The ACCEL2 Project: Precision Measurements of EFT Parameters and BAO Peak Shifts for the Lyman- Forest
arXiv:2412.06892 · doi:10.1103/PhysRevD.111.063524
Abstract
We present precision measurements of the bias parameters of the one-loop power spectrum model of the Lyman-alpha (Lya) forest, derived within the effective field theory of large-scale structure (EFT). We fit our model to the three-dimensional flux power spectrum measured from the ACCEL2 hydrodynamic simulations. The EFT model fits the data with an accuracy of below 2 percent up to a wavenumber of k = 2 h/Mpc. Further, we analytically derive how non-linearities in the three-dimensional clustering of the Lya forest introduce biases in measurements of the Baryon Acoustic Oscillations (BAO) scaling parameters in radial and transverse directions. From our EFT parameter measurements, we obtain a theoretical error budget of -0.2 (-0.3) percent for the radial (transverse) parameters at redshift two. This corresponds to a shift of -0.3 (0.1) percent for the isotropic (anisotropic) distance measurements. We provide an estimate for the shift of the BAO peak for Lya-quasar cross-correlation measurements assuming analytical and simulation-based scaling relations for the non-linear quasar bias parameters resulting in a shift of -0.2 (-0.1) percent for the radial (transverse) dilation parameters, respectively. This analysis emphasizes the robustness of Lya forest BAO measurements to the theory modeling. We provide informative priors and an error budget for measuring the BAO feature -- a key science driver of the currently observing Dark Energy Spectroscopic Instrument (DESI). Our work paves the way for full-shape cosmological analyses of Lya forest data from DESI and upcoming surveys such as the Prime Focus Spectrograph, WEAVE-QSO, and 4MOST.
arXiv comment19 pages, 10 figures
References in corpus (99)
- Planck 2015 results. XIII. Cosmological parameters
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- Large scale bias and the peak background split
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- The 2dF Galaxy Redshift Survey: Power-spectrum analysis of the final dataset and cosmological implications
- Simulating Galaxy Formation with the IllustrisTNG Model
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- Simulating galaxy formation with black hole driven thermal and kinetic feedback
- DESI 2024 VI: Cosmological Constraints from the Measurements of Baryon Acoustic Oscillations
- Cosmological parameter analysis including SDSS Ly-alpha forest and galaxy bias: constraints on the primordial spectrum of fluctuations, neutrino mass, and dark energy
- The SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Overview and Early Data
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- Cosmological Non-Linearities as an Effective Fluid
- Baryon Acoustic Oscillations in the Ly-α forest of BOSS quasars
- New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman- forest data
- Overview of the Instrumentation for the Dark Energy Spectroscopic Instrument
- Nonlinear Evolution of Baryon Acoustic Oscillations
- The Cosmological Analysis of the SDSS/BOSS data from the Effective Field Theory of Large-Scale Structure
- On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
- Cosmological Parameters from the BOSS Galaxy Power Spectrum
- The Lyman-alpha Forest Power Spectrum from the Sloan Digital Sky Survey
- Clustering of dark matter tracers: generalizing bias for the coming era of precision LSS
- The Completed SDSS-IV extended Baryon Oscillation Spectroscopic Survey: Baryon acoustic oscillations with Lyman- forests
- The Physics of the Intergalactic Medium
- The Evolution of the Intergalactic Medium
- The Observed Probability Distribution Function, Power Spectrum, and Correlation Function of the Transmitted Flux in the Lyman-alpha Forest
- 4MOST: Project overview and information for the First Call for Proposals
- Constraining the mass of light bosonic dark matter using SDSS Lyman- forest
- Nyx: A Massively Parallel AMR Code for Computational Cosmology
- Measurement of Baryon Acoustic Oscillations in the Lyman-alpha Forest Fluctuations in BOSS Data Release 9
- DESI 2024 IV: Baryon Acoustic Oscillations from the Lyman Alpha Forest
- Primordial Black Holes as Dark Matter: The Power Spectrum and Evaporation of Early Structures
- Lyman-alpha Constraints on Ultralight Scalar Dark Matter: Implications for the Early and Late Universe
- Toward a Measurement of the Cosmological Geometry at z~2: Predicting Lyman-alpha Forest Correlation in Three Dimensions, and the Potential of Future Data Sets
- The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium
- Can sterile neutrinos be ruled out as warm dark matter candidates?
- The one-dimensional Ly-alpha forest power spectrum from BOSS
- Non-linear perturbation theory extension of the Boltzmann code CLASS
- Lyman-alpha Forests cool Warm Dark Matter
- Time-Sliced Perturbation Theory II: Baryon Acoustic Oscillations and Infrared Resummation
- The Lyman- forest in optically-thin hydrodynamical simulations
- 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
- The Sherwood simulation suite: overview and data comparisons with the Lyman-alpha forest at redshifts 2 < z < 5
- Blinded challenge for precision cosmology with large-scale structure: results from effective field theory for the redshift-space galaxy power spectrum
- New Constraints on IGM Thermal Evolution from the Lyα Forest Power Spectrum
- Dark energy and curvature from a future baryonic acoustic oscillation survey using the Lyman-alpha forest
- Possible evidence for an inverted temperature-density relation in the intergalactic medium from the flux distribution of the Lyman-alpha forest
- Infrared Resummation for Biased Tracers in Redshift Space
- Revealing reionization with the thermal history of the intergalactic medium: new constraints from the Lyman- flux power spectrum
- Perturbation theory, effective field theory, and oscillations in the power spectrum
- The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
- Lyman- forest constraints on Primordial Black Holes as Dark Matter
- Modeling Biased Tracers at the Field Level
- Calibrating the Baryon Oscillation Ruler for Matter and Halos
- The Zeldovich approximation
- Clustering of quasars in SDSS-IV eBOSS : study of potential systematics and bias determination
- Time-Sliced Perturbation Theory for Large Scale Structure I: General Formalism
- The large-scale Quasar-Lyman α Forest Cross-Correlation from BOSS
- A consistent and robust measurement of the thermal state of the IGM at from a large sample of Ly forest spectra: Evidence for late and rapid HeII reionization
- Cubic Halo Bias in Eulerian and Lagrangian Space
- New Constraints on Warm Dark Matter from the Lyman- Forest Power Spectrum
- The Galaxy Power Spectrum and Bispectrum in Redshift Space
- Novel constraints on non-cold (non-thermal) Dark Matter from Lyman- forest data
- The intergalactic medium thermal history at redshift z=1.7--3.2 from the Lyman alpha forest: a comparison of measurements using wavelets and the flux distribution
- The Non-Linear Power Spectrum of the Lyman Alpha Forest
- Cosmological Analysis of Three-Dimensional BOSS Galaxy Clustering and Planck CMB Lensing Cross Correlations via Lagrangian Perturbation Theory
- Cosmological perturbation theory in 1+1 dimensions
- Unveiling Dark Matter free-streaming at the smallest scales with high redshift Lyman-alpha forest
- On Estimating Lyman-alpha Forest Correlations between Multiple Sightlines
- The Lyman- forest as a diagnostic of the nature of the dark matter
- Fewer Mocks and Less Noise: Reducing the Dimensionality of Cosmological Observables with Subspace Projections
- New limits on light dark matter - proton cross section from the cosmic large-scale structure
- Modeling Galaxies in Redshift Space at the Field Level
- Early Structure Formation Constraints on the Ultra-Light Axion in the Post-Inflation Scenario
- Bias, redshift space distortions and primordial nongaussianity of nonlinear transformations: application to Lyman alpha forest
- Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features
- LyaCoLoRe: Synthetic Datasets for Current and Future Lyman- Forest BAO Surveys
- The Dark Energy Spectroscopic Instrument: One-dimensional power spectrum from first Lyman- forest samples with Fast Fourier Transform
- How to estimate the 3D power spectrum of the Lyman- forest
- Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
- Searching for fluctuations in the IGM temperature using the Lyman alpha forest
- Cosmological inference from the EFTofLSS: the eBOSS QSO full-shape analysis
- Cosmology beyond BAO from the 3D distribution of the Lyman- forest
- Cosmological constraints from the power spectrum of eBOSS quasars
- Inferring the Thermal History of the Intergalactic Medium from the Properties of the Hydrogen and Helium Lyman-alpha Forest
- Redshift-space streaming velocity effects on the Lyman- forest baryon acoustic oscillation scale
- Non-linear matter power spectrum from Time Renormalisation Group: efficient computation and comparison with one-loop
- Effect of non-equilibrium ionization on derived physical conditions of the high- intergalactic medium
- The Ly forest flux correlation function: a perturbation theory perspective
- The 3D Lyman- Forest Power Spectrum from eBOSS DR16
- Non-linearities in the Lyman- forest and in its cross-correlation with dark matter halos
- Absorber Model: the Halo-like model for the Lyman-alpha forest
- The ACCEL project: simulating Lyman- forest in large-volume hydrodynamical simulations
- Direct cosmological inference from three-dimensional correlations of the Lyman- forest
- Measurement of the small-scale 3D Lyman- forest power spectrum
- A measurement of the Lyman-beta forest power spectrum and its cross with the Lyman-alpha forest in X-Shooter XQ-100
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- DESI DR2 Results II: Measurements of Baryon Acoustic Oscillations and Cosmological Constraints
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- Cosmology from Planck CMB Lensing and DESI DR1 Quasar Tomography
- The Compressed 3D Lyman-Alpha Forest Bispectrum
- Modeling the Cosmological Lyman- Forest at the Field Level
- Bridging Simulations and EFT: A Hybrid Model of the Lyman-Alpha Forest Field