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Large-Scale Structure Observables in General Relativity

TLDR
In this article, the authors provide covariant and gauge-invariant expressions of several key observables of the large-scale structure of the universe in a general relativistic context.
Abstract
We review recent studies that rigorously define several key observables of the large-scale structure of the Universe in a general relativistic context. Specifically, we consider (i) redshift perturbation of cosmic clock events; (ii) distortion of cosmic rulers, including weak lensing shear and magnification; and (iii) observed number density of tracers of the large-scale structure. We provide covariant and gauge-invariant expressions of these observables. Our expressions are given for a linearly perturbed flat Friedmann–Robertson–Walker metric including scalar, vector, and tensor metric perturbations. While we restrict ourselves to linear order in perturbation theory, the approach can be straightforwardly generalized to higher order.

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Large-scale galaxy bias

TL;DR: In this paper, the authors present a comprehensive overview of galaxy bias, that is, the statistical relation between the distribution of galaxies and matter, which forms the basis of the rigorous perturbative description of galaxy clustering, under the assumptions of General Relativity and Gaussian, adiabatic initial conditions.
Journal ArticleDOI

Large-Scale Galaxy Bias

TL;DR: In this article, a comprehensive overview of galaxy bias is presented, that is, the statistical relation between the distribution of galaxies and matter, under the assumptions of General Relativity and Gaussian, adiabatic initial conditions.
Journal ArticleDOI

General relativistic weak-field limit and Newtonian N-body simulations

TL;DR: In this paper, the weak-field limit of general relativity has been interpreted in terms of the weak field limit of the Newtonian motion gauge, allowing the inclusion of radiation perturbations and the non-linear evolution of matter.
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Gauge Dependence of Gravitational Waves Generated from Scalar Perturbations

TL;DR: In this paper, it was shown that the induced tensor modes dominate over the linearly evolved primordial gravitational wave amplitude for the linear scalar-type cosmological perturbation.
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How Gaussian can our Universe be

TL;DR: In this article, the authors present an 18-page, 2.26-figures, 2-figure book with references added and minor typos corrected, including minor errors.
References
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Journal ArticleDOI

Planck 2013 results. XVI. Cosmological parameters

Peter A. R. Ade, +327 more
TL;DR: In this paper, the authors present the first cosmological results based on Planck measurements of the cosmic microwave background (CMB) temperature and lensing-potential power spectra, which are extremely well described by the standard spatially-flat six-parameter ΛCDM cosmology with a power-law spectrum of adiabatic scalar perturbations.
Journal ArticleDOI

Planck 2013 results. XVI. Cosmological parameters

Peter A. R. Ade, +262 more
TL;DR: In this paper, the authors present the first results based on Planck measurements of the CMB temperature and lensing-potential power spectra, which are extremely well described by the standard spatially-flat six-parameter LCDM cosmology.
Journal ArticleDOI

Detection of the baryon acoustic peak in the large-scale correlation function of SDSS luminous red galaxies

Daniel J. Eisenstein, +51 more
TL;DR: In this paper, a large-scale correlation function measured from a spectroscopic sample of 46,748 luminous red galaxies from the Sloan Digital Sky Survey is presented, which demonstrates the linear growth of structure by gravitational instability between z ≈ 1000 and the present and confirms a firm prediction of the standard cosmological theory.
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