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20052009
most citedThe stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays

531 citations · 1.6k across the 13 of their papers we have counts for

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astro-ph200832 cited

LISA detection of massive black hole binaries: imprint of seed populations and of exterme recoils

A. Sesana, M. Volonteri, F. Haardt

All the physical processes involved in the formation, merging, and accretion history of massive black holes along the hierarchical build--up of cosmic structures are likely to leav…

astro-ph200831 cited

Ejection of hypervelocity binary stars by a black hole of intermediate mass orbiting Sgr A*

A. Sesana, P. Madau, F. Haardt

The discovery of hypervelocity binary stars (HVBs) in the Galactic halo would provide definite evidence of the existence of a massive black hole companion to Sgr A*. Here we use an…

astro-ph2008281 cited

Gravitational waves from resolvable massive black hole binary systems and observations with Pulsar Timing Arrays

A. Sesana, A. Vecchio, M. Volonteri

Massive black holes are key components of the assembly and evolution of cosmic structures and a number of surveys are currently on-going or planned to probe the demographics of the…

astro-ph200855 cited

Observing white dwarfs orbiting massive black holes in the gravitational wave and electro-magnetic window

A. Sesana, A. Vecchio, M. Eracleous +1

We consider a potentially new class of gravitational wave sources consisting of a white dwarf coalescing into a massive black hole in the mass range ~10^4-10^5\msun. These sources…

astro-ph2008531 cited

The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays

Alberto Sesana, Alberto Vecchio, Carlo Nicola Colacino

Massive black hole binary systems, with masses in the range ~10^4-10^10 \msun, are among the primary sources of gravitational waves in the frequency window ~10^-9 Hz - 0.1 Hz. Puls…

astro-ph200793 cited

Interaction of massive black hole binaries with their stellar environment: III. Scattering of bound stars

Alberto Sesana, Francesco Haardt, Piero Madau

We develop a formalism for studying the dynamics of massive black hole binaries embedded in gravitationally-bound stellar cusps, and study the binary orbital decay by three-body in…