Suppressing variance in 21-cm signal simulations during reionization
arXiv:2209.01225 · doi:10.1051/0004-6361/202244986
Abstract
Current best limits on the 21-cm signal during reionization are provided at large scales (100 Mpc). To model these scales, enormous simulation volumes are required which are computationally expensive. We find that the primary source of uncertainty at these large scales is sample variance, which decides the minimum size of simulations required to analyse current and upcoming observations. In large-scale structure simulations, the method of `fixing' the initial conditions (ICs) to exactly follow the initial power spectrum and `pairing' two simulations with exactly out-of-phase ICs has been shown to significantly reduce sample variance. Here we apply this `fixing and pairing' (F\&P) approach to reionization simulations whose clustering signal originates from both density fluctuations and reionization bubbles. Using a semi-numerical code, we show that with the traditional method, simulation boxes of (300) Mpc are required to model the large-scale clustering signal at =0.1 Mpc with a precision of 5 (10) per cent. Using F\&P, the simulation boxes can be reduced by a factor of 2 to obtain the same precision level. We conclude that the computing costs can be reduced by at least a factor of 4 when using the F\&P approach.
arXiv comment5 pages, 4 figures, accepted for publication in A&A
References in corpus (36)
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- 21-cm cosmology
- Power Spectra for Cold Dark Matter and its Variants
- 21cmFAST: A Fast, Semi-Numerical Simulation of the High-Redshift 21-cm Signal
- The Growth of HII Regions During Reionization
- Efficient Simulations of Early Structure Formation and Reionization
- The Quijote simulations
- Improved upper limits on the 21-cm signal power spectrum of neutral hydrogen at from LOFAR
- Insights on Dark Matter from Hydrogen during Cosmic Dawn
- Inferring the astrophysics of reionization and cosmic dawn from galaxy luminosity functions and the 21-cm signal
- 21CMMC: an MCMC analysis tool enabling astrophysical parameter studies of the cosmic 21 cm signal
- Introducing the THESAN project: radiation-magnetohydrodynamic simulations of the epoch of reionization
- Deep multi-redshift limits on Epoch of Reionisation 21cm Power Spectra from Four Seasons of Murchison Widefield Array Observations
- First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum
- The BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology
- Cosmological -body simulations with suppressed variance
- Simulating cosmic reionization: How large a volume is large enough?
- Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
- Quantifying the non-Gaussianity in the EoR 21-cm signal through bispectrum
- Constraining the intergalactic medium at 9.1 using LOFAR Epoch of Reionization observations
- Constraining Non-Cold Dark Matter Models with the Global 21-cm Signal
- Tight Constraints on the Excess Radio Background at from LOFAR
- Constraining the primordial black hole abundance with 21cm cosmology
- Statistical properties of paired fixed fields
- Constraining the state of the intergalactic medium during the Epoch of Reionization using MWA 21-cm signal observations
- Inverted initial conditions: exploring the growth of cosmic structure and voids
- A halo model approach for the 21-cm power spectrum at cosmic dawn
- The effect of primordial black holes on 21 cm fluctuations
- Dark Matter microphysics and 21 cm observations
- Minimum size of 21-cm simulations
- Redshift-space distortions in simulations of the 21-cm signal from the cosmic dawn
- Small-scale primordial fluctuations in the 21cm Dark Ages signal
- The large-scale 21-cm power spectrum from reionization
- Statistics of biased tracers in variance-suppressed simulations
- The 21-cm signals from ultracompact minihalos as a probe of primordial small-scale fluctuations
- Generating extremely large-volume reionisation simulations
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- BEoRN: A fast and flexible framework to simulate the epoch of reionisation and cosmic dawn
- pyCRay: A flexible and GPU-accelerated Radiative Transfer Framework for Simulating the Cosmic Epoch of Reionization
- Efficient exploration of reionization parameters for the upcoming 21 cm observations using a photon conserving semi-numerical model SCRIPT
- Mapping neutral islands during end stages of reionization with photometric intergalactic medium tomography
- Impact of anisotropic photon emission from sources during the epoch of reionisation
- Sample Variance Denoising in Cylindrical 21-cm Power Spectra