Biased Tracers of Two Fluids in the Lagrangian Picture
arXiv:1903.00437 · doi:10.1088/1475-7516/2019/06/006
Abstract
We explore Lagrangian perturbation theory (LPT) for biased tracers in the presence of two fluids, focusing on the case of cold dark matter (CDM) and baryons. The presence of two fluids induces corrections to the Lagrangian bias expansion and tracer advection, both of which we formulate as expansions in the three linear modes of the Lagrangian equations of motion. We compute the linear-order two-fluid corrections in the Zeldovich approximation, finding that modifications to the bias expansion and tracer advection both enter as percent-level corrections over a large range of wavenumbers at low redshift and draw parallels with the Eulerian formalism. We then discuss nonlinear corrections in the two-fluid picture, and calculate contributions from the relative velocity effect () at one loop order. Finally, we conduct an exploratory Fisher analysis to assess the impact of two-fluid corrections on baryon acoustic oscillations (BAO) measurements, finding that while modest values of the relative bias parameters can introduce systematic biases in the measured BAO scale of up to , fitting for these effects as additional parameters increases the error bar by less than across a wide range of bias values.
arXiv comment31 pages, 11 figures. Revised to match version accepted by JCAP
References in corpus (60)
- Efficient Computation of CMB anisotropies in closed FRW models
- The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes
- Large-Scale Structure of the Universe and Cosmological Perturbation Theory
- Observational Probes of Cosmic Acceleration
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- Cosmology and Fundamental Physics with the Euclid Satellite
- Large-Scale Galaxy Bias
- Cosmological Non-Linearities as an Effective Fluid
- The Effective Field Theory of Cosmological Large Scale Structures
- Improving Cosmological Distance Measurements by Reconstruction of the Baryon Acoustic Peak
- Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
- Relative velocity of dark matter and baryonic fluids and the formation of the first structures
- Measuring cosmological parameters with galaxy surveys
- Nonlinear perturbation theory with halo bias and redshift-space distortions via the Lagrangian picture
- Convolution Lagrangian perturbation theory for biased tracers
- Bias in the Effective Field Theory of Large Scale Structures
- The Lagrangian-space Effective Field Theory of Large Scale Structures
- Cosmology with massive neutrinos II: on the universality of the halo mass function and bias
- DEMNUni: The clustering of large-scale structures in the presence of massive neutrinos
- A Lagrangian effective field theory
- The bias field of dark matter haloes
- Reconstructing Baryon Oscillations: A Lagrangian Theory Perspective
- Modeling scale-dependent bias on the baryonic acoustic scale with the statistics of peaks of Gaussian random fields
- Perturbation theory, effective field theory, and oscillations in the power spectrum
- The Shift of the Baryon Acoustic Oscillation Scale: A Simple Physical Picture
- Modeling Biased Tracers at the Field Level
- The Zeldovich approximation
- Calibrating the Baryon Oscillation Ruler for Matter and Halos
- Large-scale BAO signatures of the smallest galaxies
- Probing dark energy with the shear-ratio geometric test
- Reconstructing baryon oscillations
- Analytic Prediction of Baryonic Effects from the EFT of Large Scale Structures
- Nonlinear power spectrum in the presence of massive neutrinos: perturbation theory approach, galaxy bias and parameter forecasts
- The Gaussian streaming model and Lagrangian effective field theory
- Halo bias in mixed dark matter cosmologies
- Reconstruction within the Zeldovich approximation
- Massive Neutrinos in Cosmology: Analytic Solutions and Fluid Approximation
- On the IR-Resummation in the EFTofLSS
- Structure formation with massive neutrinos: going beyond linear theory
- The effect of relative velocity and density perturbations between baryons and dark matter on the clustering of galaxies
- Scale-dependent bias in the BAO-scale intergalactic neutral hydrogen
- On the effect of the ionising background on the Lyα forest autocorrelation function
- Halo bias in Lagrangian Space: Estimators and theoretical predictions
- Supersonic Relative Velocity Effect on the Baryonic Acoustic Oscillation Measurements
- Streaming velocities and the baryon-acoustic oscillation scale
- Cosmological perturbation theory for baryons and dark matter I: one-loop corrections in the RPT framework
- The Effective Field Theory of Large-Scale Structure in the presence of Massive Neutrinos
- Efficient Computation of Galaxy Bias with Neutrinos and Other Relics
- Velocity bias in the distribution of dark matter halos
- Power spectra in the eikonal approximation with adiabatic and non-adiabatic modes
- Constraining the Baryon-Dark Matter Relative Velocity with the Large-Scale 3-Point Correlation Function of the SDSS BOSS DR12 CMASS Galaxies
- WFIRST Science Investigation Team "Cosmology with the High Latitude Survey" Annual Report 2017
- The Impact of Wrong Assumptions in BAO Reconstruction
- Excursion set peaks: the role of shear
- Constraining the relative velocity effect using the Baryon Oscillation Spectroscopic Survey
- Nonlinear Behavior of Baryon Acoustic Oscillations from the Zel'dovich Approximation Using a Non-Fourier Perturbation Approach
- Imprints of Reionization in Galaxy Clustering
- Lagrangian space consistency relation for large scale structure
- A new scale in the bias expansion
- Estimates for the impact of Ultraviolet Background fluctuations on galaxy clustering measurements
Cited by in corpus (25)
- A new analysis of galaxy 2-point functions in the BOSS survey, including full-shape information and post-reconstruction BAO
- Large-scale dark matter simulations
- Redshift-Space Distortions in Lagrangian Perturbation Theory
- Simulations and symmetries
- Higher-order initial conditions for mixed baryon-CDM simulations
- Unveiling dark fifth forces with linear cosmology
- Constraining primordial non-Gaussianity using two galaxy surveys and CMB lensing
- Baryonic effects on the matter bispectrum
- Baryon Acoustic Oscillation Theory and Modelling Systematics for the DESI 2024 results
- The Reconstructed Power Spectrum in the Zeldovich Approximation
- Redshift-space streaming velocity effects on the Lyman- forest baryon acoustic oscillation scale
- Baryon-CDM isocurvature galaxy bias with IllustrisTNG
- Cosmological perturbations for two cold fluids in CDM
- Unveiling dark forces with measurements of the Large Scale Structure of the Universe
- The Ly forest flux correlation function: a perturbation theory perspective
- Cosmological Vlasov-Poisson equations for dark matter: Recent developments and connections to selected plasma problems
- Baryonic effects on CMB lensing and neutrino mass constraints
- Avoiding baryonic feedback effects on neutrino mass measurements from CMB lensing
- An Analytic Hybrid Halo + Perturbation Theory Model for Small-scale Correlators: Baryons, Halos, and Galaxies
- Optical depth to reionization from perturbative 21cm clustering
- Measuring dark matter-neutrino relative velocity on cosmological scales
- New Interpretations of the Cosmological Preference for a Negative Neutrino Mass
- The Effective Field Theory of Large Scale Structure for Mixed Dark Matter Scenarios
- Cosmic voids and BAO with relative baryon-CDM perturbations
- Dark Matter Recoupling