The simulated 21 cm signal during the epoch of reionization: Full modeling of the Ly-α pumping

Astronomy and Astrophysics

Volumn 495, Issue 2, 2009, Pages 389-405

  Baek, S ^a   Di Matteo, P ^a   Semelin, B ^a   Combes, F ^a   Revaz, Y ^a,b  

^a CNRS   (France)

^b EPFL   (Switzerland)

Author keywords

Cosmology: early Universe; ISM: bubbles; ISM: HII regions; Methods: numerical; Radiative transfer

Indexed keywords

COMPUTER SIMULATION; COSMOLOGY; DIAGNOSTIC RADIOGRAPHY; EMISSION SPECTROSCOPY; FLUID DYNAMICS; GAS ABSORPTION; HEATING; HYDROGEN; IONIZATION OF GASES; NUMERICAL METHODS; POWER SPECTRUM; RADIATIVE TRANSFER; SPECTRUM ANALYSIS; SPIN DYNAMICS; TOMOGRAPHY;

BOX SIZES; COSMOLOGY: EARLY UNIVERSE; FIELD EFFECTS; HYDRODYNAMIC SHOCKS; INTERGALACTIC MEDIUMS; IONIZATION FRACTIONS; ISM: BUBBLES; ISM: HII REGIONS; KINETIC TEMPERATURES; METHODS: NUMERICAL; NEUTRAL HYDROGENS; NUMERICAL SIMULATIONS; POWER-SPECTRA; RED SHIFTS; REIONIZATION; SELF-CONSISTENT TREATMENTS; SOURCE MODELS; SPIN TEMPERATURES;

THERMAL EFFECTS;

EID: 61349126128     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810757     Document Type: Article

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