Signatures of the Baryon Acoustic Oscillations on the Convergence Power Spectrum of Weak lensing by Large Scale Structure
arXiv:0812.0521 · doi:10.1016/j.newast.2009.01.007
Abstract
We employ an analytical approach to investigate the signatures of Baryon Acoustic Oscillations (BAOs) on the convergence power spectrum of weak lensing by large scale structure. It is shown that the BAOs wiggles can be found in both of the linear and nonlinear convergence power spectra of weak lensing at about , but they are weaker than that of matter power spectrum. Although the statistical error for LSST are greatly smaller than that of CFHT and SNAP survey especially at about , they are still larger than the their maximum variations of BAOs wiggles. Thus, the detection of BAOs with the ongoing and upcoming surveys such as LSST, CFHT and SNAP survey confront a technical challenge.
arXiv comment12 pages, 6 figures. Accepted for publication in New Astronomy
References in corpus (24)
- Detection of the Baryon Acoustic Peak in the Large-Scale Correlation Function of SDSS Luminous Red Galaxies
- Weak Gravitational Lensing
- Baryonic Features in the Matter Transfer Function
- Weak Gravitational Lensing of the CMB
- Small Scale Cosmological Perturbations: An Analytic Approach
- Nonlinear evolution of cosmological power spectra
- Probing the Universe with Weak Lensing
- Weak Gravitational Lensing by Large-Scale Structure
- Effects of Baryons and Dissipation on the Matter Power Spectrum
- Weak Lensing and Cosmology
- Baryon Acoustic Oscillation Intensity Mapping as a Test of Dark Energy
- Cosmology with Weak Lensing Surveys
- Weak Lensing and Dark Energy
- The influence of baryons on the clustering of matter and weak lensing surveys
- Baryons and weak lensing power spectra
- Effect of Hot Baryons on the Weak-Lensing Shear Power Spectrum
- Detection of dark matter Skewness in the VIRMOS-DESCART survey: Implications for Ω_0
- How accurate is Limber's equation?
- Weak Lensing Reconstruction and Power Spectrum Estimation: Minimum Variance Methods
- Mapping dark matter with cosmic magnification
- Precision measurement of cosmic magnification from 21 cm emitting galaxies
- Signatures of the Baryon Acoustic Oscillations on 21cm Emission Background
- Nonsingular density profiles of dark matter halos and Strong gravitational lensing
- Observing Baryon Oscillations with Cosmic Shear
Cited by in corpus (7)
- Cosmology with cosmic shear observations: a review
- A comparison of structure formation in minimally and non-minimally coupled quintessence models
- Structure formation in cosmologies with oscillating dark energy
- Cusp-core problem and strong gravitational lensing
- Constraining primordial non-Gaussianity with cosmological weak lensing: shear and flexion
- Cosmic shear statistics in cosmologies with non-Gaussian initial conditions
- Primordial density perturbations with running spectral index: impact on non-linear cosmic structures