CORDIS Project
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This project explores the formation and evolution of Black Holes in low metallicity environments, focusing on their growth and spin characteristics. It aims to enhance understanding of gravitational waves and the origins of binary black hole mergers.
Gravitational-wave (GW) Astronomy opened a new window to the Universe from its infant state to the present.
The key physical systems which allow probing the Universe through these vast time and length scales are Black Holes (BH).
Low metallicity clouds, composed primarily of atomic hydrogen, before and during the epoch of reionization, are a natural environment for BHs to be born and form Binary Black Holes (BBH) which can merge via GW emission.
Stellar BHs, being the remnants of the death of ve…
UNIVERSITA' DEGLI STUDI DI MILANO-BICOCCA
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