Formation of supermassive black holes

O. Y. Gnedin
Institute of Astronomy, Cambridge, England

The existence of quasars at redshift z > 5 indicates that supermassive black holes were present since the very early times. If they grew by accretion, the seeds of mass >~105 MSun must have formed at z ~ 9. These seed black holes may result from the collapse and dissipation of primordial gas during the early stages of galaxy formation. I discuss the effects of the magnetic field on the collapse and fragmentation of cold clouds of gas embedded into a hot phase and a virialized dark matter halo. The field of 10-4 G ejected by supernova remnants can halt cloud break-up at 104 MSun. The magnetized clouds collapse into black holes, which later merge via dynamical friction into a single central object with Mbh ~ 6.106 MSun.


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