Measuring the topology of reionization with Betti numbers
arXiv:2012.12908 · doi:10.1093/mnras/stab1320
Abstract
The distribution of ionised hydrogen during the epoch of reionization (EoR) has a complex morphology. We propose to measure the three-dimensional topology of ionised regions using the Betti numbers. These quantify the topology using the number of components, tunnels and cavities in any given field. Based on the results for a set of reionization simulations we find that the Betti numbers of the ionisation field show a characteristic evolution during reionization, with peaks in the different Betti numbers characterising different stages of the process. The shapes of their evolutionary curves can be fitted with simple analytical functions. We also observe that the evolution of the Betti numbers shows a clear connection with the percolation of the ionized and neutral regions and differs between different reionization scenarios. Through these properties, the Betti numbers provide a more useful description of the topology than the widely studied Euler characteristic or genus. The morphology of the ionisation field will be imprinted on the redshifted 21-cm signal from the EoR. We construct mock image cubes using the properties of the low-frequency element of the future Square Kilometre Array and show that we can extract the Betti numbers from such datasets if an observation time of 1000 h is used. Even for a much shorter observation time of 100 h, some topological information can be extracted for the middle and later stages of reionization. We also find that the topological information extracted from the mock 21-cm observations can put constraints on reionization models.
15 pages, 11 figures, 3 tables. Accepted to MNRAS
References in corpus (21)
- scikit-image: Image processing in Python
- Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe
- Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR
- 21 cm fluctuations from inhomogeneous X-ray heating before reionization
- Foreground simulations for the LOFAR - Epoch of Reionization Experiment
- 21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal
- Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations
- Simulating Cosmic Reionization at Large Scales II: the 21-cm Emission Features and Statistical Signals
- Signature of Excess Radio Background in the 21-cm Global Signal and Power Spectrum
- The Effects of Dark Matter-Baryon Scattering on Redshifted 21 cm Signals
- Constraining the intergalactic medium at 9.1 using LOFAR Epoch of Reionization observations
- Bubble size statistics during reionization from 21-cm tomography
- Imaging the redshifted 21-cm pattern around the first sources during the cosmic dawn using the SKA
- Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
- The morphology of cosmological reionization by means of Minkowski Functionals
- A Space-Based Observational Strategy for Characterizing the First Stars and Galaxies Using the Redshifted 21-cm Global Spectrum
- The Topology of Cosmological Reionization
- Topological signatures of interstellar magnetic fields - I. Betti numbers and persistence diagrams
- Using Artificial Neural Networks to Constrain the Halo Baryon Fraction during Reionization
- Opening Reionization: Quantitative Morphology of the Epoch of Reionization and Its Connection to the Cosmic Density Field
- Studying neutral hydrogen structures during the epoch of reionization using fractal dimensions
Cited by in corpus (28)
- Simulation-Based Inference of Reionization Parameters From 3D Tomographic 21 cm Lightcone Images
- Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
- On the sizes of ionized bubbles around the highest redshift galaxies. Spectral shapes of the Lyman-alpha emission from galaxies
- Deep learning approach for identification of HII regions during reionization in 21-cm observations
- Exploring the cosmic 21-cm signal from the Epoch of Reionisation using the Wavelet Scattering Transform
- Inferring the properties of the sources of reionization using the morphological spectra of the ionized regions
- Studying Cosmic Dawn using redshifted HI 21-cm signal: A brief review
- The THESAN project: connecting ionized bubble sizes to their local environments during the Epoch of Reionization
- Deep learning approach for identification of HII regions during reionization in 21-cm observations -- II. foreground contamination
- BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn
- The large-scale 21-cm power spectrum from reionization
- How informative are summaries of the cosmic 21-cm signal?
- Detecting the non-Gaussianity of the 21-cm signal during reionisation with the Wavelet Scattering Transform
- Persistent topology of the reionization bubble network. II: Evolution & Classification
- SKA-Low Intensity Mapping Pathfinder Updates: Deeper 21 cm Power Spectrum Limits from Improved Analysis Frameworks
- Probing the intergalactic medium during the Epoch of Reionization using 21-cm signal power spectra
- Distinguishing reionization models using the largest cluster statistics of the 21-cm maps
- Differentiating small-scale subhalo distributions in CDM and WDM models using persistent homology
- Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics -- I: Impact of the synthetic SKA1-Low observations
- Probing the Epoch of Reionization using synergies of line intensity mapping
- Topology of Reionisation times: concepts, measurements and comparisons to gaussian random field predictions
- Reionization Parameter Inference from 3D Minkowski Functionals of the 21 cm Signals
- On the evolution of Betti curves in the Cosmic web
- Impact of anisotropic photon emission from sources during the epoch of reionisation
- Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
- A first look at the topology of reionization redshifts in models of the Epoch of the Reionization
- Interpreting the HI 21-cm cosmology maps through Largest Cluster Statistics. Part II. Impact of the realistic foreground and instrumental noise on synthetic SKA1-Low observations
- Power spectrum multipoles and clustering wedges during the Epoch of Reionization