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  Constraining properties of the black hole population using LISA

Gair, J. R., Sesana, A., Berti, E., & Volonteri, M. (2011). Constraining properties of the black hole population using LISA. Classical and quantum gravity, 28: 094018.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-0831-D Version Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-0832-B
Genre: Conference Paper

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 Creators:
Gair, Jonathan R, Author
Sesana, Alberto1, Author              
Berti, Emanuele, Author
Volonteri, Marta, Author
Affiliations:
1Astrophysical Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society, ou_24013              

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Free keywords: General Relativity and Quantum Cosmology, gr-qc,Astrophysics, Cosmology and Extragalactic Astrophysics, astro-ph.CO
 Abstract: LISA should detect gravitational waves from tens to hundreds of systems containing black holes with mass in the range from 10 thousand to 10 million solar masses. Black holes in this mass range are not well constrained by current electromagnetic observations, so LISA could significantly enhance our understanding of the astrophysics of such systems. In this paper, we describe a framework for combining LISA observations to make statements about massive black hole populations. We summarise the constraints that LISA observations of extreme-mass-ratio inspirals might be able to place on the mass function of black holes in the LISA range. We also describe how LISA observations can be used to choose between different models for the hierarchical growth of structure in the early Universe. We consider four models that differ in their prescription for the initial mass distribution of black hole seeds, and in the efficiency of accretion onto the black holes. We show that with as little as 3 months of LISA data we can clearly distinguish between these models, even under relatively pessimistic assumptions about the performance of the detector and our knowledge of the gravitational waveforms.

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 Dates: 2010-09-302010-11-292011
 Publication Status: Published in print
 Pages: 12 pages, 3 figures, submitted to Class. Quantum Grav. for proceedings of 8th LISA Symposium; v2 minor changes for consistency with accepted version
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 Table of Contents: -
 Rev. Method: -
 Identifiers: arXiv: 1009.6172
DOI: 10.1088/0264-9381/28/9/094018
URI: http://arxiv.org/abs/1009.6172
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Title: 8th International LISA Symposium
Place of Event: Stanford University, California, USA
Start-/End Date: 2010-06-28 - 2010-07-02

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Title: Classical and quantum gravity
Source Genre: Journal
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Publ. Info: Bristol, U.K. : Institute of Physics, 9
Pages: - Volume / Issue: 28 Sequence Number: 094018 Start / End Page: - Identifier: ISSN: 0264-9381
CoNE: /journals/resource/954925513480_1