Inside-out or Outside-in: The topology of reionization in the photon-starved regime suggested by Lyman-alpha forest data
arXiv:0806.1524 · doi:10.1111/j.1365-2966.2008.14383.x
Abstract
We use a set of semi-numerical simulations based on Zel'dovich approximation, friends-of-friends algorithm and excursion set formalism to generate reionization maps of high dynamic range with a range of assumptions regarding the distribution and luminosity of ionizing sources and the spatial distribution of sinks for the ionizing radiation. We find that ignoring the inhomogeneous spatial distribution of regions of high gas density where recombinations are important -- as is often done in studies of this kind -- can lead to misleading conclusions regarding the topology of reionization, especially if reionization occurs in the photon-starved regime suggested by Lya forest data. The inhomogeneous spatial distribution of recombinations significantly reduces the mean free path of ionizing photons and the typical size of coherently ionized regions. Reionization proceeds then much more as an outside-in process. Low-density regions far from ionizing sources become ionized before regions of high gas density not hosting sources of ionizing radiation. The spatial distribution of sinks of ionization radiation also significantly affects shape and amplitude the power spectrum of fluctuations of 21cm emission. The slope of the 21cm power spectrum as measured by upcoming 21cm experiments should be able to distinguish to what extent the topology of reionization proceeds outside-in or inside-out while the evolution of the amplitude of the power spectrum with increasing ionized mass fraction should be sensitive to the spatial distribution and the luminosity of ionizing sources.
Accepted in MNRAS. Revised for clarification, matches the accepted version
References in corpus (22)
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Efficient Simulations of Early Structure Formation and Reionization
- The End of the Reionization Epoch Probed by Ly-alpha Emitters at z=6.5 in the Subaru Deep Field
- The morphology of HII regions during reionization
- The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >5: Evidence for a photon starved and extended epoch of reionization
- The Global 21 Centimeter Background from High Redshifts
- Cosmological Radiative Transfer Codes Comparison Project I: The Static Density Field Tests
- Simulating Cosmic Reionization at Large Scales II: the 21-cm Emission Features and Statistical Signals
- Evolution of the 21 cm signal throughout cosmic history
- Self-regulated reionization
- Detecting the Rise and Fall of 21 cm Fluctuations with the Murchison Widefield Array
- Probing Reionization with the 21 cm-Galaxy Cross Power Spectrum
- The Lyman-alpha forest and WMAP year three
- UV Radiative Feedback During the Advanced Stages of Reionization
- Updating reionization scenarios after recent data
- Escape fraction of ionizing photons from galaxies at z=0--6
- On the minimum mass of reionization sources
- The correlation between the distribution of galaxies and 21cm emission at high redshifts
- Quasar H II Regions During Cosmic Reionization
- Are There Enough Ionizing Photons to Reionize the Universe by z=6?
Cited by in corpus (71)
- Evidence of patchy hydrogen reionization from an extreme Ly trough below redshift six
- New observations of z~7 galaxies: evidence for a patchy reionization
- Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization
- The First Billion Years Project: The escape fraction of ionizing photons in the epoch of reionization
- Rapid Decline of Lyman-alpha Emission Toward the Reionization Era
- Probing the thermal state of the intergalactic medium at with the transmission spikes in high-resolution Ly forest spectra
- Reionization and galaxy inference from the high-redshift Lyα forest
- Lyman-alpha emitters gone missing: evidence for late reionization?
- 21 cm signal from cosmic dawn: Imprints of spin temperature fluctuations and peculiar velocities
- Constraining the UV emissivity of AGN throughout cosmic time via X-ray surveys
- Hydrodynamic Response of the Intergalactic Medium to Reionization
- Imaging the redshifted 21-cm pattern around the first sources during the cosmic dawn using the SKA
- The effect of non-Gaussianity on error predictions for the Epoch of Reionization (EoR) 21-cm power spectrum
- Modelling the observed luminosity function and clustering evolution of Lyman- emitters: growing evidence for late reionization
- A New Moment Method for Continuum Radiative Transfer in Cosmological Reionization
- Towards simulating and quantifying the light-cone EoR 21-cm signal
- Re-examining the case for neutral gas near the redshift 7 quasar ULAS J1120+0641
- Large scale simulations of H and He reionization and heating driven by stars and more energetic sources
- AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
- Redshifted 21-cm Bispectrum I: Impact of the Redshift Space Distortions on the Signal from the Epoch of Reionization
- Epoch of Reionisation 21cm Forecasting From MCMC-Constrained Semi-Numerical Models
- Fluctuations in the Ionizing Background During and After Helium Reionization
- Redshifted 21-cm bispectrum II: Impact of the spin temperature fluctuations and redshift space distortions on the signal from the Cosmic Dawn
- Improving constraints on the reionization parameters using 21-cm bispectrum
- A Short Introduction to Reionization Physics
- The impact of non-Gaussianity on the error covariance for observations of the Epoch of Reionization 21-cm power spectrum
- Models of the Cosmological 21 cm Signal from the Epoch of Reionization Calibrated with Lyman-alpha and CMB Data
- Large-scale environment of z~5.7 CIV absorption systems I: projected distribution of galaxies
- The importance of galaxy formation histories in models of reionization
- Probing the thermal history during reionization using a semi-numerical photon-conserving code SCRIPT
- Improved treatments of the ionizing photon mean free path in semi-numerical simulations of reionization
- The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
- Simulating the impact of HI fluctuations on matched filter search for ionized bubbles in redshifted 21 cm maps
- The Epoch of Reionization 21-cm Bispectrum: The impact of light-cone effects and detectability
- The impact of non-Gaussianity on the Epoch of Reionization parameter forecast using 21-cm power spectrum measurements
- Inevitable imprints of patchy reionization on the cosmic microwave background anisotropy
- Constraining the reionization and thermal history of the Universe using a semi-numerical photon-conserving code SCRIPT
- Observing the Reionization : Effect of Calibration and Position Errors on Realistic Observation Conditions
- Impact of dark matter models on the EoR 21-cm signal bispectrum
- Constraining the Epoch of Reionization With Highly Dispersed Fast Radio Bursts
- Revisiting the [C II] line-intensity mapping power spectrum from the EoR using non-uniform line-luminosity scatter
- Constraints on Dark Matter-Neutrino Interaction from 21-cm Cosmology and Forecasts on SKA1-Low
- Revised estimates of CMB -mode polarization induced by patchy reionization
- Probing early universe through redshifted 21-cm signal: Modelling and observational challenges
- Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
- Quantifying Density-Ionization Correlations with the 21cm Power Spectrum
- 21-cm signatures of residual HI inside cosmic HII regions during reionization
- CII and HI 21-cm line intensity mapping from the EoR: Impact of the light-cone effect on auto and cross-power spectra
- Is patchy reionization an obstacle in detecting the primordial gravitational wave signal?
- Redshifted 21-cm bispectrum: Impact of the source models on the signal and the IGM physics from the Cosmic Dawn
- Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
- The monopole and quadrupole moments of the Epoch of Reionization (EoR) 21-cm bispectrum
- Distinguishing reionization models using the largest cluster statistics of the 21-cm maps
- Spatial Correlations in the Helium-Ionizing Background
- Line of sight anisotropies in the Cosmic Dawn and EoR 21-cm power spectrum
- Modelling the 21 cm Signal From the Epoch of Reionization and Cosmic Dawn
- Impact of the Epoch of Reionization sources on the 21-cm bispectrum
- Lyman Alpha Emitters and the 21cm Power Spectrum as Probes of Density-Ionization Correlation in the Epoch of Reionization
- Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
- Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics -- I: Impact of the synthetic SKA1-Low observations
- Calibrating excursion set reionization models to approximately conserve ionizing photons
- Impact of astrophysical scatter on the Epoch of Reionization [H I] bispectrum
- Probing the Epoch of Reionization using synergies of line intensity mapping
- The Linear Perturbation Theory of Reionization in Position-Space: Cosmological Radiative Transfer Along the Light-Cone
- Ionospheric effect on the synthetic Epoch of Reionization observations with the SKA1-Low
- Reionization relics in the cross-correlation between the Ly forest and 21 cm intensity mapping in the post-reionization era
- Synthetic Observations with the Square Kilometre Array (SKA) -- development towards an end-to-end pipeline
- Accelerating HI density predictions during the Epoch of Reionization using a GPR-based emulator on N-body simulations
- From ANN to BNN: Inferring Reionization Parameters using Uncertainty-aware Emulators of 21-cm Summaries
- CosmoUiT: A Vision Transformer-UNet Hybrid for Fast and Accurate Emulation of 21-cm Maps from the Epoch of Reionization
- Quantifying and mitigating the effect of snapshot interval in light-cone Epoch of Reionization 21-cm simulations