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Isotropic models in loop quantum cosmology allow explicit calculations, thanks largely to a completely known volume spectrum, which is exploited in order to write down the evolution equation in a discrete internal time. Because of genuinely…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Martin Bojowald

A free massless scalar field is coupled to homogeneous and isotropic loop quantum cosmology. The coupled model is investigated in the vicinity of the classical singularity, where discreteness is essential and where the quantum model is…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Martin Bojowald , Franz Hinterleitner

A brief review of various numerical techniques used in loop quantum cosmology and results is presented. These include the way extensive numerical simulations shed insights on the resolution of classical singularities, resulting in the key…

广义相对论与量子宇宙学 · 物理学 2013-07-11 Parampreet Singh

Loop quantum gravity is a mature theory. To proceed to explicit calculations in cosmology, it is necessary to make assumptions and simplifications based on the symmetries of the cosmological setting. Symmetry reduction is especially…

广义相对论与量子宇宙学 · 物理学 2016-08-03 Aurélien Barrau , Boris Bolliet

We investigate quantum cosmological models in an n-dimensional anisotropic universe in the presence of a massless scalar field. Our basic inspiration comes from Chodos and Detweiler's classical model which predicts an interesting behaviour…

广义相对论与量子宇宙学 · 物理学 2018-02-14 F. A. P. Alves-Júnior , M. L. Pucheu , A. B. Barreto , C. Romero

In this contribution we consider the issue of singularity resolution within loop quantum cosmology (LQC) for different homogeneous models. We present results of numerical evolutions of effective equations for both isotropic as well as…

广义相对论与量子宇宙学 · 物理学 2012-12-04 Alejandro Corichi , Asieh Karami , Edison Montoya

Loop quantum cosmology is an application of recent developments for a non-perturbative and background independent quantization of gravity to a cosmological setting. Characteristic properties of the quantization such as discreteness of…

天体物理学 · 物理学 2009-11-13 Martin Bojowald

We study the early-time behavior of isotropic and homogeneous solutions in vacuum as well as radiation-filled cosmological models in the full, effective, four dimensional gravity theory with higher derivatives. We use asymptotic methods to…

广义相对论与量子宇宙学 · 物理学 2017-06-06 Georgios Kolionis

In Loop Quantum Gravity mathematically rigorous models of full quantum gravity were proposed. In this paper we study a cosmological sector of one of the models describing quantum gravity with positive cosmological constant coupled to…

广义相对论与量子宇宙学 · 物理学 2022-11-09 Marcin Kisielowski

The resolution of the problem of cosmological singularity in the framework of gauge theories of gravitation is discussed. Generalized cosmological Friedmann equations for homogeneous isotropic models filled by interacting scalar fields and…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Albert V. Minkevich

Effective equations often provide powerful tools to develop a systematic understanding of detailed properties of a quantum system. This is especially helpful in quantum cosmology where several conceptual and technical difficulties…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Martin Bojowald , Hector Hernandez , Aureliano Skirzewski

The framework of quantum symmetry reduction is applied to loop quantum gravity with respect to transitively acting symmetry groups. This allows to test loop quantum gravity in a large class of minisuperspaces and to investigate its features…

广义相对论与量子宇宙学 · 物理学 2010-11-19 Martin Bojowald

A brief overview of loop quantum cosmology of homogeneous isotropic models is presented with emphasis on the origin of and subtleties associated with the resolution of big bang and big crunch singularities. These results bear out the…

广义相对论与量子宇宙学 · 物理学 2009-04-17 Abhay Ashtekar

The closed, k=1, FRW model coupled to a massless scalar field is investigated in the framework of loop quantum cosmology using analytical and numerical methods. As in the k=0 case, the scalar field can be again used as emergent time to…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Abhay Ashtekar , Tomasz Pawlowski , Parampreet Singh , Kevin Vandersloot

Semiclassical states in isotropic loop quantum cosmology are employed to show that the improved dynamics has the correct classical limit. The effective Hamiltonian for the quantum cosmological model with a massless scalar field is thus…

广义相对论与量子宇宙学 · 物理学 2009-02-27 You Ding , Yongge Ma , Jinsong Yang

The Lorentzian Hamiltonian constraint is solved for isotropic loop quantum cosmology coupled to a massless scalar field. As in the Euclidean case, the discreteness of quantum geometry removes the classical singularity from the quantum…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Franz Hinterleitner , Seth Major

In the last decade, progress on quantization of homogeneous cosmological spacetimes using techniques of loop quantum gravity has led to insights on various fundamental questions and has opened new avenues to explore Planck scale physics.…

广义相对论与量子宇宙学 · 物理学 2016-12-06 Ivan Agullo , Parampreet Singh

In recent years, Loop Quantum Gravity has emerged as a solid candidate for a nonperturbative quantum theory of General Relativity. It is a background independent theory based on a description of the gravitational field in terms of…

广义相对论与量子宇宙学 · 物理学 2009-10-16 Guillermo A. Mena Marugan

We shall present here the causal interpretation of canonical quantum gravity in terms of new variables. Then we shall apply it to the minisuperspace of cosmology. A vacuum solution of quantum cosmology is obtained and the Bohmian trajectory…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Ali Shojai , Fatimah Shojai

We provide a detailed analysis of Friedmann-Robertson-Walker universes in a wide range of scalar-tensor theories of gravity. We apply solution-generating methods to three parametrised classes of scalar-tensor theory which lead naturally to…

广义相对论与量子宇宙学 · 物理学 2009-10-28 John D. Barrow , Paul Parsons
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