FORGE -- the f(R) gravity cosmic emulator project I: Introduction and matter power spectrum emulator
arXiv:2109.04984 · doi:10.1093/mnras/stac1091
Abstract
We present a large suite of cosmological simulations, the FORGE (F-of-R Gravity Emulator) simulation suite, which is designed to build accurate emulators for cosmological observables in galaxy clustering, weak gravitational lensing and galaxy clusters, for the gravity model. The total of 200 simulations explore the cosmological parameter space around the Planck(2018) cosmology with a Latin hypercube, for 50 combinations of , , and with all other parameters fixed. For each parameter combination, or node, we ran four independent simulations, one pair using particles in simulation boxes to cover small scales, and another pair using simulation particles in boxes for larger scales. Each pair of initial conditions are selected such that sample variance on large scales is minimised on average. In this work we present an accurate emulator for the matter power spectrum in gravity trained on FORGE. We have verified, using the cross-validation technique, that the emulator accuracy is better than for the majority of nodes, particularly around the center of the explored parameter space, up to scales of . We have also checked the power spectrum emulator against simulations which are not part of our training set and found excellent agreement. Due to its high accuracy on small scales, the FORGE matter power spectrum emulator is well suited for weak lensing analysis and can play a key tool in constraining gravity using current and future observational data.
arXiv comment15 pages, FORGE emulator code publicly available from https://bitbucket.org/arnoldcn/forge_emulator/
References in corpus (91)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Measurements of Omega and Lambda from 42 High-Redshift Supernovae
- Dynamics of dark energy
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results
- Simulating the joint evolution of quasars, galaxies and their large-scale distribution
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- f(R) Theories Of Gravity
- The Confrontation between General Relativity and Experiment
- f(R) theories
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- 4D Gravity on a Brane in 5D Minkowski Space
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- E pur si muove: Galiliean-invariant cosmological hydrodynamical simulations on a moving mesh
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Cosmological Hydrodynamics with Adaptive Mesh Refinement: a new high resolution code called RAMSES
- First results from the IllustrisTNG simulations: matter and galaxy clustering
- First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Cosmological Implications from two Decades of Spectroscopic Surveys at the Apache Point observatory
- Revising the Halofit Model for the Nonlinear Matter Power Spectrum
- Chandra Cluster Cosmology Project III: Cosmological Parameter Constraints
- First Results from the TNG50 Simulation: Galactic outflows driven by supernovae and black hole feedback
- The WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 9 Spectroscopic Galaxy Sample
- KiDS-1000 Cosmology: Cosmic shear constraints and comparison between two point statistics
- Cosmological Tests of Modified Gravity
- A test of the nature of cosmic acceleration using galaxy redshift distortions
- Transients from Initial Conditions in Cosmological Simulations
- CFHTLenS tomographic weak lensing cosmological parameter constraints: Mitigating the impact of intrinsic galaxy alignments
- The Atacama Cosmology Telescope: DR4 Maps and Cosmological Parameters
- Planck 2013 results. XX. Cosmology from Sunyaev-Zeldovich cluster counts
- Evolution of structure in cold dark matter universes
- The 6dF Galaxy Survey: z \approx 0 measurement of the growth rate and sigma_8
- The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9
- Scaling relations for galaxy clusters in the Millennium-XXL simulation
- The Arepo public code release
- Cluster Cosmology Constraints from the 2500 deg SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope
- Evading Equivalence Principle Violations, Cosmological and other Experimental Constraints in Scalar Field Theories with a Strong Coupling to Matter
- Solving Large Scale Structure in Ten Easy Steps with COLA
- The Coyote Universe I: Precision Determination of the Nonlinear Matter Power Spectrum
- Weighing the Giants IV: Cosmology and Neutrino Mass
- Constraints on Cosmology from the Cosmic Microwave Background Power Spectrum of the 2500 SPT-SZ Survey
- Cosmological constraints from cosmic shear two-point correlation functions with HSC survey first-year data
- Cosmological Constraints from Galaxy Clusters in the 2500 square-degree SPT-SZ Survey
- Cosmology and Astrophysics from Relaxed Galaxy Clusters II: Cosmological Constraints
- ECOSMOG: An Efficient Code for Simulating Modified Gravity
- 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 2dF Galaxy Redshift Survey: Spherical Harmonics analysis of fluctuations in the final catalogue
- FastPM: a new scheme for fast simulations of dark matter and halos
- Dark Quest. I. Fast and Accurate Emulation of Halo Clustering Statistics and Its Application to Galaxy Clustering
- The VIMOS Public Extragalactic Redshift Survey (VIPERS): The growth of structures at from redshift-space distortions in the clustering of the PDR-2 final sample
- Cosmological -body simulations with suppressed variance
- Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
- Cosmological Constraints from Strong Gravitational Lensing in Galaxy Clusters
- Modified Gravity-GADGET: A new code for cosmological hydrodynamical simulations of modified gravity models
- Cosmological Tests of Gravity
- The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR14 quasar sample: measurement of the growth rate of structure from the anisotropic correlation function between redshift 0.8 and 2.2
- High Performance P3M N-body code: CUBEP3M
- Modified Gravity N-body Code Comparison Project
- One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
- The Aemulus Project I: Numerical Simulations for Precision Cosmology
- The nonlinear matter and velocity power spectra in f(R) gravity
- An accurate tool for the fast generation of dark matter halo catalogs
- The Aemulus Project III: Emulation of the Galaxy Correlation Function
- Cosmic Degeneracies I: Joint N-body Simulations of Modified Gravity and Massive Neutrinos
- The Aemulus Project II: Emulating the Halo Mass Function
- ISIS: a new N-body cosmological code with scalar fields based on RAMSES. Code presentation and application to the shapes of clusters
- MassiveNuS: Cosmological Massive Neutrino Simulations
- On the road to percent accuracy: nonlinear reaction of the matter power spectrum to dark energy and modified gravity
- Testing chameleon gravity with the Coma cluster
- Exploring Vainshtein mechanism on adaptively refined meshes
- Cosmic Emulation: Fast Predictions for the Galaxy Power Spectrum
- Cosmic Calibration
- The Novel Probes Project -- Tests of Gravity on Astrophysical Scales
- Cosmic Shear Cosmology Beyond 2-Point Statistics: A Combined Peak Count and Correlation Function Analysis of DES-Y1
- Dark matter statistics for large galaxy catalogs: power spectra and covariance matrices
- Structure Formation by Fifth Force I: N-Body vs. Linear Simulations
- Large-Scale Structure in Brane-Induced Gravity II. Numerical Simulations
- On the road to percent accuracy IV: ReACT -- computing the non-linear power spectrum beyond CDM
- Emulators for the non-linear matter power spectrum beyond CDM
- Cosmic Shear Covariance Matrix in CDM: Cosmology Matters
- On the road to percent accuracy II: calibration of the non-linear matter power spectrum for arbitrary cosmologies
- Realistic simulations of galaxy formation in f(R) modified gravity
- Matter Power Spectrum Emulator for f(R) Modified Gravity Cosmologies
- Speeding up -body simulations of modified gravity: Chameleon screening models
- PkANN - II. A non-linear matter power spectrum interpolator developed using artificial neural networks
- The modified gravity lightcone simulation project I: Statistics of matter and halo distributions
- Constraining cosmology with weak lensing voids
- Galaxy formation in the brane world I: overview and first results
- Discrete spectrum Radiation from a charged particle moving in a medium with Maxwell fish eye refraction index profile
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- Large-scale dark matter simulations
- Testing Screened Modified Gravity
- Fast and accurate predictions of the nonlinear matter power spectrum for general models of Dark Energy and Modified Gravity
- : Fast, approximate simulations of structure formation in Horndeski gravity
- CSST Cosmological Emulator I: Matter Power Spectrum Emulation with one percent accuracy to k = 10 h/Mpc
- Enabling matter power spectrum emulation in beyond-CDM cosmologies with COLA
- The e-MANTIS emulator: fast predictions of the non-linear matter power spectrum in CDM cosmology
- Cosmological Probes of Structure Growth and Tests of Gravity
- Sesame: A power spectrum emulator pipeline for beyond-CDM models
- Constraining f(R) gravity with cross-correlation of galaxies and cosmic microwave background lensing
- Euclid preparation. Modelling spectroscopic clustering on mildly nonlinear scales in beyond-CDM models
- Improved analytical modeling of the non-linear power spectrum in modified gravity cosmologies
- Cosmological Tests of Gravity: A Future Perspective
- Revisiting Vainshtein Screening for fast N-body simulations
- FREmu: Power Spectrum Emulator for Gravity
- A field-level emulator for modified gravity
- Euclid preparation LXXI. Simulations and nonlinearities beyond CDM. 3. Constraints on models from the photometric primary probes
- Testing modified gravity scenarios with direct peculiar velocities
- Cosmological gravity on all scales III: non-linear matter power spectrum in phenomenological modified gravity
- Euclid preparation. Simulations and nonlinearities beyond CDM. 1. Numerical methods and validation
- MF-Box: Multi-fidelity and multi-scale emulation for the matter power spectrum
- Fast simulation mapping: from standard to modified gravity cosmologies using the bias assignment method
- Euclid: Constraints on f(R) cosmologies from the spectroscopic and photometric primary probes
- Power Spectrum Emulators from Neural Networks and Tree-Based Methods
- Probing gravity with non-linear clustering in redshift space
- Marked statistics across the cosmic web: Environmental dependent clustering in modified gravity simulations
- Cosmological gravity on all scales V: MCMC forecasts combining large scale structure and CMB lensing for binned phenomenological modified gravity