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We develop a theory of nonlinear cosmological perturbations on superhorizon scales for a single scalar field with a general kinetic term and a general form of the potential. We employ the ADM formalism and the spatial gradient expansion…

宇宙学与河外天体物理 · 物理学 2010-06-24 Yu-ichi Takamizu , Shinji Mukohyama , Misao Sasaki , Yoshiharu Tanaka

A new approach to quantum gravity is presented based on a nonlinear quantization scheme for canonical field theories with an implicitly defined Hamiltonian. The constant mean curvature foliation is employed to eliminate the momentum…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Charles H-T Wang

Using the Gauss-Bonnet formula, integral of the Gaussian curvature over a 2-surface enclosed by a curve in the asymptotically flat region of a static spacetime was found to be a measure of a gravitational analogue of Aharonov-Bohm effect by…

广义相对论与量子宇宙学 · 物理学 2013-07-26 M. Nouri-Zonoz , A. Parvizi

Length scales probed by large scale structure surveys are becoming closer to the horizon scale. Further, it has been recently understood that non-Gaussianity in the initial conditions could show up in a scale dependence of the bias of…

宇宙学与河外天体物理 · 物理学 2015-05-28 Tobias Baldauf , Uros Seljak , Leonardo Senatore , Matias Zaldarriaga

In this paper, we study the problem of the nonlinear interaction of impulsive gravitational waves for the Einstein vacuum equations. The problem is studied in the context of a characteristic initial value problem with data given on two null…

广义相对论与量子宇宙学 · 物理学 2017-04-26 Jonathan Luk , Igor Rodnianski

A 3+1 spacetime, with a shift vector that is the unique fundamental solution to the linearized wave operator, is introduced to model an interpretation of Wheeler's layman's analogy of the Quantum foam. To understand the distributional…

广义相对论与量子宇宙学 · 物理学 2023-05-30 Claes Cramer

We present a new analytic approach to describe large scale structure formation in the mildly non-linear regime. The central object of the method is the time-dependent probability distribution function generating correlators of the…

宇宙学与河外天体物理 · 物理学 2016-08-09 Diego Blas , Mathias Garny , Mikhail M. Ivanov , Sergey Sibiryakov

We study light propagation in the picture of semi-classical space-time that emerges in canonical quantum gravity in the loop representation. In such picture, where space-time exhibits a polymer-like structure at microscales, it is natural…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Rodolfo Gambini , Jorge Pullin

A fourth-order and a second-order nonlinear diffusion models in spectral space are proposed to describe gravitational wave turbulence in the approximation of strongly local interactions. We show analytically that the model equations satisfy…

广义相对论与量子宇宙学 · 物理学 2019-03-27 Sébastien Galtier , Sergey V. Nazarenko , Éric Buchlin , Simon Thalabard

Time-slicing has emerged as a strategy for incorporating semiclassical propagation into real-time path integral formulation and recovering full quantum dynamics. A central step is the decomposition of a time-evolved wave function into a…

量子物理 · 物理学 2026-03-13 Rahul Sharma , Amartya Bose

We use the Hamilton-Jacobi theory to study the nonlinear evolutions of inhomogeneous spacetimes during inflation in generalized gravity. We find the exact solutions to the lowest order Hamilton-Jacobi equation for special scalar potentials…

天体物理学 · 物理学 2009-11-10 Seoktae Koh , Sang Pyo Kim , Doo Jong Song

We present the third-order analytic solution of the matter density fluctuation in the proper-time hypersurface of nonrelativistic matter flows by solving the nonlinear general relativistic equations. The proper-time hypersurface provides a…

宇宙学与河外天体物理 · 物理学 2016-01-22 Jaiyul Yoo , Jinn-Ouk Gong

We give a review of recent work aimed at understanding the dynamics of gravitational collapse in quantum gravity. Its goal is to provide a non-perturbative computational framework for understanding the emergence of the semi-classical…

广义相对论与量子宇宙学 · 物理学 2008-01-09 Viqar Husain

We develop a theory of nonlinear cosmological perturbations on superhorizon scales where a characteristic length scale of perturbations is longer than the Hubble radius, in general theoretical frameworks. Our formalism is based on the…

广义相对论与量子宇宙学 · 物理学 2018-04-24 Yu-ichi Takamizu

One of the standard approaches of incorporating the quantum gravity (QG) effects into the semiclassical analysis is to adopt the notion of a quantum-corrected spacetime arising from the QG model. This procedure assumes that the expectation…

广义相对论与量子宇宙学 · 物理学 2023-12-29 Harkirat Singh Sahota , Kinjalk Lochan

Precise understanding of nonlinear evolution of cosmological perturbations during inflation is necessary for the correct interpretation of measurements of non-Gaussian correlations in the cosmic microwave background and the large-scale…

广义相对论与量子宇宙学 · 物理学 2013-05-30 Naonori S. Sugiyama , Eiichiro Komatsu , Toshifumi Futamase

We obtain the limiting distribution of the nodal area of random Gaussian Laplace eigenfunctions on $\mathbb{T}^3= \mathbb{R}^3/ \mathbb{Z}^3$ ($3$-dimensional 'arithmetic random waves'). We prove that, as the multiplicity of the eigenspace…

概率论 · 数学 2017-08-28 Valentina Cammarota

We show that tensoriality constraints in noncommutative Riemannian geometry in the 2-dimensional bicrossproduct model quantum spacetime algebra [x,t]=\lambda x drastically reduce the moduli of possible metrics g up to normalisation to a…

广义相对论与量子宇宙学 · 物理学 2015-06-15 Edwin Beggs , Shahn Majid

In this paper, we initiate the rigorous mathematical study of the problem of impulsive gravitational spacetime waves. We construct such spacetimes as solutions to the characteristic initial value problem of the Einstein vacuum equations…

广义相对论与量子宇宙学 · 物理学 2014-07-21 Jonathan Luk , Igor Rodnianski

We consider the evolution of perturbations to a flat FRW universe that arise from a ``stiff source,'' such as a self-ordering cosmic field that forms in a global symmetry-breaking phase transition and evolves via the Kibble mechanism.…

天体物理学 · 物理学 2009-10-22 Andrew H. Jaffe
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