Journal Club//2014 1st quarterJournal Club 24 Mars 2014(This text is not available in English, we apologize.)
Black hole formation in the high-redshift Universe
Par Dr. D. Schleicher
Salle L269 (ex D18), 2e étage, à l'ENS, 24 rue Lhomond, 13:30 à 14:30
Abstract :
While supermassive black holes with more than one billion solar masses have been observed at z>6, it remains a challenge to explain their origin in structure formation models.
Here, I present (magneto-)hydrodynamical adaptive mesh refinement simulations following the formation of the first massive black holes from cosmological scales down to less than 1 astronomical unit. I will quantify the expected mass scale of the first massive black holes and discuss the role of chemistry, turbulence and magnetic fields during their formation process. I will conclude with an outlook on future simulations and implications for the far-infrared - radio correlation in galaxies.
Last update 03-21-2014 03:27 pm / Jean-François RabasseJournal Club archives
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