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相关论文: Quantum cosmology with big-brake singularity

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Classical models for dark energy can exhibit a variety of singularities, many of which occur for scale factors much bigger than the Planck length. We address here the issue whether some of these singularities, the big freeze and the big…

广义相对论与量子宇宙学 · 物理学 2009-07-09 Mariam Bouhmadi-Lopez , Claus Kiefer , Barbara Sandhoefer , Paulo Vargas Moniz

We apply the formalism of quantum cosmology to models containing a phantom field. Three models are discussed explicitly: a toy model, a model with an exponential phantom potential, and a model with phantom field accompanied by a negative…

高能物理 - 理论 · 物理学 2009-11-11 Mariusz P. Dabrowski , Claus Kiefer , Barbara Sandhoefer

We investigate a cosmological model whose energy content is described by a Chaplygin gas represented by a scalar field $\phi$ with an associated potential producing a big bang singularity such that for vanishing scale factor, $a\to 0$, one…

广义相对论与量子宇宙学 · 物理学 2010-01-29 Frank Steiner , Andreas Woehr

We give an introduction into quantum cosmology with emphasis on its conceptual parts. After a general motivation we review the formalism of canonical quantum gravity on which discussions of quantum cosmology are usually based. We then…

广义相对论与量子宇宙学 · 物理学 2022-09-23 Claus Kiefer , Barbara Sandhoefer

The problems encountered in trying to quantize the various cosmological models, are brought forward by means of a concrete example. The Automorphism groups are revealed as the key element through which G.C.T.'s can be used for a general…

广义相对论与量子宇宙学 · 物理学 2011-07-19 T. Christodoulakis

Loop quantum gravity is believed to eliminate singularities such as the big bang and big crunch singularity. This belief is based on studies of so-called loop quantum cosmology which concerns symmetry-reduced models of quantum gravity. In…

广义相对论与量子宇宙学 · 物理学 2017-09-12 Ward Struyve

It is shown that the cosmological singularity in isotropic minisuperspaces is naturally removed by quantum geometry. Already at the kinematical level, this is indicated by the fact that the inverse scale factor is represented by a bounded…

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

In an open Friedmann-Robertson-Walker (FRW) space background, we study the classical and quantum cosmological models in the framework of the recently proposed nonlinear massive gravity theory. Although the constraints which are present in…

广义相对论与量子宇宙学 · 物理学 2015-06-04 Babak Vakili , Nima Khosravi

Quantum cosmology implies corrections to the classical equations of motion which may lead to significant departures from the classical trajectory, especially at high curvature near the big-bang singularity. Corrections could in principle be…

广义相对论与量子宇宙学 · 物理学 2014-09-09 Martin Bojowald , David Simpson

We study the polymeric nature of quantum matter fields using the example of a Friedmann-Lemaitre-Robertson-Walker universe sourced by a minimally coupled massless scalar field. The model is treated in the symmetry reduced regime via…

广义相对论与量子宇宙学 · 物理学 2015-09-16 Andreas Kreienbuehl , Tomasz Pawlowski

We canonically quantize the dynamics of the brane universe embedded into the five-dimensional Schwarzschild-anti-deSitter bulk space-time. We show that in the brane-world settings the formulation of the quantum cosmology, including the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 A. Boyarsky , A. Neronov , I. Tkachev

By regarding the vacuum as a perfect fluid with equation of state p=-rho, de Sitter's cosmological model is quantized. Our treatment differs from previous ones in that it endows the vacuum with dynamical degrees of freedom. Instead of being…

广义相对论与量子宇宙学 · 物理学 2015-06-25 Flavio G. Alvarenga , Nivaldo A. Lemos

We discuss the way non-perturbative quantization of cosmological spacetimes in loop quantum cosmology provides insights on the physics of Planck scale and the resolution of big bang singularity. In recent years, rigorous examination of…

广义相对论与量子宇宙学 · 物理学 2009-03-27 Parampreet Singh

Quantum cosmology in general denotes the application of quantum physics to the whole universe and thus gives rise to many realizations and examples, covering problems at different mathematical and conceptual levels. It is related to quantum…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Martin Bojowald

We comment on two issues in quantum cosmology, in the context of the Wheeler-De Witt equation and wave function of the Universe: (i) arrow of time and interpretation of the wave function in the classically allowed regions; (ii) stability of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 V. A. Rubakov

In this article we perform the Wheeler-DeWitt quantization for Bianchi type $I$ anisotropic cosmological model in the presence of a scalar field minimally coupled to the Einstein-Hilbert gravity theory. We also consider the cosmological…

广义相对论与量子宇宙学 · 物理学 2019-08-14 Saumya Ghosh , Sunandan Gangopadhyay , Prasanta K. Panigrahi

We illustrate the crucial role played by decoherence (consistency of quantum histories) in extracting consistent quantum probabilities for alternative histories in quantum cosmology. Specifically, within a Wheeler-DeWitt quantization of a…

广义相对论与量子宇宙学 · 物理学 2011-05-26 David A. Craig , Parampreet Singh

We consider two-dimensional quantum gravity endowed with a positive cosmological constant and coupled to a conformal field theory of large and positive central charge. We study cosmological properties at the classical and quantum level. We…

高能物理 - 理论 · 物理学 2025-03-05 Dionysios Anninos , Chiara Baracco , Beatrix Mühlmann

In this paper we discuss classical and quantum aspects of cosmological models in Brans-Dicke theory. First, we review cosmological bounce solution in Brans-Dicke theory that obeys energy conditions (without ghost) for a universe filled with…

广义相对论与量子宇宙学 · 物理学 2021-08-09 Carla R. Almeida , O. Galkina , J. C. Fabris

We consider a renormalizable two-dimensional model of dilaton gravity coupled to a set of conformal fields as a toy model for quantum cosmology. We discuss the cosmological solutions of the model and study the effect of including the…

高能物理 - 理论 · 物理学 2009-10-22 F. D. Mazzitelli , J. G. Russo
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