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SUMMARY:Modelling the evolution of  mass and spin  of supermassive black h
 oles  with hydrodynamical simulations - Yohan Dubois (IAP)
DTSTART:20150515T103000Z
DTEND:20150515T113000Z
UID:TALK58946@talks.cam.ac.uk
CONTACT:Martin Haehnelt
DESCRIPTION:Supermassive black holes at high redshift (z>6) with masses as
  large as those in  our local Universe are now abundantly observed in larg
 e-scale surveys. This questions our understanding of black hole growth in 
 the first Gyrs of cosmological evolution\, and how 10^9 Msun of gas can be
  trapped at the heart of primordial galaxies. I will show how cosmological
  hydrodynamical simulations can help to design a scenario for feeding thos
 e massive beasts\, and what problems arise when one wants to take into acc
 ount the spin of BHs in the global picture.\n
LOCATION:Kavli LMR\, IoA
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