Seminar

Formation of supermassive black hole seeds in first galaxies

Recent observations reveal the existence of supermassive black holes (SMBH) with > 10^9 Msun in the early universe with redshift z>7. The existence of high-z SMBHs puts strong constraints on the origins and formation pathways of SMBHs because the time required to form such massive objects from stellar-mass seed BHs becomes longer than the Hubble time at z>7. As a solution for this problem, formation of massive seed BHs via the collapse of supermassive stars (SMSs; >10^5 Msun) has been invoked. I will present our result of hydrodynamical simulation of gravitational collapse of a massive primordial cloud with >10^5Msun in the first galaxy, and discuss the fate of formed SMSs.

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