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Exact diffusion coefficient of self-gravitating Brownian particles in two dimensions

机译:二维自重布朗粒子的精确扩散系数

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摘要

We derive the exact expression of the diffusion coefficient of a self-gravitating Brownian gas in two dimensions. Our formula generalizes the usual Einstein relation for a free Brownian motion to the context of two-dimensional gravity. We show the existence of a critical temperature T-c at which the diffusion coefficient vanishes. For T < T-c, the diffusion coefficient is negative and the gas undergoes gravitational collapse. This leads to the formation of a Dirac peak concentrating the whole mass in a finite time. We also stress that the critical temperature T-c is different from the collapse temperature T-* at which the partition function diverges. These quantities differ by a factor 1-1/N where N is the number of particles in the system. We provide clear evidence of this difference by explicitly solving the case N = 2. We also mention the analogy with the chemotactic aggregation of bacteria in biology, the formation of "atoms" in a two-dimensional (2D) plasma and the formation of dipoles or "supervortices" in 2D point vortex dynamics.
机译:我们在二维中得出了自重布朗气体的扩散系数的精确表达式。我们的公式概括了自由布朗运动对二维重力上下文的通常爱因斯坦关系。我们显示了扩散系数消失的临界温度T-c的存在。对于T

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