The extreme density fluctuations necessary to produce primordial black holes (PBHs) also lead to the formation of a much greater abundance of dark matter ultradense haloes that form during the radiation epoch. The aim of this thesis is to explore in detail the dynamics, properties and statistical abundance of these dark matter mini-haloes from its earliest formation, during the radiation epoch, up to the late-time Universe.
The extreme density fluctuations necessary to produce primordial black holes (PBHs) also lead to the formation of a much greater abundance of dark matter ultradense haloes that form during the radiation epoch. The aim of this thesis is to explore in detail the dynamics, properties and statistical abundance of these dark matter mini-haloes from its earliest formation, during the radiation epoch, up to the late-time Universe.
Abundance and Dynamical Properties of the Ultradense Dark Matter Halos
KULUBAYEVA, DIANA
2022/2023
Abstract
The extreme density fluctuations necessary to produce primordial black holes (PBHs) also lead to the formation of a much greater abundance of dark matter ultradense haloes that form during the radiation epoch. The aim of this thesis is to explore in detail the dynamics, properties and statistical abundance of these dark matter mini-haloes from its earliest formation, during the radiation epoch, up to the late-time Universe.| File | Dimensione | Formato | |
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https://hdl.handle.net/20.500.12608/51829