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arXiv 2602.07972astro-ph.COgr-qchep-th
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变形吸引子模型中的自共振预热:振子的形成与演化

Self-resonance preheating in deformed attractor models: oscillon formation and evolution

Nanchang University(南昌大学);Lanzhou University(兰州大学)

Bao-Min Gu, Yu-Peng Zhang, Fu-Wen Shu, Yu-Xiao Liu

AI总结:

研究变形α吸引子T模型中自共振预热过程,发现振子形成与演化受潜在特征参数影响,揭示了潜在特征在预热动态和宇宙学影响中的重要作用。

摘要:

在近最小值处二次但远离最小值处更浅的势中,如小α(<<M_P^2)吸引子,自共振预热期间暴涨凝聚物会分裂成局部紧凑物体,即振子。本文研究了变形α-吸引子T模型中自共振现象,该模型在最小值附近具有高斯特征,远离膨胀结束点。线性分析显示共振带和变形Floquet图随特征参数变化而改变。在非线性晶格模拟中,发现梯度能量转移与潜在特征参数h无关,但共振终止后梯度能量演化强烈依赖于h。统计分析显示具有潜在特征的模型产生更多较小振子,这些物体中储存的能量减少,随着h增大而被抑制。通过追踪振子中的总能量和梯度能量,发现非零h模型中振子寿命更短,h越大影响越显著。引力波发射主要由共振阶段主导,一旦振子形成则被强烈抑制。潜在特征使低频谱基本不变,但显著改变高频尾部。尽管完全再加热描述需要外部耦合和更高分辨率模拟,但我们的模拟时间窗口内已出现明显的宇宙膨胀历史差异。这些结果突显了潜在特征在塑造再加热动态和宇宙学影响中的重要作用,并加深了对预热动态和振子性质的理解。

英文摘要:

It is well known that, in potentials that are quadratic near the minimum but shallower away, such as small-$α$ ($α\ll M_P^2$) attractors, the inflaton condensate fragments into localized compact objects known as oscillons during self-resonance preheating. In this work, we investigate self-resonance in a deformed $α$-attractor T-model with a Gaussian feature near the minimum, distant from the end of inflation. Linear analysis reveals altered resonance bands and deformed Floquet charts dependent on feature parameters, primarily through the localized modification of $V''(ϕ)$. In fully nonlinear lattice simulations, we find that the potential feature has only a modest influence on gradient-energy transfer during resonance, whereas the subsequent evolution becomes strongly dependent on the Gaussian feature's dimensionless amplitude $h$. Increasing $|h|$ suppresses the formation and persistence of compact oscillons, resulting in fewer objects and a smaller fraction of energy stored in them. The total-energy and internal-gradient-energy diagnostics give consistent lifetime trends. Within the directly resolved range, the oscillon lifetime decreases nonlinearly with increasing $|h|$, with negative $h$ generally producing shorter lifetimes than positive $h$ of the same magnitude. The gravitational wave emission is dominated by the resonant stage and becomes strongly suppressed after oscillon formation. We further find an enhancement in the high-frequency tail of the spectrum, sourced by the potential feature. Although a complete reheating description requires external couplings and higher-resolution simulations, clear qualitative differences in the post-inflationary expansion history already emerge within our simulated time window. These results clarify how potential features affect preheating dynamics and oscillon evolution.

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