc in $H_0$ and 0.02 in $\Omega_{k0}$ using only data in the range $0<z<0.5$. We also find that the use of sirens as tracers of density, and not only velocity, yields good improvements on the growth of structure constraints.
DOI:doi:10.48550/arXiv.2205.14034
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext ; Verlag: https://doi.org/10.48550/arXiv.2205.14034
 Volltext: http://arxiv.org/abs/2205.14034
 DOI: https://doi.org/10.48550/arXiv.2205.14034
Datenträger:Online-Ressource
Sprache:eng
Sach-SW:Astrophysics - Cosmology and Nongalactic Astrophysics
 General Relativity and Quantum Cosmology
K10plus-PPN:1808028759
Verknüpfungen:→ Sammelwerk

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