In this paper, we investigate the nature and distribution of large neutral regions during the late epoch of reionization. In the "bubble model" of reionization, the mass distribution of large ionized regions ("bubbles") during the early stage of reionization is obtained by using the excursion set model, where the ionization of a region corresponds to the first up-crossing of a barrier by random trajectories. We generalize this idea and develop a method to predict the distribution of large-scale neutral regions during the late stage of reionization, taking into account the ionizing background after the percolation of H II regions. The large-scale neutral regions, which we call "neutral islands," are not individual galaxies or minihalos, but ...
Based on observations of the early Universe, we know that shortly after the Big Bang, the Universe w...
One of the most sought-after signatures of reionization is a rapid increase in the ionizing backgrou...
We present results from a large volume simulation of Hydrogen reionization. We combine 3d radia-tive...
In this paper, we investigate the nature and distribution of large neutral regions during the late e...
In this paper, we investigate the nature and distribution of large neutral regions during the late e...
We present the prospects of extracting information about the epoch of reionization by identifying th...
We present predictions for two statistical measures of the hydrogen reionization process at high red...
A key physical quantity during reionization is the size of H II regions. Previous studies found a ch...
The size distribution of ionized regions during the epoch of reionization – a key ingredient in unde...
We use the results of large-scale simulations of reionization to explore methods for characterizing ...
After the era of recombination, roughly 360 000 years after the big bang (redshift 1100), the univer...
International audienceContext. During the epoch of reionisation (EoR), the first stars and galaxies ...
Philosophiae Doctor - PhD (Physics)We improve on the physical treatment of ionising source and sink ...
We consider the early stages of cosmic hydrogen or helium reionization, when ionizing sources were s...
The visibility of Lyα-emitting galaxies during the Epoch of Reionization is controlled by both diffu...
Based on observations of the early Universe, we know that shortly after the Big Bang, the Universe w...
One of the most sought-after signatures of reionization is a rapid increase in the ionizing backgrou...
We present results from a large volume simulation of Hydrogen reionization. We combine 3d radia-tive...
In this paper, we investigate the nature and distribution of large neutral regions during the late e...
In this paper, we investigate the nature and distribution of large neutral regions during the late e...
We present the prospects of extracting information about the epoch of reionization by identifying th...
We present predictions for two statistical measures of the hydrogen reionization process at high red...
A key physical quantity during reionization is the size of H II regions. Previous studies found a ch...
The size distribution of ionized regions during the epoch of reionization – a key ingredient in unde...
We use the results of large-scale simulations of reionization to explore methods for characterizing ...
After the era of recombination, roughly 360 000 years after the big bang (redshift 1100), the univer...
International audienceContext. During the epoch of reionisation (EoR), the first stars and galaxies ...
Philosophiae Doctor - PhD (Physics)We improve on the physical treatment of ionising source and sink ...
We consider the early stages of cosmic hydrogen or helium reionization, when ionizing sources were s...
The visibility of Lyα-emitting galaxies during the Epoch of Reionization is controlled by both diffu...
Based on observations of the early Universe, we know that shortly after the Big Bang, the Universe w...
One of the most sought-after signatures of reionization is a rapid increase in the ionizing backgrou...
We present results from a large volume simulation of Hydrogen reionization. We combine 3d radia-tive...