In this thesis I evaluate the merger rate density of binary black holes from Population III stars. This work takes into consideration different models for the stellar system's initial conditions and for the star formation rate density. The aim is to identify the influence that a specific model choice has on the resulting merger rate density.
Binary black holes from population III stars.
MERLI, LORENZO
2021/2022
Abstract
In this thesis I evaluate the merger rate density of binary black holes from Population III stars. This work takes into consideration different models for the stellar system's initial conditions and for the star formation rate density. The aim is to identify the influence that a specific model choice has on the resulting merger rate density.File in questo prodotto:
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Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.12608/30022