Euclid preparation: IX. EuclidEmulator2 -- Power spectrum emulation with massive neutrinos and self-consistent dark energy perturbations
arXiv:2010.11288 · doi:10.1093/mnras/stab1366
Abstract
We present a new, updated version of the EuclidEmulator (called EuclidEmulator2), a fast and accurate predictor for the nonlinear correction of the matter power spectrum. Percent-level accurate emulation is now supported in the eight-dimensional parameter space of CDMmodels between redshift and for spatial scales within the range 0.01 /Mpc 10 /Mpc. In order to achieve this level of accuracy, we have had to improve the quality of the underlying N-body simulations used as training data: (1) we use self-consistent linear evolution of non-dark matter species such as massive neutrinos, photons, dark energy and the metric field, (2) we perform the simulations in the so-called N-body gauge, which allows one to interpret the results in the framework of general relativity, (3) we run over 250 high-resolution simulations with particles in boxes of 1 (Gpc/) volumes based on paired-and-fixed initial conditions and (4) we provide a resolution correction that can be applied to emulated results as a post-processing step in order to drastically reduce systematic biases on small scales due to residual resolution effects in the simulations. We find that the inclusion of the dynamical dark energy parameter significantly increases the complexity and expense of creating the emulator. The high fidelity of EuclidEmulator2 is tested in various comparisons against N-body simulations as well as alternative fast predictors like Halofit, HMCode and CosmicEmu. A blind test is successfully performed against the Euclid Flagship v2.0 simulation. Nonlinear correction factors emulated with EuclidEmulator2 are accurate at the level of 1% or better for 0.01 /Mpc 10 /Mpc and compared to high-resolution dark matter only simulations. EuclidEmulator2 is publicly available at https://github.com/miknab/EuclidEmulator2 .
arXiv comment28 pages, 19 figures, submitted to MNRAS
References in corpus (79)
- Planck 2015 results. XIII. Cosmological parameters
- Discussion of "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Least Angle Regression
- Discussion of "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Rejoinder to "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Discussion of "Least angle regression" by Efron et al
- Evidence for oscillation of atmospheric neutrinos
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- Improved cosmological constraints from a joint analysis of the SDSS-II and SNLS supernova samples
- Revising the Halofit Model for the Nonlinear Matter Power Spectrum
- The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
- Measurement of the Total Active 8B Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity
- Measurements of the Solar Neutrino Flux from Super-Kamiokande's First 300 Days
- Three-flavour neutrino oscillation update
- A Parameterized Post-Friedmann Framework for Modified Gravity
- The Cosmic Linear Anisotropy Solving System (CLASS) IV: Efficient implementation of non-cold relics
- Massive Neutrinos and the Non-linear Matter Power Spectrum
- The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum
- The fourth data release of the Kilo-Degree Survey: ugri imaging and nine-band optical-IR photometry over 1000 square degrees
- An active-learning algorithm that combines sparse polynomial chaos expansions and bootstrap for structural reliability analysis
- Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces
- Crossing the Phantom Divide with Parameterized Post-Friedmann Dark Energy
- The Coyote Universe II: Cosmological Models and Precision Emulation of the Nonlinear Matter Power Spectrum
- The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
- The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium
- Learning to Predict the Cosmological Structure Formation
- Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
- The Coyote Universe III: Simulation Suite and Precision Emulator for the Nonlinear Matter Power Spectrum
- Cosmological -body simulations with suppressed variance
- Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
- Chi**2 analysis of the minimal supergravity model including WMAP, g(mu)-2 and b -> s gamma constraints
- Matter power spectrum and the challenge of percent accuracy
- Data-driven polynomial chaos expansion for machine learning regression
- Numerical studies of space filling designs: optimization of Latin Hypercube Samples and subprojection properties
- Neutrino masses and cosmological parameters from a Euclid-like survey: Markov Chain Monte Carlo forecasts including theoretical errors
- gevolution: a cosmological N-body code based on General Relativity
- The Aemulus Project I: Numerical Simulations for Precision Cosmology
- The Mira-Titan Universe: Precision Predictions for Dark Energy Surveys
- The Mira-Titan Universe II: Matter Power Spectrum Emulation
- The Aemulus Project III: Emulation of the Galaxy Correlation Function
- The Aemulus Project II: Emulating the Halo Mass Function
- Connection between Newtonian simulations and general relativity
- The Abacus Cosmos: A Suite of Cosmological N-body Simulations
- A High-Fidelity Realization of the Euclid Code Comparison -body Simulation with Abacus
- Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
- Relativistic N-body simulations with massive neutrinos
- Improving Initial Conditions for Cosmological -Body Simulations
- Constraints on Neutrino Masses from Weak Lensing
- General relativistic corrections to -body simulations and the Zel'dovich approximation
- The effect of massive neutrinos on the matter power spectrum
- Bayesian emulator optimisation for cosmology: application to the Lyman-alpha forest
- An Efficient and Accurate Hybrid Method for Simulating Non-Linear Neutrino Structure
- Emulators for the non-linear matter power spectrum beyond CDM
- The halo model in a massive neutrino cosmology
- Constraining Neutrino Mass with the Tomographic Weak Lensing Bispectrum
- Baryonic effects for weak lensing. Part II. Combination with X-ray data and extended cosmologies
- Fitting the nonlinear matter bispectrum by the Halofit approach
- On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
- Reducing Noise in Cosmological N-body Simulations with Neutrinos
- Fully relativistic treatment of light neutrinos in -body simulations
- Precision modelling of the matter power spectrum in a Planck-like Universe
- The HDUV Survey: Six Lyman Continuum Emitter Candidates at z~2 Revealed by HST UV Imaging
- Cosmological -body simulations including radiation perturbations
- Simulating cosmologies beyond CDM with PINOCCHIO
- Spoon or slide? The non-linear matter power spectrum in the presence of massive neutrinos
- Dark energy perturbations in -body simulations
- Neutrinos in Non-linear Structure Formation - a Simple SPH Approach
- BE-HaPPY: Bias Emulator for Halo Power Spectrum including massive neutrinos
- Fully relativistic treatment of decaying cold dark matter in -body simulations
- Towards determining the neutrino mass hierarchy: weak lensing and galaxy clustering forecasts with baryons and intrinsic alignments
- First observation of the decay
- Dynamical modelling of dwarf-spheroidal galaxies using Gaussian-process emulation
- Neutrino masses and oscillations
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- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- COSMOPOWER: emulating cosmological power spectra for accelerated Bayesian inference from next-generation surveys
- Large-scale dark matter simulations
- DES Y3 + KiDS-1000: Consistent cosmology combining cosmic shear surveys
- Joint constraints on cosmology and the impact of baryon feedback: combining KiDS-1000 lensing with the thermal Sunyaev-Zeldovich effect from Planck and ACT
- The MillenniumTNG Project: High-precision predictions for matter clustering and halo statistics
- DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
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- The BACCO simulation project: biased tracers in real space
- The Mira-Titan Universe IV. High Precision Power Spectrum Emulation
- CONNECT: A neural network based framework for emulating cosmological observables and cosmological parameter inference
- Euclid. V. The Flagship galaxy mock catalogue: a comprehensive simulation for the Euclid mission
- Growth of Cosmic Structure
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- On the road to percent accuracy V: the non-linear power spectrum beyond CDM with massive neutrinos and baryonic feedback
- Aemulus : Precise Predictions for Matter and Biased Tracer Power Spectra in the Presence of Neutrinos
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- CosmoGridV1: a simulated CDM theory prediction for map-level cosmological inference
- Euclid preparation. Sensitivity to neutrino parameters
- Machine Learning for Observational Cosmology
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- COMET: Clustering Observables Modelled by Emulated perturbation Theory
- Cosmological Constraints from the eBOSS Lyman- Forest using the PRIYA Simulations
- Euclid: Modelling massive neutrinos in cosmology -- a code comparison
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- Enabling matter power spectrum emulation in beyond-CDM cosmologies with COLA
- Redshift requirements for cosmic shear with intrinsic alignment
- The e-MANTIS emulator: fast predictions of the non-linear matter power spectrum in CDM cosmology
- Euclid preparation. XLI. Galaxy power spectrum modelling in real space
- LINNA: Likelihood Inference Neural Network Accelerator
- The Aemulus Project VI: Emulation of beyond-standard galaxy clustering statistics to improve cosmological constraints
- A precise symbolic emulator of the linear matter power spectrum
- The matter density PDF for modified gravity and dark energy with Large Deviations Theory
- Evolution mapping: a new approach to describe matter clustering in the non-linear regime
- syren-new: Precise formulae for the linear and nonlinear matter power spectra with massive neutrinos and dynamical dark energy
- The cosmological simulation code
- Sesame: A power spectrum emulator pipeline for beyond-CDM models
- An empirical approach to model selection: weak lensing and intrinsic alignments
- Suppressing variance in 21-cm signal simulations during reionization
- A revised density split statistic model for general filters
- A Multi-Fidelity Emulator for the Lyman- Forest Flux Power Spectrum
- The BAHAMAS project: Evaluating the accuracy of the halo model in predicting the non-linear matter power spectrum
- Revisiting Vainshtein Screening for fast N-body simulations
- Galaxy Clustering in the Mira-Titan Universe I: Emulators for the redshift space galaxy correlation function and galaxy-galaxy lensing
- On the degeneracies between baryons, massive neutrinos and f(R) gravity in Stage IV cosmic shear analyses
- Fast likelihood-free inference in the LSS Stage IV era
- A representation learning approach to probe for dynamical dark energy in matter power spectra
- Fully relativistic predictions in Horndeski gravity from standard Newtonian N-body simulations
- A field-level emulator for modeling baryonic effects across hydrodynamic simulations
- Fast generation of mock galaxy catalogues with COLA
- Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses
- A field-level emulator for modified gravity
- Growth and Geometry Split in Light of the DES-Y3 Survey
- Euclid preparation LXXI. Simulations and nonlinearities beyond CDM. 3. Constraints on models from the photometric primary probes
- CSST Cosmological Emulator II: Generalized Accurate Halo Mass Function Emulation
- MF-Box: Multi-fidelity and multi-scale emulation for the matter power spectrum
- Euclid preparation. Sensitivity to non-standard particle dark matter model
- Prospects for disentangling dark matter with weak lensing
- Dynamics of pairwise motions in the fully non-linear regime in LCDM and Modified Gravity cosmologies
- Cosmological Inference with Cosmic Voids and Neural Network Emulators
- Assessing theoretical uncertainties for cosmological constraints from weak lensing surveys
- The BACCO Simulation Project: A baryonification emulator with Neural Networks
- jaxspec : a fast and robust Python library for X-ray spectral fitting
- Cosmological perturbation theory for large scale structure in phase space
- Cosmological gravity on all scales IV: 3x2pt Fisher forecasts for pixelised phenomenological modified gravity
- Updated neutrino mass constraints from galaxy clustering and CMB lensing-galaxy cross-correlation measurements
- Extending evolution mapping to massive neutrinos with COMET
- Cosmological parameters from the joint analysis of Density Split and Second Order Statistics: an Emulator based on the Halo Occupation Distribution
- Aemulus : Precision halo mass functions in wCDM cosmologies
- Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
- Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
- Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
- Ten-dimensional neural network emulator for the nonlinear matter power spectrum
- Design and optimization of neural networks for multifidelity cosmological emulation
- Power Spectrum Emulators from Neural Networks and Tree-Based Methods
- Emulating the Non-Linear Matter Power-Spectrum in Mixed Axion Dark Matter Models
- Simulation budgeting for hybrid effective field theories
- Cosmic magnification on high-redshift submillimeter galaxies
- A semi-analytic estimate for the effective sound speed counterterm in the EFTofLSS
- Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
- On the road to percent accuracy VI: the nonlinear power spectrum for interacting dark energy with baryonic feedback and massive neutrinos
- Constraining cosmological parameters using density split lensing and the conditional stellar mass function
- Aletheia: Emulating the non-linear matter power spectrum in the context of evolution mapping
- A simple prediction of the nonlinear matter power spectrum in Brans-Dicke gravity from linear theory
- Skew-spectra: a generalization to spin-
- Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
- About One-point Statistics of the Ratio of Two Fourier-transformed Cosmic Fields and an Application
- Incorporating curved geometry in cosmological simulations