Nonlinear reconstruction
arXiv:1611.09638 · doi:10.1103/PhysRevD.96.123502
Abstract
We present a direct approach to nonparametrically reconstruct the linear density field from an observed nonlinear map. We solve for the unique displacement potential consistent with the nonlinear density and positive definite coordinate transformation using a multigrid algorithm. We show that we recover the linear initial conditions up to the nonlinear scale ( for ) with minimal computational cost. This reconstruction approach generalizes the linear displacement theory to fully nonlinear fields, potentially substantially expanding the baryon acoustic oscillations and redshift space distortions information content of dense large scale structure surveys, including for example SDSS main sample and 21cm intensity mapping initiatives.
7 pages, 7 figures, published version
References in corpus (18)
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: cosmological analysis of the DR12 galaxy sample
- The DESI Experiment Part I: Science,Targeting, and Survey Design
- 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
- Nonlinear Evolution of Baryon Acoustic Oscillations
- On the Robustness of the Acoustic Scale in the Low-Redshift Clustering of Matter
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Anisotropic galaxy clustering in Fourier-space
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Observational systematics and baryon acoustic oscillations in the correlation function
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in Fourier-space
- Canadian Hydrogen Intensity Mapping Experiment (CHIME) Pathfinder
- ELUCID - Exploring the Local Universe with reConstructed Initial Density field I: Hamiltonian Markov Chain Monte Carlo Method with Particle Mesh Dynamics
- Reconstructing Baryon Oscillations: A Lagrangian Theory Perspective
- The clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: On the measurement of growth rate using galaxy correlation functions
- Forecasts on the Dark Energy and Primordial Non-Gaussianity Observations with the Tianlai Cylinder Array
- Super-Sample Signal
- Large-scale tidal effect on redshift-space power spectrum in a finite-volume survey
- Nonlinear -mode clustering in Lagrangian space
- Primordial density and BAO reconstruction
Cited by in corpus (33)
- Infrared Resummation for Biased Tracers in Redshift Space
- Measuring neutrino masses with large-scale structure: Euclid forecast with controlled theoretical error
- Modeling Biased Tracers at the Field Level
- Cosmological Reconstruction From Galaxy Light: Neural Network Based Light-Matter Connection
- An iterative reconstruction of cosmological initial density fields
- Galaxy power-spectrum responses and redshift-space super-sample effect
- Probing Primordial Chirality with Galaxy Spins
- New method for initial density reconstruction
- Observational detection of correlation between galaxy spins and initial conditions
- Baryon acoustic oscillations reconstruction using convolutional neural networks
- Recovering lost 21 cm radial modes via cosmic tidal reconstruction
- Exploring the posterior surface of the large scale structure reconstruction
- Euclid: The search for primordial features
- Nonlinear reconstruction of redshift space distortions
- Reconstructing the baryon acoustic oscillations using biased tracers
- Parity-odd Neutrino Torque Detection
- Application of the iterative reconstruction to simulated galaxy fields
- Iterative removal of redshift space distortions from galaxy clustering
- Biased tracer reconstruction with halo mass information
- Understanding the Reconstruction of the Biased Tracer
- BAO Modulation as a Probe of Compensated Isocurvature Perturbations
- The Phase of the BAO on Observable Scales
- Measuring dark matter-neutrino relative velocity on cosmological scales
- Nonlinear reconstruction of features in the primordial power spectrum from large-scale structure
- Modeling iterative reconstruction and displacement field in the large scale structure
- Measuring the BAO peak position with different galaxy selections
- Reconstruction with velocities
- Nonlinear Reconstruction of the Velocity Field
- Mind the gap: the power of combining photometric surveys with intensity mapping
- Lagrangian displacement field estimators in cosmology
- Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
- Dipole Distortions in the Intergalactic Medium
- Searching optimal scales for reconstructing cosmological initial conditions using convolutional neural networks