The aim of this thesis is to find a way to discern the effects due to the effective sources (i.e. modifications of dynamics related to the matter we put in the model) from those due to the conformal factor (i.e. those due to the choice of the metric) in the case of a specific f(R)-cosmology, then we will compare the Hubble drift of the extended cosmology with the Hubble drift predicted by the LambdaCDM model (which is frequently referred to as the standard model of cosmology).
Hubble drift in cosmologie estese
DEL VECCHIO, LEONARDO
2017/2018
Abstract
The aim of this thesis is to find a way to discern the effects due to the effective sources (i.e. modifications of dynamics related to the matter we put in the model) from those due to the conformal factor (i.e. those due to the choice of the metric) in the case of a specific f(R)-cosmology, then we will compare the Hubble drift of the extended cosmology with the Hubble drift predicted by the LambdaCDM model (which is frequently referred to as the standard model of cosmology).File in questo prodotto:
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Utilizza questo identificativo per citare o creare un link a questo documento:
https://hdl.handle.net/20.500.14240/50567