Simultaneous modelling of matter power spectrum and bispectrum in the presence of baryons
arXiv:2009.14225 · doi:10.1093/mnras/stab699
Abstract
We demonstrate that baryonification algorithms, which displace particles in gravity-only simulations according to physically-motivated prescriptions, can simultaneously capture the impact of baryonic physics on the 2 and 3-point statistics of matter. Specifically, we show that our implementation of a baryonification algorithm jointly fits the changes induced by baryons on the power spectrum and equilateral bispectrum on scales up to k < 5 h/Mpc and redshifts z<2, as measured in six different cosmological hydrodynamical simulations. The accuracy of our fits are typically 1% for the power spectrum, and for the equilateral and squeezed bispectra, which somewhat degrades to 3% for simulations with extreme feedback prescriptions. Our results support the physical assumptions underlying baryonification approaches, and encourage their use in interpreting weak gravitational lensing and other cosmological observables.
arXiv comment14 pages, 15 figures. To be submitted to MNRAS. Comments are welcome
References in corpus (66)
- A Universal Density Profile from Hierarchical Clustering
- The cosmological simulation code GADGET-2
- The EAGLE project: Simulating the evolution and assembly of galaxies and their environments
- Introducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe
- The Average Star Formation Histories of Galaxies in Dark Matter Halos from z=0-8
- 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
- First results from the IllustrisTNG simulations: the galaxy color bimodality
- The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
- Properties of galaxies reproduced by a hydrodynamic simulation
- First results from the IllustrisTNG simulations: A tale of two elements -- chemical evolution of magnesium and europium
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Tensions between the Early and the Late Universe
- H0LiCOW XIII. A 2.4% measurement of from lensed quasars: tension between early and late-Universe probes
- First results from the IllustrisTNG simulations: radio haloes and magnetic fields
- The Hyper Suprime-Cam SSP Survey: Overview and Survey Design
- A model for cosmological simulations of galaxy formation physics
- Euclid Definition Study Report
- Dark Energy Survey Year 1 Results: Cosmological Constraints from Cosmic Shear
- The Illustris simulation: the evolving population of black holes across cosmic time
- Evolution of structure in cold dark matter universes
- The BAHAMAS project: Calibrated hydrodynamical simulations for large-scale structure cosmology
- Scaling relations for galaxy clusters in the Millennium-XXL simulation
- The EAGLE simulations of galaxy formation: public release of halo and galaxy catalogues
- An accurate halo model for fitting non-linear cosmological power spectra and baryonic feedback models
- Systematic Errors in Future Weak Lensing Surveys: Requirements and Prospects for Self-Calibration
- Stellar mass -- halo mass relation and star formation efficiency in high-mass halos
- nbodykit: an open-source, massively parallel toolkit for large-scale structure
- The bispectrum of galaxies from high-redshift galaxy surveys: primordial non-Gaussianity and non-linear galaxy bias
- The Coyote Universe Extended: Precision Emulation of the Matter Power Spectrum
- Accurate Estimators of Correlation Functions in Fourier Space
- A new method to quantify the effects of baryons on the matter power spectrum
- The BACCO Simulation Project: Exploiting the full power of large-scale structure for cosmology
- Cosmological -body simulations with suppressed variance
- Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
- Euclid preparation: II. The EuclidEmulator -- A tool to compute the cosmology dependence of the nonlinear matter power spectrum
- The impact of baryons on the matter power spectrum from the Horizon-AGN cosmological hydrodynamical simulation
- The Bispectrum: From Theory to Observations
- The BAHAMAS project: the CMB--large-scale structure tension and the roles of massive neutrinos and galaxy formation
- Exploring the effects of galaxy formation on matter clustering through a library of simulation power spectra
- J-PAS: The Javalambre-Physics of the Accelerated Universe Astrophysical Survey
- One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
- Effect of baryonic feedback on two- and three-point shear statistics: prospects for detection and improved modelling
- The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
- Accurate estimators of power spectra in N-body simulations
- Modelling the large scale structure of the Universe as a function of cosmology and baryonic physics
- Cosmological parameters from combined second- and third-order aperture mass statistics of cosmic shear
- Baryonic effects for weak lensing. Part I. Power spectrum and covariance matrix
- Cosmological constraints from the CFHTLenS shear measurements using a new, accurate and flexible way of predicting nonlinear mass clustering
- Emulators for the non-linear matter power spectrum beyond CDM
- Optimal capture of non-Gaussianity in weak lensing surveys: power spectrum, bispectrum and halo counts
- Baryonic effects on the matter bispectrum
- How to add massive neutrinos to your CDM simulation -- extending cosmology rescaling algorithms
- The EAGLE simulations of galaxy formation: Public release of particle data
- The Strikingly Similar Relation between Satellite and Central Galaxies and Their Dark Matter Halos Since z=2
- Separate Universe Simulations with IllustrisTNG: baryonic effects on power spectrum responses and higher-order statistics
- 3\%-accurate predictions for the clustering of dark matter, haloes and subhaloes, over a wide range of cosmologies and scales
- k-cut Cosmic Shear: Tunable Power Spectrum Sensitivity to Test Gravity
- Cosmological parameter estimation via iterative emulation of likelihoods
- Preparing for the Cosmic Shear Data Flood: Optimal Data Extraction and Simulation Requirements for Stage IV Dark Energy Experiments
- Rapid simulation rescaling from standard to modified gravity models
- Remapping dark matter halo catalogues between cosmological simulations
- How accurate is it to update the cosmology of your halo catalogues?
- Reconstructing Probability Distributions with Gaussian Processes
- Halo mass and weak galaxy-galaxy lensing profiles in rescaled cosmological -body simulations
- Remapping simulated halo catalogues in redshift space
Cited by in corpus (37)
- The FLAMINGO project: cosmological hydrodynamical simulations for large-scale structure and galaxy cluster surveys
- Large-scale dark matter simulations
- Emulation of baryonic effects on the matter power spectrum and constraints from galaxy cluster data
- DES Y3 cosmic shear down to small scales: constraints on cosmology and baryons
- Calibration of bias and scatter involved in cluster mass measurements using optical weak gravitational lensing
- Euclid: impact of nonlinear prescriptions on cosmological parameter estimation from weak lensing cosmic shear
- Constraining baryonic feedback and cosmology with weak-lensing, X-ray, and kinematic Sunyaev-Zeldovich observations
- Constraining the Baryonic Feedback with Cosmic Shear Using the DES Year-3 Small-Scale Measurements
- Cosmic shear with small scales: DES-Y3, KiDS-1000 and HSC-DR1
- TNG: Effect of Baryonic Processes on Weak Lensing with IllustrisTNG Simulations
- Offset between X-ray and optical centers in clusters of galaxies: connecting eROSITA data and simulations
- The radial acceleration relation in a CDM universe
- The MillenniumTNG Project: Inferring cosmology from galaxy clustering with accelerated N-body scaling and subhalo abundance matching
- From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning
- Consistent and simultaneous modelling of galaxy clustering and galaxy-galaxy lensing with Subhalo Abundance Matching
- Effects of Baryonic Feedback on the Cosmic Web
- Multi-wavelength mock galaxy catalogs of the low-redshift Universe
- Comparing weak lensing peak counts in baryonic correction models to hydrodynamical simulations
- SHAMe-SF: Predicting the clustering of star-forming galaxies with an enhanced abundance matching model
- Galaxy formation physics behind bar formation: A view from cosmological hydrodynamical simulations
- Cosmological feedback from a halo assembly perspective
- Impact of baryonic feedback on HSC Y1 weak lensing non-Gaussian statistics
- Validating the clustering predictions of empirical models with the FLAMINGO simulations
- Baryonification extended to thermal Sunyaev Zeldovich
- How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
- The quasi-adiabatic relaxation of haloes in the IllustrisTNG and EAGLE cosmological simulations
- The halo bispectrum as a sensitive probe of massive neutrinos and baryon physics
- Third-order intrinsic alignment of SDSS BOSS LOWZ galaxies
- Map-level baryonification: unified treatment of weak lensing two-point and higher-order statistics
- The BACCO Simulation Project: A baryonification emulator with Neural Networks
- A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
- Calibrating baryonic effects in cosmic shear with external data in the LSST era
- syren-baryon: Analytic emulators for the impact of baryons on the matter power spectrum
- The evolution of the barred galaxy population in the TNG50 simulation
- FLAMINGO: Galaxy formation and feedback effects on the gas density and velocity fields
- One latent to fit them all: a unified representation of baryonic feedback on matter distribution
- Response approach to the integrated shear 3-point correlation function: the impact of baryonic effects on small scales