Astronomy and Astrophysics – Astrophysics
Scientific paper
2004-01-26
Astrophys.J. 611 (2004) 623-632
Astronomy and Astrophysics
Astrophysics
11 pages, 8 figues. Revised version accepted to be published in ApJ Discussion on number counts corrected and expanded
Scientific paper
10.1086/422185
We compute the expected gravitational wave signal from coalescing massive black hole (MBH) binaries at the center of galaxies in a hierarchical structure formation scenario in which seed holes of intermediate mass form far up in the dark halo merger tree. The merger history of DM halos and MBHs is followed from z=20 to the present in a LCDM cosmology. MBHs get incorporated through halo mergers into larger and larger structures, sink to the center owing to dynamical friction against the DM background, accrete cold material in the merger remnant, and form MBH binary systems. Stellar dynamical interactions cause the hardening of the binary at large separations, while gravitational wave emission takes over at small radii and leads to the final coalescence of the pair. The integrated emission from inspiraling MBH binaries results in a gravitational wave background (GWB). The characteristic strain spectrum has the standard h_c(f)\propto f^{-2/3} behavior only in the range 1E-9
Haardt Francesco
Madau Piero
Sesana Alberto
Volonteri Marta
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