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Title: EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE

Abstract

We show how the nonlinearity of general relativity generates a characteristic nonGaussian signal in cosmological large-scale structure that we calculate at all perturbative orders in a large-scale limit. Newtonian gravity and general relativity provide complementary theoretical frameworks for modeling large-scale structure in ΛCDM cosmology; a relativistic approach is essential to determine initial conditions, which can then be used in Newtonian simulations studying the nonlinear evolution of the matter density. Most inflationary models in the very early universe predict an almost Gaussian distribution for the primordial metric perturbation, ζ. However, we argue that it is the Ricci curvature of comoving-orthogonal spatial hypersurfaces, R, that drives structure formation at large scales. We show how the nonlinear relation between the spatial curvature, R, and the metric perturbation, ζ, translates into a specific nonGaussian contribution to the initial comoving matter density that we calculate for the simple case of an initially Gaussian ζ. Our analysis shows the nonlinear signature of Einstein's gravity in large-scale structure.

Authors:
; ;  [1]
  1. Institute of Cosmology and Gravitation, University of Portsmouth, Dennis Sciama Building, Burnaby Road, Portsmouth PO1 3FX (United Kingdom)
Publication Date:
OSTI Identifier:
22364938
Resource Type:
Journal Article
Resource Relation:
Journal Name: Astrophysical Journal Letters; Journal Volume: 794; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA)
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; COMPUTERIZED SIMULATION; COSMOLOGY; DENSITY; DISTURBANCES; GAUSS FUNCTION; GENERAL RELATIVITY THEORY; GRAVITATION; METRICS; NONLINEAR PROBLEMS; NONLUMINOUS MATTER; RELATIVISTIC RANGE; UNIVERSE

Citation Formats

Bruni, Marco, Hidalgo, Juan Carlos, and Wands, David, E-mail: hidalgo@fis.unam.mx. EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE. United States: N. p., 2014. Web. doi:10.1088/2041-8205/794/1/L11.
Bruni, Marco, Hidalgo, Juan Carlos, & Wands, David, E-mail: hidalgo@fis.unam.mx. EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE. United States. doi:10.1088/2041-8205/794/1/L11.
Bruni, Marco, Hidalgo, Juan Carlos, and Wands, David, E-mail: hidalgo@fis.unam.mx. 2014. "EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE". United States. doi:10.1088/2041-8205/794/1/L11.
@article{osti_22364938,
title = {EINSTEIN'S SIGNATURE IN COSMOLOGICAL LARGE-SCALE STRUCTURE},
author = {Bruni, Marco and Hidalgo, Juan Carlos and Wands, David, E-mail: hidalgo@fis.unam.mx},
abstractNote = {We show how the nonlinearity of general relativity generates a characteristic nonGaussian signal in cosmological large-scale structure that we calculate at all perturbative orders in a large-scale limit. Newtonian gravity and general relativity provide complementary theoretical frameworks for modeling large-scale structure in ΛCDM cosmology; a relativistic approach is essential to determine initial conditions, which can then be used in Newtonian simulations studying the nonlinear evolution of the matter density. Most inflationary models in the very early universe predict an almost Gaussian distribution for the primordial metric perturbation, ζ. However, we argue that it is the Ricci curvature of comoving-orthogonal spatial hypersurfaces, R, that drives structure formation at large scales. We show how the nonlinear relation between the spatial curvature, R, and the metric perturbation, ζ, translates into a specific nonGaussian contribution to the initial comoving matter density that we calculate for the simple case of an initially Gaussian ζ. Our analysis shows the nonlinear signature of Einstein's gravity in large-scale structure.},
doi = {10.1088/2041-8205/794/1/L11},
journal = {Astrophysical Journal Letters},
number = 1,
volume = 794,
place = {United States},
year = 2014,
month =
}
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