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相关论文: Solving Stochastic Inflation for Arbitrary Potenti…

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We provide a formulation of Stochastic Inflation in full general relativity that goes beyond the slow-roll and separate universe approximations. We show how gauge invariant Langevin source terms can be obtained for the complete set of…

广义相对论与量子宇宙学 · 物理学 2024-06-18 Yoann L. Launay , Gerasimos I. Rigopoulos , E. P. S. Shellard

In our previous paper, we have proposed a new algorithm to calculate the power spectrum of the curvature perturbations generated in inflationary universe with use of the stochastic approach. Since this algorithm does not need the…

宇宙学与河外天体物理 · 物理学 2014-10-15 Tomohiro Fujita , Masahiro Kawasaki , Yuichiro Tada

Quantum gravitational back-reaction offers the potential of simultaneously resolving the problem of the cosmological constant and providing a natural model of inflation in which scalars play no special role. In this model inflation begins…

天体物理学 · 物理学 2007-05-23 R. P. Woodard

By making a suitable generalization of the Starobinsky stochastic inflation, we propose a classical phase space formulation of stochastic inflation which may be used for a quantitative study of decoherence of cosmological perturbations…

广义相对论与量子宇宙学 · 物理学 2012-01-04 Jan Weenink , Tomislav Prokopec

Environment interaction may induce stochastic semiclassical dynamics in open quantum systems. In the gravitational context, stress-energy fluctuations of quantum matter fields give rise to a stochastic behaviour in the spacetime geometry.…

广义相对论与量子宇宙学 · 物理学 2011-04-15 Albert Roura , Enric Verdaguer

We evaluate the quantum backreaction due to a gauge field coupled to a pseudo-scalar field driving a slow-roll inflationary stage, the so-called axion inflation. The backreaction is evaluated for the first time using a gauge invariant…

广义相对论与量子宇宙学 · 物理学 2024-10-23 Davide Campanella Galanti , Pietro Conzinu , Giovanni Marozzi , Simony Santos da Costa

We prove that the stochastic and standard field-theoretical approaches produce exactly the same results for the amount of light massive scalar field fluctuations generated during inflation in the leading order of the slow-roll…

高能物理 - 理论 · 物理学 2009-02-10 F. Finelli , G. Marozzi , A. A. Starobinsky , G. P. Vacca , G. Venturi

We consider a universe in which inflation commences because of a positive cosmological constant, the effect of which is progressively screened by the interaction between virtual gravitons that become trapped in the expansion of spacetime.…

高能物理 - 唯象学 · 物理学 2009-10-30 N. C. Tsamis , R. P. Woodard

We obtain the non-equilibrium effective action of an inflaton like scalar field --the system-- by tracing over sub Hubble degrees of freedom of "environmental" light scalar fields. The effective action is stochastic leading to effective…

宇宙学与河外天体物理 · 物理学 2016-02-04 D. Boyanovsky

I describe a recently derived stochastic approach to inflaton dynamics which can address some serious problems associated with conventional inflationary theory. Using this theory I derive an exact solution to the stochastic dynamics for the…

广义相对论与量子宇宙学 · 物理学 2009-12-30 Andrew Matacz

One common approach for cosmic inflation consists in couple Einstein's gravity with a scalar field, often referred to inflaton field. In order to derive analytic simple scenarios, we usually work in the {\it slow-roll} regime. In such an…

广义相对论与量子宇宙学 · 物理学 2021-01-01 J. R. L. Santos , P. H. R. S. Moraes

In this paper, we compare dispersions of a scalar field in Euclidean quantum gravity with stochastic inflation. We use Einstein gravity and a minimally coupled scalar field with a quadratic potential. We restrict our attention to small mass…

广义相对论与量子宇宙学 · 物理学 2014-09-16 Dong-il Hwang , Bum-Hoon Lee , Ewan D. Stewart , Dong-han Yeom , Heeseung Zoe

The stochastic inflation program is a framework for understanding the dynamics of a quantum scalar field driving an inflationary phase. Though widely used and accepted, there have over recent years been serious criticisms of this theory. In…

广义相对论与量子宇宙学 · 物理学 2014-11-17 Andrew Matacz

We show how the quantum to classical transition of the cosmological fluctuations produced during inflation can be described by means of the influence functional and the master equation. We split the inflaton field into the system-field…

广义相对论与量子宇宙学 · 物理学 2016-08-31 Fernando C. Lombardo , Diana Lopez Nacir

This thesis is dedicated to studying cosmological inflation, which is a period of accelerated expansion in the very early Universe that is required to explain the observed anisotropies in the cosmic microwave background. Inflation, when…

宇宙学与河外天体物理 · 物理学 2021-02-02 Chris Pattison

For simple inflationary models, we provide a consistent and complete scheme by which the macro-physical details of early universe inflation may be determined explicitly from the underlying micro-physical theory. We examine inflationary…

高能物理 - 唯象学 · 物理学 2007-05-23 D. Cormier

We propose functional approach to the stochastic inflationary universe dynamics. It is based on path integral representation of the solution to the differential equation for the scalar field probability distribution. In the saddle-point…

广义相对论与量子宇宙学 · 物理学 2010-01-15 Yuri V. Shtanov

We present a review on the state-of-the-art of the mathematical framework known as stochastic inflation, paying special attention to its derivation and giving references for the readers interested on results coming from the application of…

广义相对论与量子宇宙学 · 物理学 2022-06-20 Diego Cruces

We generalize the stochastic approach to quasi-power-law inflationary Universes,obtain the corresponding Langevin and Fokker-Planck equations for the scalar field driving inflation and find stationary solutions to the above FP equation.

高能物理 - 理论 · 物理学 2009-10-22 Boris Spokoiny

In this paper we present a path integral formulation of stochastic inflation, in which volume weighting can easily be implemented. With an in-depth study of inflation in a quartic potential, we investigate how the inflaton evolves and how…

高能物理 - 理论 · 物理学 2013-05-29 Steven Gratton