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相关论文: Patterns from preheating

200 篇论文

Systems that exhibit pattern formation are typically driven and dissipative. In the early universe, parametric resonance can drive explosive particle production called preheating. The fields that are populated then decay quantum…

高能物理 - 唯象学 · 物理学 2016-09-06 A. Sornborger , M. Parry

It is assumed that during inflation, all energy was contained in a slow-rolling inflaton field $\phi$. The particles constituting the Universe are created due to interactions with the field $\phi$ coherently oscillating after inflation. The…

高能物理 - 唯象学 · 物理学 2007-05-23 Lev Kofman

In inflationary cosmology, the particles constituting the Universe are created after inflation in the process of reheating due to the interaction with the oscillating inflaton field. We briefly review the basics of the slow reheating, and…

天体物理学 · 物理学 2007-05-23 Lev Kofman

In the single-field model, the preheating process occurs through self-resonance of inflaton field. We study the nonlinear structures generated during preheating in the $\alpha$-attractor models and monodromy models. The potentials have a…

宇宙学与河外天体物理 · 物理学 2025-04-16 Tianyu Jia , Yu Sang , Xue Zhang

Reheating after inflation occurs due to particle production by the oscillating inflaton field. In this paper we describe the perturbative approach to reheating, and then concentrate on effects beyond the perturbation theory. They are…

高能物理 - 唯象学 · 物理学 2009-09-29 Lev Kofman , Andrei Linde , Alexei Starobinsky

The paradigm of the inflationary universe provides a possible explanation for several observed cosmological properties. In order for such solutions to be successful, the universe must convert the energy stored in the inflaton potential into…

宇宙学与河外天体物理 · 物理学 2025-09-01 Leia Barrowes , Fred C. Adams , Anthony M. Bloch , John T. Giblin, , Scott Watson

In this work, we investigate the preheating mechanism in a disformally-coupled inflationary model where the scalar field $\phi$ (which is the inflaton field) naturally coupled to another matter field $\chi$ induced by the disformal…

高能物理 - 唯象学 · 物理学 2017-07-26 Khamphee Karwan , Phongpichit Channuie

Exciton-polaritons generated by light-induced potentials can spontaneously condense into macroscopic quantum states that display nontrivial spatial and temporal density modulation. While these patterns and their dynamics can be reproduced…

介观与纳米尺度物理 · 物理学 2013-11-20 Li Ge , Ani Nersisyan , Baris Oztop , Hakan E. Tureci

Polariton condensation can be regarded as a self-organization phenomenon, where phase ordering is established among particles in the system. In such condensed systems, further ordering can possibly occur in the particle density…

量子气体 · 物理学 2015-03-19 F. Manni , K. G. Lagoudakis , T. C. H. Liew , R. André , B. Deveaud-Plédran

We propose a new mechanism of non-thermal particle production during inflation based on a narrow parametric resonance, akin to the dynamics of post-inflationary preheating. The mechanism is based on the production of scalar particles with a…

高能物理 - 唯象学 · 物理学 2025-07-18 Diogo S. Gorgulho , João G. Rosa

Whereas preheating after chaotic and hybrid inflation models has been abundantly studied in the literature, preheating in small field inflation models, where the curvature of the inflaton potential is negative during inflation, remains less…

高能物理 - 理论 · 物理学 2015-03-17 Philippe Brax , Jean-Francois Dufaux , Sophie Mariadassou

The phenomenon of resonant production of particles {\it after} inflation has received much attention in the past few years. In a new application of resonant production of particles, we consider the effect of a resonance {\em during}…

高能物理 - 唯象学 · 物理学 2009-10-31 Daniel J. H. Chung , Edward W. Kolb , Antonio Riotto , Igor I. Tkachev

Preheating after inflation proceeds through parametric resonance, leading to efficient particle production in scalar field models. In this work, we investigate the structure of parametric resonance in the $\phi^4$ chaotic inflationary model…

宇宙学与河外天体物理 · 物理学 2026-04-28 Hrisikesh Thakur , Malay K. Nandy

In inflationary cosmology, the particles constituting the Universe are created after inflation due to their interaction with moving inflaton field(s) in the process of preheating. In the fermionic sector, the leading channel is out-of…

高能物理 - 唯象学 · 物理学 2009-10-31 Patrick B. Greene , Lev Kofman

We investigate the particle production due to parametric resonances in model of inflation where the lightest composite state stemming from the minimal walking technicolor theory plays the role of the inflaton. For model of inflation, the…

高能物理 - 唯象学 · 物理学 2016-08-25 Phongpichit Channuie , Peeravit Koad

Certain inflation models undergo pre-heating, in which inflaton oscillations can drive parametric resonance instabilities. We discuss several phenomena stemming from such instabilities, especially in weak-scale models; generically, these…

高能物理 - 唯象学 · 物理学 2009-10-31 John M. Cornwall , Alexander Kusenko

We study the preheating process in a model of DBI inflation with a DBI-type inflaton coupling to a canonical entropy field. At the end of inflation, the inflaton field oscillates around its vacuum which can arise from an infrared cutoff…

高能物理 - 理论 · 物理学 2013-08-12 Jun Zhang , Yifu Cai , Yun-Song Piao

We report on the formation of a diverse family of transverse spatial polygon patterns in a microcavity polariton fluid under coherent driving by a blue-detuned pump. Patterns emerge spontaneously as a result of energy-degenerate…

In this paper I review the theory and numerical simulations of non-linear dynamics of preheating, a stage of dynamical instability at the end of inflation during which homogeneous inflaton explosively decays and deposits its energy into…

广义相对论与量子宇宙学 · 物理学 2015-03-14 Andrei V. Frolov

It is proposed that the spatial (and temporal) patterns spontaneously appearing in dissipative systems maximize the energy flow through the pattern forming interface. In other words - the patterns maximize the entropy growth rate in an…

适应与自组织系统 · 物理学 2007-05-23 Kestutis Staliunas
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