Is the cosmic UV background fluctuating at redshift z ~ 6 ?
arXiv:astro-ph/0605614 · doi:10.1086/506149
Abstract
We study the Gunn-Peterson effect of the photo-ionized intergalactic medium(IGM) in the redshift range 5< z <6.4 using semi-analytic simulations based on the lognormal model. Assuming a rapidly evolved and spatially uniform ionizing background, the simulation can produce all the observed abnormal statistical features near redshift z ~ 6. They include: 1) rapidly increase of absorption depths; 2) large scatter in the optical depths; 3) long-tailed distributions of transmitted flux and 4) long dark gaps in spectra. These abnormal features are mainly due to rare events, which correspond to the long-tailed probability distribution of the IGM density field, and therefore, they may not imply significantly spatial fluctuations in the UV ionizing background at z ~ 6.
12 pages, 4 figs, accepted by ApJL
References in corpus (32)
- Equation of State of the Photoionized Intergalactic Medium
- Evolution of the Ionizing Background and the Epoch of Reionization from the Spectra of z~6 Quasars
- The Lyman Alpha Forest in the Spectra of QSOs
- Luminosity functions of Lyman-alpha emitters at z=6.5, and z=5.7: evidence against reionization at z=6
- Evolution of Structure in the Intergalactic Medium and the Nature of the Ly-alpha Forest
- Probing the Ionization State of the Universe at z>6
- The Evolution of the Intergalactic Medium Transmission to Redshift Six
- Evolution of One-Point Distributions from Gaussian Initial Fluctuations
- Approaching Reionization: The Evolution of the Lyman Alpha Forest from Redshifts Four to Six
- Cosmological Hydrogen Reionization with Three Dimensional Radiative Transfer
- Discovery of excess O I absorption towards the z = 6.42 QSO SDSS J1148+5251
- Reionization, SLOAN, and WMAP: is the Picture Consistent?
- A first step towards a direct inversion of the Lyman forest in QSO spectra
- Have We Detected Patchy Reionization in Quasar Spectra?
- Undetected Sources Allow Transmission of the Lyman-alpha Line From Galaxies Prior to Reionization
- The growth of structure in the intergalactic medium
- Semi analytic approach to understanding the distribution of neutral hydrogen in the universe: Comparison of simulations with observations
- A Simulation of Ly-alpha Absorption Forests in Linear Approximation in Cold and Cold+Hot Dark Matter Models
- Stochastic fluctuations and structure formation in the Universe
- Non-Gaussianity and the recovery of the mass power spectrum from the Ly forest
- A Statistical Analysis of Intergalactic Medium Transmission Approaching Reionization
- Temperature and Entropy Fields of Baryonic Gas in the Universe
- Measuring the galaxy power spectrum with multiresolution decomposition -- III. velocity field analysis
- Intermittent Features of the QSO Ly Transmitted Flux: Results from Hydrodynamic Cosmological Simulations
- Intermittent behavior of cosmic mass field revealed by QSO's Ly_alpha forests
- Multiple-streaming and the Probability Distribution of Density in Redshift Space
- Non-Gaussian Features of Transmitted Flux of QSO's Ly Absorption: Intermittent Exponent
- Power spectrum and intermittency of the transmitted flux of QSOs Ly-alpha absorption spectra
- The intermittent behavior and hierarchical clustering of the cosmic mass field
- Hydrogen Clouds before Reionization: a Lognormal Model Approach
- The local power spectrum and correlation hierarchy of the cosmic mass field
- Power Spectrum and Intermittency of Ly Transmitted Flux of QSO He2347-4342
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- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Studying Reionization with Ly-alpha Emitters
- The Evolution of Optical Depth in the Ly-alpha Forest: Evidence Against Reionization at z~6
- The nature and evolution of the highly ionized near-zones in the absorption spectra of z~6 quasars
- Quasar Proximity Zones and Patchy Reionization
- Glimpsing through the high redshift neutral hydrogen fog
- Log-Poisson Non-Gaussianity of Ly Transmitted Flux Fluctuations at High Redshift
- Ly Leaks in the Absorption Spectra of High Redshift QSOs
- Ly Leaks and Reionization