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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-41692

Bleuler, A; Jetzer, P; Volonteri, M; Begelman, M C (2010). Strong lensing of gravitational waves as seen by LISA. Physical Review Letters, 105(25):251101-4pp.

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Abstract

We discuss strong gravitational lensing of gravitational waves from merging of massive black hole binaries in the context of the LISA mission. Detection of multiple events would provide invaluable information on competing theories of gravity, evolution and formation of structures and, with complementary observations, constraints on H_0 and other cosmological parameters. Most of the optical depth for lensing is provided by intervening massive galactic halos, for which wave optics effects are negligible. Probabilities to observe multiple events are sizable for a broad range of formation histories. For the most optimistic models, up to 4 multiple events with a signal to noise ratio >= 8 are expected in a 5-year mission. Chances are significant even for conservative models with either light (<= 60%) or heavy (<= 40%) seeds. Due to lensing amplification, some intrinsically too faint signals are brought over threshold (<= 2 per year)

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
DDC:530 Physics
Language:English
Date:November 2010
Deposited On:01 Mar 2011 14:33
Last Modified:08 Dec 2013 12:46
Publisher:American Physical Society
ISSN:0031-9007
Publisher DOI:10.1103/PhysRevLett.105.251101
Related URLs:http://arxiv.org/abs/1011.5238
Citations:Web of Science®. Times Cited: 5
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Scopus®. Citation Count: 3

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