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Open AccessJournal ArticleDOI

Lattice loop quantum cosmology: scalar perturbations

Edward Wilson-Ewing
- 10 Oct 2012 - 
- Vol. 29, Iss: 21, pp 215013
TLDR
In this article, the scalar modes of linear perturbations in loop quantum cosmology were studied on a lattice where each cell is taken to be homogeneous and isotropic and can be quantized via the standard homogeneous loop physics techniques.
Abstract
We study the scalar modes of linear perturbations in loop quantum cosmology. This is done on a lattice where each cell is taken to be homogeneous and isotropic and can be quantized via the standard homogeneous loop quantum cosmology techniques. The appropriate interactions between nearby cells are included in the Hamiltonian in order to obtain the correct physics. It is shown that the quantum theory is anomaly free: the scalar and diffeomorphism constraint operators weakly commute with the Hamiltonian. Finally, the effective theory encoding the leading order quantum gravity corrections is derived and is shown to give the same holonomy-corrected effective equations that have been obtained in previous studies. Communicated by P R L V Moniz.

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Citations
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Homogeneous cosmologies as group field theory condensates

TL;DR: In this paper, the authors give a general procedure for constructing states that describe macroscopic, spatially homogeneous universes, which are close to coherent states used in the description of Bose-Einstein condensates.
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The matter bounce scenario in loop quantum cosmology

TL;DR: In this article, the authors considered the scale-invariance of scalar perturbations by a scalar field whose equation of state is P = −ρ, where is a small positive number.
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Emergent Friedmann dynamics with a quantum bounce from quantum gravity condensates

TL;DR: In this article, the authors studied the hydrodynamics of simple condensate states of a group field theory model for quantum gravity coupled to a massless scalar field and reduced to its isotropic sector.
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Non-singular bounce scenarios in loop quantum cosmology and the effective field description

TL;DR: In this article, the authors compare the dynamics in loop quantum cosmology and in a non-singular bouncing effective field model with a nonstandard kinetic term at both the background and perturbative levels.
Journal ArticleDOI

Detailed analysis of the predictions of loop quantum cosmology for the primordial power spectra

Ivan Agullo, +1 more
- 18 Sep 2015 - 
TL;DR: In this article, the authors provide an exhaustive numerical exploration of the predictions of loop quantum cosmology with a postbounce phase of inflation for the primordial power spectrum of scalar and tensor perturbations.
References
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Book

Theory of Cosmological Perturbations

TL;DR: In this paper, the authors present in a manifestly gauge-invariant form the theory of classical linear gravitational perturbations in part I, and a quantum theory of cosmological perturbation in part II.
Journal ArticleDOI

Quantum Nature of the Big Bang: Improved dynamics

TL;DR: In this article, an improved Hamiltonian constraint operator is introduced in loop quantum cosmology for the isotropic model with a massless scalar field and the big bang is replaced by a quantum bounce.
Journal ArticleDOI

Loop Quantum Cosmology: A Status Report

TL;DR: Loop quantum cosmology (LQC) as mentioned in this paper is the result of applying principles of loop quantum gravity to cosmological settings, where quantum geometry creates a brand new repulsive force which is totally negligible at low spacetime curvature but rises very rapidly in the Planck regime, overwhelming the classical gravitational attraction.
Journal ArticleDOI

A New approach to the evolution of cosmological perturbations on large scales

TL;DR: In this article, the evolution of linear perturbations about a Friedmann-Robertson-Walker background metric, using only the local conservation of energy momentum, has been discussed, and it has been shown that on sufficiently large scales the curvature perturbation on spatial hypersurfaces of uniform density is conserved when the non-adiabatic pressure is negligible.
Journal ArticleDOI

Loop Quantum Cosmology

TL;DR: In this paper, an application of loop quantum cosmology to homogeneous systems, which removes classical singularities, is presented, where the main effects are introduced into effective classical equations, which allow one to avoid the interpretational problems of quantum theory.
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