Cosmic voids are large underdense regions of the Universe that, together with galaxy clusters, filaments and walls, characterise the large-scale structure of the Universe, the so-called cosmic web. Since voids in biased tracers are systematically larger than those identified in the dark matter field, a correction to the dark matter void size function is necessary. The scientific goals of this thesis work are the following: (i) to test the algorithm to clean void catalogues on Λ-cold dark matter (ΛCDM) N-body simulations, (ii) to quantify the accuracy of the theoretical void size function model with dark matter catalogues, (iii) to re-parametrise the theoretical model of the void size function for biased tracers, and (iv) to investigate the ...
The investigations of the large-scale structure of our Universe provide us with extremely powerful t...
Modern surveys allow us to access to high quality measurements, by sampling the galaxy distribution ...
Cosmic voids are a promising environment to characterize neutrino-induced effects on the large-scale...
Cosmic voids are large underdense regions that, together with galaxy clusters, filaments and walls, ...
The Standard Cosmological Model is generally accepted by the scientific community, there are still ...
Cosmic voids occupy most of the volume of the Universe, and their statistical properties can be expl...
A stately fraction of the Universe volume is dominated by almost empty space. Alongside the luminous...
In this work, we analyse the properties of cosmic voids in standard and coupled dark energy cosmolog...
We present the first cosmological constraints derived from the analysis of the void size function. T...
Cosmic voids are effective cosmological probes to discriminate among competing world models. Their i...
The large-scale structure of the universe can only be observed directly via luminous tracers of the ...
The last decade has witnessed the establishment of a Standard Cosmological Model, which is based on...
What do we know about voids in the dark matter distribution given the Sloan Digital Sky Survey (SDSS...
Luminous tracers of large-scale structure are not entirely representative of the distribution of mas...
none2noContext. We present new numerical tools to analyse cosmic void catalogues, implemented inside...
The investigations of the large-scale structure of our Universe provide us with extremely powerful t...
Modern surveys allow us to access to high quality measurements, by sampling the galaxy distribution ...
Cosmic voids are a promising environment to characterize neutrino-induced effects on the large-scale...
Cosmic voids are large underdense regions that, together with galaxy clusters, filaments and walls, ...
The Standard Cosmological Model is generally accepted by the scientific community, there are still ...
Cosmic voids occupy most of the volume of the Universe, and their statistical properties can be expl...
A stately fraction of the Universe volume is dominated by almost empty space. Alongside the luminous...
In this work, we analyse the properties of cosmic voids in standard and coupled dark energy cosmolog...
We present the first cosmological constraints derived from the analysis of the void size function. T...
Cosmic voids are effective cosmological probes to discriminate among competing world models. Their i...
The large-scale structure of the universe can only be observed directly via luminous tracers of the ...
The last decade has witnessed the establishment of a Standard Cosmological Model, which is based on...
What do we know about voids in the dark matter distribution given the Sloan Digital Sky Survey (SDSS...
Luminous tracers of large-scale structure are not entirely representative of the distribution of mas...
none2noContext. We present new numerical tools to analyse cosmic void catalogues, implemented inside...
The investigations of the large-scale structure of our Universe provide us with extremely powerful t...
Modern surveys allow us to access to high quality measurements, by sampling the galaxy distribution ...
Cosmic voids are a promising environment to characterize neutrino-induced effects on the large-scale...