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A quantitative Brenier decomposition shows that the deviation of a map from volume preserving is bounded by the deviation of the derivative from volume preserving. A study of the matrix nearness problem for $SL(n)$ and $Sp(2n)$ relates the…

偏微分方程分析 · 数学 2017-04-19 Christopher Policastro

We develop a non-linear framework for describing long-wavelength perturbations in multiple-field inflation. The basic variables describing inhomogeneities are defined in a non-perturbative manner, are invariant under changes of time slicing…

天体物理学 · 物理学 2009-11-11 G. I. Rigopoulos , E. P. S. Shellard , B. J. W. van Tent

In this paper, we discuss some limitations of the modified equations approach as a tool for stability analysis for a class of explicit linear schemes to scalar partial derivative equations. We show that the infinite series obtained by…

数值分析 · 数学 2020-04-28 Firas Dhaouadi , Emilie Duval , Sergey Tkachenko , Jean-Paul Vila

We study the detectability, given CMB polarization maps, of departures from the inflationary consistency equation, r \equiv T/S \simeq -5 n_T, where T and S are the tensor and scalar contributions to the quadrupole variance, respectively.…

天体物理学 · 物理学 2009-11-07 Yong-Seon Song , Lloyd Knox

At the end of inflation, dynamical instability can rapidly deposit the energy of homogeneous cold inflaton into excitations of other fields. This process, known as preheating, is rather violent, inhomogeneous and non-linear, and has to be…

高能物理 - 唯象学 · 物理学 2009-03-27 Andrei V. Frolov

The so-called "trans-Planckian" problem of inflation may be evaded by positing that modes come into existence only when they became "cis-Planckian" by virtue of expansion. However, this would imply that for any mode a new random realization…

宇宙学与河外天体物理 · 物理学 2019-01-31 Carlo R. Contaldi , Joao Magueijo

To first order in the deviation from scale invariance the inflationary potential and its first two derivatives can be expressed in terms of the spectral indices of the scalar and tensor perturbations, $n$ and $n_T$, and their contributions…

天体物理学 · 物理学 2014-10-13 Andrew R Liddle , Michael S Turner

In the framework of a flat FLRW model we derive an inflationary regime in which the scalar field, laying on the plateau of its potential, admits a linear time dependence and remains close to a constant value. The behaviour of inhomogeneous…

广义相对论与量子宇宙学 · 物理学 2016-11-09 Giovanni Imponente , Giovanni Montani

We propose a new method for spatio-temporal forecasting on arbitrarily distributed points. Assuming that the observed system follows an unknown partial differential equation, we derive a continuous-time model for the dynamics of the data…

机器学习 · 计算机科学 2022-03-18 Marten Lienen , Stephan Günnemann

Previously defined covariant and gauge-invariant perturbation variables, representing, e.g., the fractional spatial energy density gradient on hypersurfaces of constant expansion, are used to simplify the linear perturbation analysis of a…

天体物理学 · 物理学 2009-10-30 Winfried Zimdahl

We study closed systems of particles that are subject to stochastic forces in addition to the conservative forces. The stochastic equations of motion are set up in such a way that the energy is strictly conserved at all times. To ensure…

统计力学 · 物理学 2022-10-05 Tânia Tomé , Mário J. de Oliveira

We propose a new mechanism to generate density perturbations in inflationary models. Spatial fluctuations in the decay rate of the inflaton field to ordinary matter lead to fluctuations in the reheating temperature. We argue that in most…

天体物理学 · 物理学 2009-11-07 Gia Dvali , Andrei Gruzinov , Matias Zaldarriaga

To assess the durability of structures, heat and moisture transport need to be analyzed. To provide a reliable estimation of heat and moisture distribution in a certain structure, one needs to include all available information about the…

数值分析 · 计算机科学 2013-03-19 Anna Kucerova , Jan Sykora

In this work, we study the effects on the relevant observational parameters of an inflationary universe from a chaotic potential with a step. We numerically evolve the perturbation equations within both cold inflation and warm inflation. On…

广义相对论与量子宇宙学 · 物理学 2023-03-09 Clara Rojas , Rafael Hernández-Jiménez

Inflation is the currently accepted paradigm for the beginnings of the Universe. To explain the observed almost scale invariant spectrum of density perturbations with only a slight spectral tilt, inflation must have been "slow roll", that…

高能物理 - 理论 · 物理学 2021-01-07 Hao Geng

We consider a coarse-grained description of a system of self-propelled particles given by hydrodynamic equations for the density and polarization fields. We find that the ordered moving or flocking state of the system is unstable to spatial…

统计力学 · 物理学 2013-05-29 Shradha Mishra , Aparna Baskaran , M. Cristina Marchetti

Physics Informed Neural Networks is a numerical method which uses neural networks to approximate solutions of partial differential equations. It has received a lot of attention and is currently used in numerous physical and engineering…

数值分析 · 数学 2025-07-10 Dimitrios Gazoulis , Ioannis Gkanis , Charalambos G. Makridakis

The convergence of stochastic interacting particle systems in the mean-field limit to solutions of conservative stochastic partial differential equations is established, with optimal rate of convergence. As a second main result, a…

概率论 · 数学 2022-12-15 Benjamin Gess , Rishabh S. Gvalani , Vitalii Konarovskyi

The linear cosmological perturbation theory of almost homogeneous and isotropic perfect fluid and scalar field universes is reconsidered and formally simplified. Using the existence of a covariant conserved quantity on large perturbation…

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

Thermal convection in an inclined layer between two parallel walls kept at different fixed temperatures is studied for fixed Prandtl number Pr=1.07. Depending on the angle of inclination and the imposed temperature difference, the flow…

斑图形成与孤子 · 物理学 2020-08-26 Florian Reetz , Tobias M. Schneider