Cosmological perturbations in teleparallel Loop Quantum Cosmology
Abstract
Cosmological perturbations in Loop Quantum Cosmology (LQC) are usually studied incorporating either holonomy corrections, where the Ashtekar connection is replaced by a suitable sinus function in order to have a welldefined quantum analogue, or inversevolume corrections coming from the eigenvalues of the inversevolume operator. In this paper we will develop an alternative approach to calculate cosmological perturbations in LQC based on the fact that, holonomy corrected LQC in the flat FriedmannLemaîtreRobertsonWalker (FLRW) geometry could be also obtained as a particular case of teleparallel F(T) gravity (teleparallel LQC). The main idea of our approach is to mix the simple bounce provided by holonomy corrections in LQC with the nonsingular perturbation equations given by F(T) gravity, in order to obtain a matter bounce scenario as a viable alternative to slowroll inflation. In our study, we have obtained an scale invariant power spectrum of cosmological perturbations. However, the ratio of tensor to scalar perturbations is of order 1, which does not agree with the current observations. For this reason, we suggest a model where a transition from the matter domination to a quasi de Sitter phase is produced in order to enhance the scalar power spectrum.
 Authors:

 Departament de Matemàtica Aplicada I, Universitat Politècnica de Catalunya, Diagonal 647, 08028 Barcelona (Spain)
 Publication Date:
 OSTI Identifier:
 22369893
 Resource Type:
 Journal Article
 Journal Name:
 Journal of Cosmology and Astroparticle Physics
 Additional Journal Information:
 Journal Volume: 2013; Journal Issue: 11; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 14757516
 Country of Publication:
 United States
 Language:
 English
 Subject:
 71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS; 79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; CORRECTIONS; DE SITTER GROUP; DE SITTER SPACE; EIGENVALUES; GEOMETRY; PERTURBATION THEORY; QUANTUM COSMOLOGY
Citation Formats
Haro, Jaime. Cosmological perturbations in teleparallel Loop Quantum Cosmology. United States: N. p., 2013.
Web. doi:10.1088/14757516/2013/11/068.
Haro, Jaime. Cosmological perturbations in teleparallel Loop Quantum Cosmology. United States. doi:10.1088/14757516/2013/11/068.
Haro, Jaime. Fri .
"Cosmological perturbations in teleparallel Loop Quantum Cosmology". United States. doi:10.1088/14757516/2013/11/068.
@article{osti_22369893,
title = {Cosmological perturbations in teleparallel Loop Quantum Cosmology},
author = {Haro, Jaime},
abstractNote = {Cosmological perturbations in Loop Quantum Cosmology (LQC) are usually studied incorporating either holonomy corrections, where the Ashtekar connection is replaced by a suitable sinus function in order to have a welldefined quantum analogue, or inversevolume corrections coming from the eigenvalues of the inversevolume operator. In this paper we will develop an alternative approach to calculate cosmological perturbations in LQC based on the fact that, holonomy corrected LQC in the flat FriedmannLemaîtreRobertsonWalker (FLRW) geometry could be also obtained as a particular case of teleparallel F(T) gravity (teleparallel LQC). The main idea of our approach is to mix the simple bounce provided by holonomy corrections in LQC with the nonsingular perturbation equations given by F(T) gravity, in order to obtain a matter bounce scenario as a viable alternative to slowroll inflation. In our study, we have obtained an scale invariant power spectrum of cosmological perturbations. However, the ratio of tensor to scalar perturbations is of order 1, which does not agree with the current observations. For this reason, we suggest a model where a transition from the matter domination to a quasi de Sitter phase is produced in order to enhance the scalar power spectrum.},
doi = {10.1088/14757516/2013/11/068},
journal = {Journal of Cosmology and Astroparticle Physics},
issn = {14757516},
number = 11,
volume = 2013,
place = {United States},
year = {2013},
month = {11}
}