The BOSS bispectrum analysis at one loop from the Effective Field Theory of Large-Scale Structure
arXiv:2206.08327 · doi:10.1088/1475-7516/2024/05/059
Abstract
We analyze the BOSS power spectrum monopole and quadrupole, and the bispectrum monopole and quadrupole data, using the predictions from the Effective Field Theory of Large-Scale Structure (EFTofLSS). Specifically, we use the one loop prediction for the power spectrum and the bispectrum monopole, and the tree level for the bispectrum quadrupole. After validating our pipeline against numerical simulations as well as checking for several internal consistencies, we apply it to the observational data. We find that analyzing the bispectrum monopole to higher wavenumbers thanks to the one-loop prediction, as well as the addition of the tree-level quadrupole, significantly reduces the error bars with respect to our original analysis of the power spectrum at one loop and bispectrum monopole at tree level. After fixing the spectral tilt to Planck preferred value and using a Big Bang Nucleosynthesis prior, we measure , , and to about , , and , at CL, respectively. This represents an error bar reduction with respect to the power spectrum-only analysis of about , , and respectively. Remarkably, the results are compatible with the ones obtained with a power-spectrum-only analysis, showing the power of the EFTofLSS in simultaneously predicting several observables. We find no tension with Planck.
JCAP version, 23+18 pages, 6 figures, 5 tables
References in corpus (108)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics Beyond LambdaCDM
- Tensions between the Early and the Late Universe
- Power Spectrum Analysis of Three-Dimensional Redshift Surveys
- Cosmology and fundamental physics with the Euclid satellite
- Why your model parameter confidences might be too optimistic -- unbiased estimation of the inverse covariance matrix
- The imprints of primordial non-gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects
- The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch
- The primordial density perturbation in the curvaton scenario
- Cosmological Non-Linearities as an Effective Fluid
- The Effective Field Theory of Cosmological Large Scale Structures
- The shape of non-Gaussianities
- Constraints on local primordial non-Gaussianity from large scale structure
- The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
- Cosmological Parameters from the BOSS Galaxy Power Spectrum
- Non-Gaussianities in Single Field Inflation and their Optimal Limits from the WMAP 5-year Data
- Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
- The DESI Experiment, a whitepaper for Snowmass 2013
- Limits on non-Gaussianities from WMAP data
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the power spectrum and bispectrum of the DR12 BOSS galaxies
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the BOSS Final Data Release
- Non-Linear Evolution of the Bispectrum of Cosmological Perturbations
- The Bispectrum as a Signature of Gravitational Instability in Redshift-Space
- Non-Gaussianity in multi-field inflation
- nbodykit: an open-source, massively parallel toolkit for large-scale structure
- Non-Gaussianities in models with a varying inflaton decay rate
- The IR-resummed Effective Field Theory of Large Scale Structures
- Constraining Early Dark Energy with Large-Scale Structure
- The Effective Field Theory of Multifield Inflation
- Accurate Estimators of Correlation Functions in Fourier Space
- The power spectrum and bispectrum of SDSS DR11 BOSS galaxies I: bias and gravity
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: RSD measurement from the LOS-dependent power spectrum of DR12 BOSS galaxies
- Equivalence Principle and the Baryon Acoustic Peak
- Non-linear perturbation theory extension of the Boltzmann code CLASS
- Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0
- Fast Estimators for Redshift-Space Clustering
- Bias in the Effective Field Theory of Large Scale Structures
- The Lagrangian-space Effective Field Theory of Large Scale Structures
- A Measurement of the Quadrupole Power Spectrum in the Clustering of the 2dF QSO Survey
- Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
- Biased Tracers and Time Evolution
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: measurement of the BAO and growth rate of structure of the emission line galaxy sample from the anisotropic power spectrum between redshift 0.6 and 1.1
- The Effective Field Theory of Large Scale Structures at Two Loops
- 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
- On the Renormalization of the Effective Field Theory of Large Scale Structures
- Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
- Efficient Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
- Limits on CDM from the EFTofLSS with the PyBird code
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- Measuring line-of-sight dependent Fourier-space clustering using FFTs
- Infrared Resummation for Biased Tracers in Redshift Space
- The Hubble Tension in Light of the Full-Shape Analysis of Large-Scale Structure Data
- Cosmological parameters from large scale structure - geometric versus shape information
- Redshift-Space Distortions in Lagrangian Perturbation Theory
- The Effective Field Theory of Large Scale Structure at Two Loops: the apparent scale dependence of the speed of sound
- Detectability of the effect of Inflationary non-Gaussianity on halo bias
- Constraints on Multi-Field Inflation from the BOSS Galaxy Survey
- A Consistent Effective Theory of Long-Wavelength Cosmological Perturbations
- Halo Clustering with Non-Local Non-Gaussianity
- Constraints on Single-Field Inflation from the BOSS Galaxy Survey
- 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
- Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
- The 2-loop matter power spectrum and the IR-safe integrand
- On the Velocity in the Effective Field Theory of Large Scale Structures
- Precision Comparison of the Power Spectrum in the EFTofLSS with Simulations
- BOSS Correlation Function Analysis from the Effective Field Theory of Large-Scale Structure
- On the EFT of Large Scale Structures in Redshift Space
- A complete FFT-based decomposition formalism for the redshift-space bispectrum
- Interpreting measurements of the anisotropic galaxy power spectrum
- Effective Theory of Large-Scale Structure with Primordial Non-Gaussianity
- Unified galaxy power spectrum measurements from 6dFGS, BOSS, and eBOSS
- New Early Dark Energy is compatible with current LSS data
- 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
- Integral constraints in spectroscopic surveys
- Redshift Space Distortions in the Effective Field Theory of Large Scale Structures
- Systematic Renormalization of the Effective Theory of Large Scale Structure
- The Trispectrum in the Effective Field Theory of Large Scale Structure
- Perturbation theory approach to predict the covariance matrices of the galaxy power spectrum and bispectrum in redshift space
- Testing one-loop galaxy bias: joint analysis of power spectrum and bispectrum
- 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
- The Effective Field Theory of Large Scale Structure at Three Loops
- Towards Precision Constraints on Gravity with the Effective Field Theory of Large-Scale Structure
- Very Massive Tracers and Higher Derivative Biases
- 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
- The Effective Field Theory of Large-Scale Structure in the presence of Massive Neutrinos
- Biased Tracers in Redshift Space in the EFTofLSS with exact time dependence
- Tree-Level Bispectrum in the Effective Field Theory of Large-Scale Structure extended to Massive Neutrinos
- On the reach of perturbative methods for dark matter density fields
- 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
- The Halo Bispectrum Multipoles in Redshift Space
- Towards a self-consistent analysis of the anisotropic galaxy two- and three-point correlation functions on large scales: application to mock galaxy catalogues
- Optimal Weighting Scheme in Redshift-space Power Spectrum Analysis and a Prospect for Measuring the Cosmic Equation of State
- Bispectrum-window convolution via Hankel transform
- Principal Shapes and Squeezed Limits in the Effective Field Theory of Large Scale Structure
- Limits on Clustering and Smooth Quintessence from the EFTofLSS
- Taming redshift-space distortion effects in the EFTofLSS and its application to data
Cited by in corpus (24)
- The CosmoVerse White Paper: Addressing observational tensions in cosmology with systematics and fundamental physics
- How much information can be extracted from galaxy clustering at the field level?
- Limits on primordial non-Gaussianities from BOSS galaxy-clustering data
- The one-loop bispectrum of galaxies in redshift space from the Effective Field Theory of Large-Scale Structure
- A Parameter-Masked Mock Data Challenge for Beyond-Two-Point Galaxy Clustering Statistics
- Neutrino masses from large-scale structures: future sensitivity and theory dependence
- Cosmology with Persistent Homology: a Fisher Forecast
- Cosmological Probes of Structure Growth and Tests of Gravity
- From 100 kpc to 10 Gpc: Dark Matter self-interactions before and after DESI
- A multitracer analysis for the eBOSS galaxy sample based on the effective field theory of large-scale structure
- Status of the Tension: A 2026 Review of Probe Discrepancies
- Reducing nuisance prior sensitivity via non-linear reparameterization, with application to EFT analyses of large-scale structure
- A Model for the Redshift-Space Galaxy 4-Point Correlation Function
- Brisk estimator for the angular multipoles of the redshift space bispectrum
- Bispectrum constraints on Primordial non-Gaussianities with the eBOSS DR16 quasars
- Cosmological perturbation theory for large scale structure in phase space
- The Compressed 3D Lyman-Alpha Forest Bispectrum
- A model-independent measurement of the expansion and growth rates from BOSS using the FreePower method
- Catalog-level blinding on the bispectrum for DESI-like galaxy surveys
- Bye-bye, Local-in-matter-density Bias: The Statistics of the Halo Field Are Poorly Determined by the Local Mass Density
- Modelling the covariance matrix for the power spectra before and after the BAO reconstruction
- Cosmology with Persistent Homology: Parameter Inference via Machine Learning
- Three-point intrinsic alignments of galaxies and haloes in the FLAMINGO simulations
- On the range of validity of perturbative models for galaxy clustering and its uncertainty