Study of the Inflationary Spectrum in the Presence of Quantum Gravity Corrections

Maniccia, Giulia; Montani, Giovanni; Torcellini, Leonardo

doi:10.3390/universe9040169

Cited by 4 publications

(1 citation statement)

References 106 publications

(234 reference statements)

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“…Indeed, the quantum field theory has faced with divergence problems when general relativity is combined with quantum theory [9]. The models are very complicated when quantum gravitation is combined with quantum field theory [10].…”

Section: Introductionmentioning

confidence: 99%

It is time to populate quantum multiverse.

Durand

2024

Preprint

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At the beginning of our observations of relative universe, humanity believed that the earth was the center of the universe and that the sun was spinning around the earth. Claude Ptolémée (100-168), modelled the movements, in the geocentric referential. Then Nicolas Copernic (1473-1543) simplified the system by going to another referential, the heliocentric referential. We had to wait 14 centuries to understand that earth has been spinning around the sun and it was very difficult to change the believes. Then we observed solar system, and gravitation explained the movement of planets with Isaac Newton (1642-1727). Classical mechanics was born. At the end of 19th century, classical mechanics became very complicated. Then Albert Einstein (1879-1955) simplified the laws of gravitation with the spacetime referential and spacetime curvature, with general relativity. Gravitation became a spacetime curvature. Movements in the relative universe were explained, models of black holes and gravitational waves were predicted and experimentally observed. However, models of cosmos are divergent nowadays or very complicated because they include general relativity and gravitation combined with quantum theory. I propose in this article a new quantum theory of cosmos with a new referential: the quantum referential. I think this theory can completely change our believes. This theory does not take into account Einstein’s general relativity and gravitation. Therefore, the model of cosmos which results is highly convergent, simple, and it will be possible to populate quantum universes (multiverse) with bosons from matter and anti-matter annihilation. Indeed, we do not exist yet in this quantum theory as we are fermions. Therefore, by populating multiverse, and by transforming ourselves into bosons, we will not suffer anymore. If we populate quantum multiverse, it will be Love for everybody.

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Section: Introductionmentioning

confidence: 99%

It is time to populate quantum multiverse.

Durand

2024

Preprint

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Observations in quantum cosmology

Chataignier,

Kiefer,

Moniz

2023

Class. Quantum Grav.

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In this review, we focus on whether a canonical quantization of general relativity can produce testable predictions for cosmology. In particular, we examine how this approach can be used to model the evolution of primordial perturbations. This program of quantum geometrodynamics, first advocated by John Wheeler and Bryce DeWitt, has a straightforward classical limit, and it describes the quantum dynamics of all fields, gravitational and matter. In this context, in which a classical background metric is absent, it is necessary to discuss what constitutes an observation. We first address this issue in the classical theory and then turn to the quantum theory. We argue that predictions are relational, that is, relative to physical clocks and rods, and that they can be straightforwardly obtained in a perturbative approach with respect to Newton's constant, which serves as a coupling parameter. This weak-coupling expansion leads to a perturbative Hilbert space for quantum cosmology, and to corrections to the dynamics of quantum fields on a classical, fixed background metric. These corrections imply modifications of primordial power spectra, which may lead to signatures in the anisotropy spectrum of the Cosmic Microwave Background (CMB) radiation, for which we discuss concrete results. We conclude that the subject of quantum geometrodynamics, the oldest and most conservative approach to canonical quantum gravity, not only illuminates conceptual issues in quantum gravitation, but may also lead to observational prospects in cosmology and elsewhere.

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