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相关论文: Loop Quantum Gravity and the The Planck Regime of …

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Within the framework of loop quantum cosmology, there exists a semi-classical regime where spacetime may be approximated in terms of a continuous manifold, but where the standard Friedmann equations of classical Einstein gravity receive…

广义相对论与量子宇宙学 · 物理学 2009-11-10 James E. Lidsey

We explore a reduced phase space quantization of loop quantum cosmology (LQC) for a spatially flat FLRW universe filled with reference fields and an inflaton field in a Starobinsky inflationary potential. We consider three separate cases in…

广义相对论与量子宇宙学 · 物理学 2021-01-04 Kristina Giesel , Bao-Fei Li , Parampreet Singh

We investigate a nonsingular initial state of the Universe which leads to inflation naturally. The model is described by a scalar field with a quadratic potential in Eddington-inspired Born-Infeld gravity. The curvature of this initial…

广义相对论与量子宇宙学 · 物理学 2013-08-26 Inyong Cho , Hyeong-Chan Kim , Taeyoon Moon

Quantum fluctuations of the gravitational field in the early Universe, amplified by inflation, produce a primordial gravitational-wave background across a broad frequency band. We derive constraints on the spectrum of this gravitational…

The standard inflationary version of the origin of the cosmic structure as the result of the quantum fluctuations during the inflationary stage is less than fully satisfactory: how exactly does the Universe transit from a homogeneous and…

广义相对论与量子宇宙学 · 物理学 2015-03-17 Adolfo De Unánue

The ability to reproduce the observed matter power spectrum $P(k)$ to high accuracy is often considered as a triumph of inflation. In this work, we explore an alternative explanation for the power spectrum based on nonperturbative quantum…

广义相对论与量子宇宙学 · 物理学 2019-03-18 Herbert W. Hamber , Lu Heng Sunny Yu

It is shown that the inflationary era in early universe is realized due to the effect of backreaction of quantized matter fields. In fact we start by quantizing a free scalar field in the Friedmann-Robertson-Walker space-time, and the field…

高能物理 - 理论 · 物理学 2015-06-23 Yoshinobu Habara , Hikaru Kawai , Masao Ninomiya

Theoretical arguments and cosmological observations suggest that Einstein's theory of general relativity needs to be modified at high energies. One of the best motivated higher-curvature extensions of general relativity is…

广义相对论与量子宇宙学 · 物理学 2017-08-04 Laura Sberna

Cosmic inflation provides a window to the highest energy densities accessible in nature, far beyond those achievable in any realistic terrestrial experiment. Theoretical insights into the inflationary era and its observational probes may…

We use the separate universe framework to study cosmological perturbations within the group field theory formalism for quantum gravity, based on multi-condensate quantum states. Working with a group field theory action for gravity minimally…

广义相对论与量子宇宙学 · 物理学 2018-09-26 Florian Gerhardt , Daniele Oriti , Edward Wilson-Ewing

Loop quantum cosmology is a symmetry-reduced application of loop quantum gravity. The theory predicts a bounce for the universe at the Planck scale and resolves the singularity of standard cosmology. The dynamics is also governed by an…

广义相对论与量子宇宙学 · 物理学 2024-06-27 Abolhassan Mohammadi

A fascinating and deep question about nature is what one would see if one could probe space and time at smaller and smaller distances. Already the 19th-century founders of modern geometry contemplated the possibility that a piece of empty…

高能物理 - 理论 · 物理学 2009-11-11 R. Loll , J. Ambjorn , J. Jurkiewicz

A static non-singular 10-dimensional closed Friedmann universe of Planck size, filled with a perfect fluid with an equation of state with w = -2/3, can arise spontaneously by a quantum fluctuation from nothing in 11-dimensional spacetime. A…

广义相对论与量子宇宙学 · 物理学 2009-11-11 T. R. Mongan

It is widely accepted that the primordial universe experienced a brief period of accelerated expansion called inflation. This scenario provides a plausible solution to the horizon and flatness problems. However, the particle physics…

广义相对论与量子宇宙学 · 物理学 2020-07-17 Sebastien Galtier , Jason Laurie , Sergey V. Nazarenko

According to the inflationary scenario for the very early Universe, all inhomogeneities in the Universe are of genuine quantum origin. On the other hand, looking at these inhomogeneities and measuring them, clearly no specific quantum…

广义相对论与量子宇宙学 · 物理学 2009-10-31 C. Kiefer , D. Polarski , A. A. Starobinsky

In a previous paper we proposed a new approach to the beginning of inflation -- a lingering universe. The universe begins in a lingering state with a nearly vanishing Hubble parameter. This calls into question the absolute age of the…

宇宙学与河外天体物理 · 物理学 2025-01-09 Brandon Melcher , Arnab Pradhan , Scott Watson

Quantum gravity places entirely new challenges on the formulation of a consistent theory as well as on an extraction of potentially observable effects. Quantum corrections due to the gravitational field are commonly expected to be tiny…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Martin Bojowald

This work is an analytical study of the main differences between classical inflationary effects of a fast-roll regime and imprints of hybrid Loop Quantum Cosmology (LQC) on the primordial power spectrum. Effective LQC solutions of…

广义相对论与量子宇宙学 · 物理学 2021-10-01 Beatriz Elizaga Navascués , Guillermo A. Mena Marugán

This chapter provides a review of the frameworks developed for cosmological perturbation theory in loop quantum cosmology, and applications to various models of the early universe including inflation, ekpyrosis and the matter bounce, with…

广义相对论与量子宇宙学 · 物理学 2024-03-08 Ivan Agullo , Anzhong Wang , Edward Wilson-Ewing

In this paper we investigate the cosmological dynamics of geometric inflation by means of the tools of the dynamical systems theory. We focus in the study of two explicit models where it is possible to sum the infinite series of higher…

广义相对论与量子宇宙学 · 物理学 2021-03-31 Israel Quiros , Roberto De Arcia , Ricardo García-Salcedo , Tame Gonzalez , Francisco X. Linares Cedeño , Ulises Nucamendi