CORDIS Project
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This project aims to understand the formation of supermassive black holes in the early universe by analyzing their mass distribution and growth mechanisms. Using advanced simulations, it investigates the dynamics of gas in massive primordial halos to derive scaling relations that explain the properties of these black h…
Supermassive black holes (BHs) of more than a billion solar masses have been observed at z > 6 when the Universe was less than a billion years old.
Forming such objects is highly challenging, as high accretion rates need to be maintained over very long time scales.
Seed BHs with masses of 10^4 -10^6 solar masses, as predicted by the “direct collapse” scenario, provide a promising pathway to explain their presence.
During this project, I will derive the mass distribution of the BHs to provide con…
CENTRE NATIONAL DE LA RECHERCHE SCIENTIFIQUE CNRS
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