2 citations · 2 across the 3 of their papers we have counts for
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Net Cooling Tables for Cosmological Simulations under Multiple UV/X-ray Background Models
Laura Di Federico, Klaus Dolag, Ildar Khabibullin +3
We present three sets of net cooling tables for cosmological hydrodynamical simulations, computed with CLOUDY 23.01 for optically thin gas in photoionization equilibrium with three…
A novel sub-grid model for super-Eddington accretion of spinning black holes in galaxy-scale simulations
Wei-Bo Kao, Pedro R. Capelo, Elia Cenci +3
Super-Eddington accretion has been proposed to explain the existence of black holes (BHs) with masses exceeding a billion solar masses within the first billion years after the Big…
Supermassive black hole spin evolution in cosmological simulations with OpenGadget3
Luca Sala, Milena Valentini, Veronica Biffi +1
Mass and spin of massive black holes (BHs) at the centre of galaxies evolve due to gas accretion and mergers with other BHs. Besides affecting e.g. the evolution of relativistic je…