Direct Collapse to Precursors of Supermassive Black Hole Seeds: Radiation-feedback-generated Outflows
Yang Luo,
Isaac Shlosman,
Kentaro Nagamine
Abstract:We use high-resolution zoom-in cosmological simulations to model outflow triggered by radiation and thermal drivers around the central mass accumulation during direct collapse within the dark matter (DM) halo. The maximal resolution is 1.3 × 10−5 pc, and no restrictions are put on the geometry of the inflow/outflow. The central mass is considered prior to the formation of the supermassive black hole seed at a redshift of z ∼ 15.9 and can constitute either a supermassive star (SMS) of ∼105
M
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