189 citations · 378 across the 7 of their papers we have counts for
7 papers
The Growth and Enrichment of the Intragroup Gas
Lichen Liang, Fabrice Durier, Arif Babul +5
The thermal and chemical properties of the hot diffuse intragroup medium (IGrM) provide important constraints on the feedback processes associated with massive galaxy formation and…
The Evolution of the Baryon Distribution in the Universe from Cosmological Simulations
Fabrice Durier, Jose Antonio de Freitas Pacheco
The evolution of the baryon distribution in different phases, derived from cosmological simulations, are here reported. These computations indicate that presently most of baryons a…
Coalescence Rate of Supermassive Black Hole Binaries Derived from Cosmological Simulations: Detection Rates for LISA and ET
Ch. Filloux, J. A. de Freitas Pacheco, F. Durier +1
The coalescence history of massive black holes has been derived from cosmological simulations, in which the evolution of those objects and that of the host galaxies are followed in…
Implementation of feedback in SPH: towards concordance of methods
Fabrice Durier, Claudio Dalla Vecchia
We perform simulations of feedback from supernovae and black holes with smoothed particle hydrodynamics (SPH). Such strong perturbations are inaccurately handled with standard time…
Accretion onto black holes formed by direct collapse
Jarrett L. Johnson, Sadegh Khochfar, Thomas H. Greif +1
One possible scenario for the formation of massive black holes (BHs) in the early Universe is from the direct collapse of primordial gas in atomic-cooling dark matter haloes in whi…
Evolution of Supermassive Black Holes from Cosmological Simulations
Ch. Filloux, F. Durier, J. A. de Freitas Pacheco +1
The correlations between the mass of supermassive black holes and properties of their host galaxies are investigated through cosmological simulations. Black holes grow from seeds o…
Evolution of the Phase-Space Density of Dark Matter Halos and Mixing Effects in Merger Events
Sébastien Peirani, Fabrice Durier, José Antonio De Freitas Pacheco
Cosmological N-body simulations were performed to study the evolution of the phase-space density Q = rho/sigma^3 of dark matter halos. No significant differences in the scale relat…