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arXiv 2602.16043astro-ph.EP
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尘埃盘中的扩散不稳定性:线性增长与非线性崩溃

Diffusive Instabilities in Dusty Disks: Linear Growth and Nonlinear Breakdown

University of Chicago(芝加哥大学);Yale University(耶鲁大学);Academia Sinica(中央研究院);National Center for Theoretical Sciences(国家理论科学中心)

Konstantin Gerbig, Min-Kai Lin

AI总结:

研究尘埃盘中扩散不稳定性,发现线性增长和非线性崩溃机制,指出需额外物理实现真实非线性饱和。

摘要:

我们重新审视了尘埃盘中由于尘埃质量扩散性和/或粘性随着尘埃密度增加而足够陡峭地减小时出现的扩散不稳定性。我们的更新模型包括一个不可压缩、粘性气体,其在方位角上响应并通过拖拽与尘埃耦合。我们表明,对于小的尘埃停止时间,扩散斜率驱动不稳定的基准则仍近似为β_diff ≲ -2,气体反馈仅对受流体不稳定性湍流激发的参数产生适度的定量变化。我们进行了非线性数值计算,并确认了线性增长和向最快增长波数选择的模式选择。然而,对于幂律闭合D∝Σ^{β_diff},当β_diff<0时,非线性演化不会饱和。相反,梯度的陡峭化会放大非线性尘埃压力项并驱动有限时间崩溃,形成越来越尖锐的尖峰。受我们一维框架中缺乏多维饱和通道的启发,我们测试了一个简单的分段闭合,其中负扩散斜率仅在有限的密度区间内操作。这种修改消除了爆炸并产生了受施加饱和尺度控制的峰值密度。我们的结果支持扩散不稳定性作为尘埃湍流中线性组织机制,同时强调现实的非线性饱和需要超越当前闭合的额外物理。

英文摘要:

We revisit the diffusive instability in dusty disks that arises when the dust mass diffusivity and/or viscosity decreases sufficiently steeply with increasing dust density. Our updated model includes an incompressible, viscous gas that responds azimuthally and couples to the dust through drag. We show that the basic criterion for diffusion-slope-driven instability remains approximately $β_\mathrm{diff}\lesssim -2$ for small dust stopping times, with gas feedback providing only modest quantitative changes for parameters motivated by streaming-instability turbulence. We perform nonlinear numerical calculations and confirm linear growth and mode selection toward the fastest-growing wavenumber. However, for power-law closures $D\proptoΣ^{β_\mathrm{diff}}$ with $β_\mathrm{diff}<0$, the nonlinear evolution does not saturate. Instead, steepening gradients amplify the nonlinear dust-pressure term and drive finite-time collapse into increasingly sharp spikes. Motivated by the absence of multidimensional saturation channels in our 1D framework, we test a simple piecewise closure in which the negative diffusion slope operates only over a finite density interval. This modification eliminates blowup and produces peak densities controlled by the imposed saturation scale. Our results support diffusive instabilities as a linear organizing mechanism in dusty turbulence, while highlighting that realistic nonlinear saturation requires additional physics beyond the present closure.

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