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相关论文: SO(4) Invariant States in Quantum Cosmology

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Transition to the semiclassical behaviour and the decoherence process for inhomogeneous perturbations generated from the vacuum state during an inflationary stage in the early Universe are considered both in the Heisenberg and the…

广义相对论与量子宇宙学 · 物理学 2010-11-01 David Polarski , Alexei A. Starobinsky

The Standard Model is the low-energy limit of a microscopic theory which includes extra dimensions and new symmetries. A part of my thesis consisted in constructing a new class of models with two extra dimensions. We showed that these…

高能物理 - 理论 · 物理学 2007-08-27 Chloe Papineau

Increasingly accurate observations are driving theoretical cosmology toward the use of more sophisticated descriptions of matter and the study of nonlinear perturbations of FL cosmologies, whose governing equations are notoriously…

广义相对论与量子宇宙学 · 物理学 2015-05-27 Claes Uggla , John Wainwright

We argue that models in which an observable variation of the fine structure constant is explained by motion of a cosmic scalar field, are not stable under renormalization, and require massive fine tuning that cannot be explained by any…

高能物理 - 唯象学 · 物理学 2009-11-07 T. Banks , M. Dine , M. R. Douglas

In the matter bounce scenario, a dust-dominated contracting space-time generates scale-invariant perturbations that, assuming a nonsingular bouncing cosmology, propagate to the expanding branch and set appropriate initial conditions for the…

广义相对论与量子宇宙学 · 物理学 2015-06-12 Edward Wilson-Ewing

We present the first experimental observation of modulation instability of partially spatially incoherent light beams in non-instantaneous nonlinear media. We show that even in such a nonlinear partially coherent system (of…

There is a formal analogy between the evolution of the universe, when this is seen as a trajectory in the minisuperspace, and the worldline followed by a test particle in a curved spacetime. The analogy can be extended to the quantum realm,…

广义相对论与量子宇宙学 · 物理学 2018-12-31 Salvador J. Robles-Pérez

We consider multidimensional gravitational models with a nonlinear scalar curvature term and form fields in the action functional. In our scenario it is assumed that the higher dimensional spacetime undergoes a spontaneous compactification…

高能物理 - 理论 · 物理学 2007-05-23 U. Guenther , P. Moniz , A. Zhuk

A quantum gravity theory which becomes renormalizable at short distances due to a spontaneous symmetry breaking of Lorentz invariance and diffeomorphism invariance is studied. A breaking of Lorentz invariance with the breaking patterns…

高能物理 - 理论 · 物理学 2010-05-25 J. W. Moffat

The full spectrum and eigenfunctions of the quantum version of a nonlinear oscillator defined on an N-dimensional space with nonconstant curvature are rigorously found. Since the underlying curved space generates a position-dependent…

Contrary to what is often stated, a fundamental spacetime discreteness need not contradict Lorentz invariance. A causal set's discreteness is in fact locally Lorentz invariant, and we recall the reasons why. For illustration, we introduce a…

广义相对论与量子宇宙学 · 物理学 2009-11-10 Fay Dowker , Joe Henson , Rafael D. Sorkin

We analyze the constraints of general coordinate invariance for quantum theories possessing conformal symmetry in four dimensions. The character of these constraints simplifies enormously on the Einstein universe $R \times S^3$. The…

高能物理 - 理论 · 物理学 2016-08-24 Ignatios Antoniadis , Pawel O. Mazur , Emil Mottola

We describe a mechanism that results in the nonlinear instability of stationary states even in the case where the stationary states are linearly stable. This instability is due to the nonlinearity-induced coupling of the linearization's…

斑图形成与孤子 · 物理学 2015-06-03 P. G. Kevrekidis , D. E. Pelinovsky , A. Saxena

In general quantum systems there are two kinds of spacetime modes, those that fluctuate and those that do not. Fluctuating modes have normalizable wavefunctions. In the context of 2D gravity and ``non-critical'' string theory these are…

高能物理 - 理论 · 物理学 2009-09-15 Nathan Seiberg , Stephen Shenker

Quantum decoherence can arise due to classical fluctuations in the parameters which define the dynamics of the system. In this case decoherence, and complementary noise, is manifest when data from repeated measurement trials are combined.…

广义相对论与量子宇宙学 · 物理学 2011-09-13 G. J. Milburn

We complete the formulation of a general framework for the analysis of high-order nonspherical perturbations of a four-dimensional spherical spacetime by including a gauge-invariant description of the perturbations. We present a general…

广义相对论与量子宇宙学 · 物理学 2008-11-26 David Brizuela , Jose M. Martin-Garcia , Guillermo A. Mena Marugan

In classical Lorentz-invariant field theories, localized soliton solutions necessarily break translation symmetry. In the corresponding quantum field theories, the position is quantized and, if the theory is not compactified, they have…

高能物理 - 理论 · 物理学 2026-04-27 Jarah Evslin

Incoherence in the controlled Hamiltonian is an important limitation on the precision of coherent control in quantum information processing. Incoherence can typically be modelled as a distribution of unitary processes arising from slowly…

量子物理 · 物理学 2009-11-10 N. Boulant , S. Furuta , J. Emerson , T. F. Havel , D. G. Cory

In this paper we present a gauge-invariant formalism for perturbations of the brane-world model developed by the author, A. Ishibashi and O. Seto recently, and analyze the behavior of cosmological perturbations in a spatially flat expanding…

高能物理 - 理论 · 物理学 2009-10-31 Hideo Kodama

Three of the big puzzles of theoretical physics are the following: (i) There is apparently no time evolution in the dynamics of quantum general relativity, because the allowed quantum states must obey the Hamiltonian constraint. (ii) During…

广义相对论与量子宇宙学 · 物理学 2015-12-29 Shreya Banerjee , Sayantani Bera , Tejinder P. Singh