GridSPT: Grid-based calculation for perturbation theory of large-scale structure
arXiv:1807.04215 · doi:10.1103/PhysRevD.98.103532
Abstract
Perturbation theory (PT) calculation of large-scale structure has been used to interpret the observed non-linear statistics of large-scale structure at the quasi-linear regime. In particular, the so-called standard perturbation theory (SPT) provides a basis for the analytical computation of the higher-order quantities of large-scale structure. Here, we present a novel, grid-based algorithm for the SPT calculation, hence named GridSPT, to generate the higher-order density and velocity fields from a given linear power spectrum. Taking advantage of the Fast Fourier Transform, the GridSPT quickly generates the nonlinear density fields at each order, from which we calculate the statistical quantities such as non-linear power spectrum and bispectrum. Comparing the density fields (to fifth order) from GridSPT with those from the full N-body simulations in the configuration space, we find that GridSPT accurately reproduces the N-body result on large scales. The agreement worsens with smaller smoothing radius, particularly for the under-dense regions where we find that 2LPT (second-order Lagrangian perturbation theory) algorithm performs well.
19 pages, 15 figures
References in corpus (17)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Transients from Initial Conditions in Cosmological Simulations
- The Effective Field Theory of Cosmological Large Scale Structures
- Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
- Nonlinear Evolution of Baryon Acoustic Oscillations
- A critical look at cosmological perturbation theory techniques
- Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations
- Multi-Point Propagators in Cosmological Gravitational Instability
- A Closure Theory for Non-linear Evolution of Cosmological Power Spectra
- The Bispectrum in the Effective Field Theory of Large Scale Structure
- ELUCID - Exploring the Local Universe with reConstructed Initial Density field I: Hamiltonian Markov Chain Monte Carlo Method with Particle Mesh Dynamics
- Linear perturbative theory of the discrete cosmological N-body problem
- Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations
- Simulations of Baryon Acoustic Oscillations I: Growth of Large-Scale Density Fluctuations
- Quantification of discreteness effects in cosmological N-body simulations: II. Evolution up to shell crossing
- New method for initial density reconstruction
- Large-scale structure perturbation theory without losing stream crossing
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