The first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization fronts sweeping outward through their surroundings, overtaking other condensed objects and photoevaporating them. This feedback of universal reionization on cosmic structure formation is demonstrated here by gas dynamical simulations, including radiative transfer, for a cosmological minihalo of dark matter and baryons exposed to an external source of ionizing radiation, either starlight or quasar light, just after the passage of the global ionization front created by the source
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
Understanding the epoch of reionization and the properties of the first galaxies rep-resents an impo...
An ionizing ultraviolet background (UVB) inhibits gas accretion and photoevaporates gas from the sha...
The first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization ...
We present the first gas dynamical simulations of the photoevaporation of cosmological minihalos ove...
We examine the epoch of hydrogen reionization using a new numerical method that allows us to self-co...
The reionization is a milestone in the history of the universe which is still poorly understood. We ...
The first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization ...
At the earliest epochs of structure formation in cold dark matter (CDM) cosmologies, the smallest no...
In this thesis we investigate numerically how ionizing photons emitted by stars in galaxies cause th...
textIonized intergalactic medium (IGM) is an important component in cosmic history. After recombinat...
We have studied the IGM reionization process in its full cosmological context including structure ev...
The first, self-consistent calculations of the cosmological H2 dissociating UV background produced d...
We introduce a new self-consistent model of galaxy evolution and reionization, ASTRAEUS (seminumeric...
The intergalactic medium was reionized before redshift z ∼ 6, most likely by starlight which escaped...
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
Understanding the epoch of reionization and the properties of the first galaxies rep-resents an impo...
An ionizing ultraviolet background (UVB) inhibits gas accretion and photoevaporates gas from the sha...
The first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization ...
We present the first gas dynamical simulations of the photoevaporation of cosmological minihalos ove...
We examine the epoch of hydrogen reionization using a new numerical method that allows us to self-co...
The reionization is a milestone in the history of the universe which is still poorly understood. We ...
The first sources of ionizing radiation to condense out of the dark and neutral IGM sent ionization ...
At the earliest epochs of structure formation in cold dark matter (CDM) cosmologies, the smallest no...
In this thesis we investigate numerically how ionizing photons emitted by stars in galaxies cause th...
textIonized intergalactic medium (IGM) is an important component in cosmic history. After recombinat...
We have studied the IGM reionization process in its full cosmological context including structure ev...
The first, self-consistent calculations of the cosmological H2 dissociating UV background produced d...
We introduce a new self-consistent model of galaxy evolution and reionization, ASTRAEUS (seminumeric...
The intergalactic medium was reionized before redshift z ∼ 6, most likely by starlight which escaped...
We present results on the evolution of dark matter halos and reionization. Dark matter halos enshro...
Understanding the epoch of reionization and the properties of the first galaxies rep-resents an impo...
An ionizing ultraviolet background (UVB) inhibits gas accretion and photoevaporates gas from the sha...