Nonlinear Effects in the Amplitude of Cosmological Density Fluctuations
arXiv:0901.0697 · doi:10.1088/1475-7516/2010/02/021
Abstract
The amplitude of cosmological density fluctuations, sigma_8, has been studied and estimated by analysing many cosmological observations. The values of the estimates vary considerably between the various probes. However, different estimators probe the value of sigma_8 in different cosmological scales and do not take into account the nonlinear evolution of the parameter at late times. We show that estimates of the amplitude of cosmological density fluctuations derived from cosmic flows are systematically higher than those inferred at early epochs from the CMB because of nonlinear evolution at later times. We discuss the past and future evolution of linear and nonlinear perturbations, derive corrections to the value of sigma_8 and compare amplitudes after accounting for these differences.
9 pages, 4 figures, 1 table. Accepted for publication in JCAP
References in corpus (11)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Chandra Cluster Cosmology Project II: Samples and X-ray Data Reduction
- Consistently Large Cosmic Flows on Scales of 100 Mpc/h: a Challenge for the Standard LCDM Cosmology
- High resolution CMB power spectrum from the complete ACBAR data set
- Cosmological Constraints From the 100 Square Degree Weak Lensing Survey
- SFI++ I: A New I-band Tully-Fisher Template, the Cluster Peculiar Velocity Dispersion and H0
- Cosmic flow from 2MASS redshift survey: The origin of CMB dipole and implications for LCDM cosmology
- SFI++ II: A New I-band Tully-Fisher Catalog, Derivation of Peculiar Velocities and Dataset Properties
- Current Status Of Velocity Field Surveys: A Consistency Check
- Power Spectrum Shape from Peculiar Velocity Data
- Bulk Flow and Shear Moments of the SFI++ Survey
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- The darkness that shaped the void: dark energy and cosmic voids
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- Cosmic flows in the nearby Universe: new peculiar velocities from SNe and cosmological constraints
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- A local measurement of the growth rate from peculiar velocities and galaxy clustering correlations in the 6dF Galaxy Survey
- Encircling the dark: constraining dark energy via cosmic density in spheres
- The homogeneity scale and the growth rate of cosmic structures
- Detected fluctuations in SDSS LRG magnitudes: Bulk flow signature or systematic?
- Galaxy Peculiar Velocities From Large-Scale Supernova Surveys as a Dark Energy Probe
- The Peculiar Velocity Correlation Function
- Measuring the matter fluctuations in the Local Universe with the ALFALFA catalog
- The Planck SZ Cluster Catalog: Expected X-ray Properties
- Anomalous anisotropic cross-correlations between WMAP CMB maps and SDSS galaxy distribution and implications on the dark flow scenario
- The Velocity Field Olympics: Assessing velocity field reconstructions with direct distance tracers
- from peculiar velocities: agreement with Planck for Tully--Fisher and supernovae, tension for the fundamental plane