Perturbations in Quantum Cosmology: The Continuum Limit in Fourier Space
arXiv:1809.03884 · doi:10.1103/PhysRevD.98.103522
Abstract
We analyze the passage to a continuum limit of the mode spectrum of primordial perturbations around flat cosmological spacetimes in Quantum Cosmology, showing that this limit can be reached even if one starts by considering a finite fiducial cell as spatial slice. Whereas the resulting system can be described in an invariant way under changes of the fiducial volume using appropriate variables, both for the background cosmology and the perturbations, obtaining in this way a discrete mode spectrum owing to the compactness of the fiducial cell, we show that the desired continuum limit for the perturbations can still be established by means of scaling transformations of the physical volume when this volume grows unboundedly. These transformations lead to a model with a continuum of modes and independent of any scale of reference for the physical volume. For the sake of comparison, we also consider an alternative road to the continuum in Fourier space that has been employed in geometrodynamics and is based on the use of scaling transformations of the fiducial volume, together with variables that are independent of them.
arXiv comment12 pages
References in corpus (25)
- Loop Quantum Cosmology: A Status Report
- Quantum Nature of the Big Bang: Improved dynamics
- Quantum Nature of the Big Bang: An Analytical and Numerical Investigation
- The pre-inflationary dynamics of loop quantum cosmology: Confronting quantum gravity with observations
- A Quantum Gravity Extension of the Inflationary Scenario
- An Extension of the Quantum Theory of Cosmological Perturbations to the Planck Era
- Quantum Gravitational Contributions to the CMB Anisotropy Spectrum
- Gauge-Invariant Perturbations in Hybrid Quantum Cosmology
- Detailed analysis of the predictions of loop quantum cosmology for the primordial power spectra
- Further Improvements in the Understanding of Isotropic Loop Quantum Cosmology
- Scalar and Vector Perturbations in Quantum Cosmological Backgrounds
- Cosmological perturbations in Hybrid Loop Quantum Cosmology: Mukhanov-Sasaki variables
- Hybrid quantization of an inflationary model: The flat case
- Primordial power spectra for scalar perturbations in loop quantum cosmology
- Exploring cosmic homogeneity with the BOSS DR12 galaxy sample
- Hybrid loop quantum cosmology and predictions for the cosmic microwave background
- Testing loop quantum cosmology
- Generalized effective description of loop quantum cosmology
- Primordial tensor modes of the early Universe
- Scalar Perturbations in Scalar Field Quantum Cosmology
- Time-dependent mass of cosmological perturbations in the hybrid and dressed metric approaches to loop quantum cosmology
- Phenomenology with fluctuating quantum geometries in loop quantum cosmology
- Quantization of pure gravitational plane waves
- Large quantum gravity effects: Cylindrical waves in four dimensions
- Probing large scale homogeneity and periodicity in the LRG distribution using Shannon entropy
Cited by in corpus (9)
- Hybrid Loop Quantum Cosmology: An Overview
- The Vacuum State of Primordial Fluctuations in Hybrid Loop Quantum Cosmology
- Non-oscillating power spectra in Loop Quantum Cosmology
- Power spectrum of primordial perturbations for an emergent universe in quantum reduced loop gravity
- Primordial perturbations in the Dapor-Liegener model of hybrid loop quantum cosmology
- The time-dependent mass of cosmological perturbations in loop quantum cosmology: Dapor-Liegener regularization
- A Brief Overview of Results about Uniqueness of the Quantization in Cosmology
- Primordial perturbations in kinetically dominated regimes of general relativity and hybrid quantum cosmology
- Expansion-sensitive coupling of a local quantum system in de Sitter cosmology