We summarize our recent results on the evolution of super-massive black holes in the cores of galaxies. Our models are based on the viscous, Eddington-limited evolution of self-gravitating accretion disks. We find that, within this framework, one can explain the growth time scales and the luminosities of individual objects as well as the variation of these quantities for AGN with different black hole masses
The aim of this thesis is to investigate the key points concerning the evolution of the local Super-...
There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMB...
We introduce a new model for the formation and evolution of supermassive black holes (SMBHs) in the ...
We summarize our recent results on the evolution of super-massive black holes in the cores of galaxi...
We investigate the growth of black holes and their effects on the evolution of galaxies through cosm...
I use cosmological hydrodynamic simulations to investigate different aspects of the evolution of gal...
We analyse the demographics of black holes (BHs) in the large-volume cosmological hydrodynamical sim...
Supermassive black holes are nowadays believed to reside in most local galaxies. Observations have r...
First observed as early as redshift z = 7 and now thought to be found at the centre of every massive...
Beyond all reasonable doubt, black holes are commonly found in the nuclei of most normal galaxies. I...
This thesis examines many of the ways in which massive galaxies and their super- massive black holes...
We investigate the cosmic evolution of the black hole (BH) mass–bulge luminosity relation using a sa...
Recent models of black hole growth in a cosmological context have forwarded a paradigm in which the ...
We append two additional black hole (BH) accretion models, namely viscous disc and gravitational tor...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
The aim of this thesis is to investigate the key points concerning the evolution of the local Super-...
There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMB...
We introduce a new model for the formation and evolution of supermassive black holes (SMBHs) in the ...
We summarize our recent results on the evolution of super-massive black holes in the cores of galaxi...
We investigate the growth of black holes and their effects on the evolution of galaxies through cosm...
I use cosmological hydrodynamic simulations to investigate different aspects of the evolution of gal...
We analyse the demographics of black holes (BHs) in the large-volume cosmological hydrodynamical sim...
Supermassive black holes are nowadays believed to reside in most local galaxies. Observations have r...
First observed as early as redshift z = 7 and now thought to be found at the centre of every massive...
Beyond all reasonable doubt, black holes are commonly found in the nuclei of most normal galaxies. I...
This thesis examines many of the ways in which massive galaxies and their super- massive black holes...
We investigate the cosmic evolution of the black hole (BH) mass–bulge luminosity relation using a sa...
Recent models of black hole growth in a cosmological context have forwarded a paradigm in which the ...
We append two additional black hole (BH) accretion models, namely viscous disc and gravitational tor...
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ...
The aim of this thesis is to investigate the key points concerning the evolution of the local Super-...
There is compelling evidence that most -if not all- galaxies harbour a super-massive black hole (SMB...
We introduce a new model for the formation and evolution of supermassive black holes (SMBHs) in the ...
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