Results 101 to 110 of about 727 (169)
Do Minihalos Affect Cosmic Reionization?
The role of unresolved structures (“minihalos”) in determining the consumption of ionizing photons during cosmic reionization remains an unsolved problem in modeling cosmic reionization, despite recent extensive studies with small-box high-resolution ...
Nickolay Y. Gnedin
doaj +1 more source
On the Properties of Cosmological Ionization Fronts
We investigate the properties of cosmological ionization fronts during the epoch of reionization using the Cosmic Reionization on Computers simulations. By analyzing reionization timing maps, we characterize ionization front velocities and curvatures and
Hanjue Zhu, Nickolay Y. Gnedin
doaj +1 more source
Physics of Cosmic Reionization
Invited review (to be published by RSP), edited by R. Fabbri.
Choudhury, T. Roy, Ferrara, A.
openaire +2 more sources
Mass spectrometric detection of fleeting neutral intermediates generated in electrochemical reactions. [PDF]
Liu J +5 more
europepmc +1 more source
Simulating Cosmic Reionization at Large Scales I: the Geometry of Reionization
We present the first large-scale radiative transfer simulations of cosmic reionization, in a simulation volume of (100/h Mpc)^3, while at the same time capturing the dwarf galaxies which are primarily responsible for reionization. We achieve this by combining the results from extremely large, cosmological, N-body simulations with a new, fast and ...
Iliev, Ilian T. +5 more
openaire +2 more sources
The relation between the Lyman-$\alpha$ effective optical depth of quasar sightlines ($\tau_\mathrm{los}$) and the distribution of galaxies around them is an emerging probe of the connection between the first collapsed structures and the IGM properties ...
Enrico Garaldi +3 more
doaj +1 more source
A New Approach for Constraining Large-scale Temperature Fluctuations in the Intergalactic Medium
The reionization of helium is thought to occur at 2.5 ≲ z ≲ 4, marking the last phase transition and final global heating event of the intergalactic medium (IGM).
Saba Etezad-Razavi +2 more
doaj +1 more source
We present the evolution of Ly α emission derived from 53 galaxies at z = 6.6–13.2, which have been identified by multiple JWST/NIRSpec spectroscopy programs of Early Release Science, General Observer, Director's Discretionary Time, and Guaranteed Time ...
Minami Nakane +8 more
doaj +1 more source
Nearby primitive galaxies offer a window into the early universe. [PDF]
Croswell K.
europepmc +1 more source

