Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure

Abstract

The precision of the cosmological data allows us to accurately approximate the predictions for cosmological observables by Taylor expanding up to a low order the dependence on the cosmological parameters around a reference cosmology. By applying this observation to the redshift-space one-loop galaxy power spectrum of the Effective Field Theory of Large-Scale Structure, we analyze the BOSS DR12 data by scanning over all the parameters of $\Lambda$CDM cosmology with massive neutrinos. We impose several sets of priors, the widest of which is just a Big Bang Nucleosynthesis prior on the current fractional energy density of baryons, ${\Omega }_b{h}^2$, and a bound on the sum of neutrino masses to be less than 0.9 eV. In this case we measure the primordial amplitude of the power spectrum, $A_s$, the abundance of matter, ${\Omega }_m$, the Hubble parameter, $H_0$, and the tilt of the primordial power spectrum, $n_s$, to about $19\%$, $5.7\%$, $2.2\%$ and $7.3\%$ respectively, obtaining $\ln (10^{10}{A}_s)=2.91\pm 0.19$, ${\Omega }_m=0.314\pm 0.018$, $H_0=68.7\pm 1.5$ km/(s Mpc) and $n_s=0.979\pm 0.071$ at $68\%$ confidence level. A public code is released with this preprint.

arXiv comment15 + 10 pages, 15 figures. Code publicly available. Removed prior on the tilt, improved presentation and accuracy

References in corpus (48)

• emcee: The MCMC Hammer
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
• The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
• Cosmological Non-Linearities as an Effective Fluid
• The Effective Field Theory of Cosmological Large Scale Structures
• The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
• Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
• The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
• The IR-resummed Effective Field Theory of Large Scale Structures
• Equivalence Principle and the Baryon Acoustic Peak
• Bias in the Effective Field Theory of Large Scale Structures
• The Lagrangian-space Effective Field Theory of Large Scale Structures
• Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
• Biased Tracers and Time Evolution
• Consistent Calibration of the Tip of the Red Giant Branch in the Large Magellanic Cloud on the Hubble Space Telescope Photometric System and a Re-determination of the Hubble Constant
• The Effective Field Theory of Large Scale Structures at Two Loops
• On the Renormalization of the Effective Field Theory of Large Scale Structures
• The Bispectrum in the Effective Field Theory of Large Scale Structure
• The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
• A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
• Galaxy Bias and Primordial Non-Gaussianity
• Cosmological Perturbation Theory Using the FFTLog: Formalism and Connection to QFT Loop Integrals
• The One-Loop Matter Bispectrum in the Effective Field Theory of Large Scale Structures
• The 2-loop matter power spectrum and the IR-safe integrand
• Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
• Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
• On the Velocity in the Effective Field Theory of Large Scale Structures
• On the EFT of Large Scale Structures in Redshift Space
• Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
• The Effect of Fiber Collisions on the Galaxy Power Spectrum Multipole
• Non-Gaussian Covariance of the Matter Power Spectrum in the Effective Field Theory of Large Scale Structure
• On the IR-Resummation in the EFTofLSS
• Cosmological perturbation theory in 1+1 dimensions
• On the reach of perturbative descriptions for dark matter displacement fields
• Systematic Renormalization of the Effective Theory of Large Scale Structure
• On the Statistics of Biased Tracers in the Effective Field Theory of Large Scale Structures
• The Trispectrum in the Effective Field Theory of Large Scale Structure
• Dark Energy and Modified Gravity in the Effective Field Theory of Large-Scale Structure
• An analytic implementation of the IR-resummation for the BAO peak
• Very Massive Tracers and Higher Derivative Biases
• Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
• The EFT of Large Scale Structures at All Redshifts: Analytical Predictions for Lensing
• IR-safe and UV-safe integrands in the EFTofLSS with exact time dependence
• Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
• An effective description of dark matter and dark energy in the mildly non-linear regime
• Efficient exploration of cosmology dependence in the EFT of LSS
• On the Bispectra of Very Massive Tracers in the Effective Field Theory of Large-Scale Structure
• Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure

Cited by in corpus (114)

• In the Realm of the Hubble tension $-$ a Review of Solutions
• Challenges for $\Lambda$CDM: An update
• Early Dark Energy Does Not Restore Cosmological Concordance
• Constraining Early Dark Energy with Large-Scale Structure
• A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
• Early dark energy is not excluded by current large-scale structure data
• Limits on $w$CDM from the EFTofLSS with the PyBird code
• The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
• Early modified gravity in light of the $H_0$ tension and LSS data
• Consistent Modeling of Velocity Statistics and Redshift-Space Distortions in One-Loop Perturbation Theory
• The galaxy power spectrum take on spatial curvature and cosmic concordance
• On the most constraining cosmological neutrino mass bounds
• KiDS-1000 Methodology: Modelling and inference for joint weak gravitational lensing and spectroscopic galaxy clustering analysis
• Cosmological constraints from unWISE and Planck CMB lensing tomography
• Constraints on the curvature of the Universe and dynamical dark energy from the Full-shape and BAO data
• Cosmological constraints from the tomographic cross-correlation of DESI Luminous Red Galaxies and Planck CMB lensing
• BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
• ShapeFit: extracting the power spectrum shape information in galaxy surveys beyond BAO and RSD
• New Early Dark Energy is compatible with current LSS data
• Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations
• Cosmology with the Galaxy Bispectrum Multipoles: Optimal Estimation and Application to BOSS Data
• Arguments against using $h^{-1}\mathrm{Mpc}$ units in observational cosmology
• Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
• Can Conformally Coupled Modified Gravity Solve The Hubble Tension?
• The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
• Primordial Non-Gaussianity from Biased Tracers: Likelihood Analysis of Real-Space Power Spectrum and Bispectrum
• Dark Sector to Restore Cosmological Concordance
• The completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: geometry and growth from the anisotropic void-galaxy correlation function in the luminous red galaxy sample
• H0 tension or T0 tension?
• Updated constraints from the effective field theory analysis of BOSS power spectrum on Early Dark Energy
• Consistency of effective field theory analyses of the BOSS power spectrum
• Symmetry of Cosmological Observables, and a High Hubble Constant as an Indicator of a Mirror World Dark Sector
• Linear cosmological constraints on 2-body decaying dark matter scenarios and the $S_8$ tension
• Optimizing large-scale structure data analysis with the theoretical error likelihood
• Galaxy redshift-space bispectrum: the Importance of Being Anisotropic
• Cosmological constraints without fingers of God
• The clustering of the SDSS-IV extended Baryon Oscillation Spectroscopic Survey DR16 luminous red galaxy and emission line galaxy samples: cosmic distance and structure growth measurements using multiple tracers in configuration space
• The BACCO simulation project: biased tracers in real space
• Constraints on modified gravity from the BOSS galaxy survey
• Biased Tracers in Redshift Space in the EFTofLSS with exact time dependence
• ENCORE: An $\mathcal{O}(N_{\mathrm{g}}^2)$ Estimator for Galaxy $N$-Point Correlation Functions
• Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
• Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
• Fast computation of non-linear power spectrum in cosmologies with massive neutrinos
• The minimally extended Varying Speed of Light (meVSL)
• Determining the Hubble Constant without the Sound Horizon: Perspectives with Future Galaxy Surveys
• Clustering in Massive Neutrino Cosmologies via Eulerian Perturbation Theory
• Small-scale clumping at recombination and the Hubble tension
• The two-mode puzzle: Confronting self-interacting neutrinos with the full shape of the galaxy power spectrum
• Updating non-standard neutrinos properties with Planck-CMB data and full-shape analysis of BOSS and eBOSS galaxies
• Priors on Lagrangian bias parameters from galaxy formation modelling
• Modified gravity and massive neutrinos: constraints from the full shape analysis of BOSS galaxies and forecasts for Stage IV surveys
• Higher-order initial conditions with massive neutrinos
• The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure
• The Reconstruction of Constant Jerk Parameter with $f(R,T)$ Gravity
• Testing signatures of phantom crossing through full-shape galaxy clustering analysis
• Limits on Clustering and Smooth Quintessence from the EFTofLSS
• Minkowski Functionals of SDSS-III BOSS : Hints of Possible Anisotropy in the Density Field?
• Taming redshift-space distortion effects in the EFTofLSS and its application to data
• Decoherence out of fire: Purity loss in expanding and contracting universes
• Redshift space power spectrum beyond Einstein-de Sitter kernels
• The Effective Field Theory of Large-Scale Structure and Multi-tracer
• Reconstruction of an Observationally Constrained $f(R,T)$ gravity model
• BOSS full-shape analysis from the EFTofLSS with exact time dependence
• Cosmological constraints from the cross-correlation of DESI Luminous Red Galaxies with CMB lensing from Planck PR4 and ACT DR6
• Violation of the consistency relations for large-scale structure with dark energy
• A comparison between Shapefit compression and Full-Modelling method with PyBird for DESI 2024 and beyond
• Neutrino mass bounds from confronting an effective model with BOSS Lyman-alpha data
• Modelling galaxy clustering in redshift space with a Lagrangian bias formalism and $N$-body simulations
• Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
• Non-Linear Matter Power Spectrum Modeling in Interacting Dark Energy Cosmologies
• Dark Sectors with Mass Thresholds Face Cosmological Datasets
• An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
• An absolute $\nu$ mass measurement with the DUNE experiment
• Compressed baryon acoustic oscillation analysis is robust to modified-gravity models
• Addressing Cosmological Tensions by Non-Local Gravity
• Neutrino masses from large-scale structures: future sensitivity and theory dependence
• Combined full shape analysis of BOSS galaxies and eBOSS quasars using an iterative emulator
• Cosmology with Persistent Homology: a Fisher Forecast
• Fisher matrix for the one-loop galaxy power spectrum: measuring expansion and growth rates without assuming a cosmological model
• Boltzmann hierarchies for self-interacting warm dark matter scenarios
• Search for the $f(R,T)$ gravity functional form via gaussian processes
• Possible Resolution of the Hubble Tension with Weyl Invariant Gravity
• Baryogenesis through Asymmetric Hawking Radiation from Primordial Black Holes as Dark Matter
• Functors of actions
• Using peculiar velocity surveys to constrain neutrino masses
• Improving precision and accuracy in cosmology with model-independent spectrum and bispectrum
• Direct signatures of the formation time of galaxies
• Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
• Can acoustic and axion-like early dark energy still resolve the Hubble tension?
• The Effective Field Theory and Perturbative Analysis for Log-Density Fields
• The clustering of LRGs in the DECaLS DR8 footprint: distance constraints from baryon acoustic oscillations using photometric redshifts
• CSST Cosmological Emulator III: Hybrid Lagrangian Bias Expansion Emulation of Galaxy Clustering
• Sensitivity of Cosmological Parameter Estimation to Nonlinear Prescription from Galaxy Clustering
• Power spectrum response of large-scale structure in 1D and in 3D: tests of prescriptions for post-collapse dynamics
• Faster cosmological analysis with power spectrum without simulations
• Predictive uncertainty on improved astrophysics recovery from multifield cosmology
• Position-dependent Voronoi probability distribution functions for matter and halos
• A 1% accurate method to include baryonic effects in galaxy-galaxy lensing models
• Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
• Testing the assumptions of the Effective Field Theory of Large-Scale Structure
• Cosmological perturbation theory for large scale structure in phase space
• Baryonic effects in the Effective Field Theory of Large-Scale Structure and an analytic recipe for lensing in CMB-S4
• Cosmology with Persistent Homology: Parameter Inference via Machine Learning
• Probabilistic Lagrangian bias estimators and the cumulant bias expansion
• Gaussian Lagrangian Galaxy Bias
• Perturbation theory challenge for cosmological parameters estimation II.: Matter power spectrum in redshift space
• Parameter inference with non-linear galaxy clustering: accounting for theoretical uncertainties
• Implementing spectra response function approaches for fast calculation of power spectra and bispectra
• Constraining decaying dark matter with BOSS data and the effective field theory of large-scale structures
• The Large Scale Structure Bootstrap: perturbation theory and bias expansion from symmetries
• New tests of dark sector interactions from the full-shape galaxy power spectrum
• Neural Network Acceleration of Large-scale Structure Theory Calculations
• Cosmology with the Redshift-Space Galaxy Bispectrum Monopole at One-Loop Order