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Asymptotic self-similar blow-up profile for three-dimensional axisymmetric Euler equations using neural networks
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Whether there exist finite time blow-up solutions for the 2-D Boussinesq and the 3-D Euler equations are of fundamental importance to the field of fluid mechanics. We develop a new numerical framework, employing physics-informed neural networks (PINNs), that discover, for the first time, a smooth self-similar blow-up profile for both equations. The solution itself could form the basis of a future computer-assisted proof of blow-up for both equations. In addition, we demonstrate PINNs could be successfully applied to find unstable self-similar solutions to fluid equations by constructing the first example of an unstable self-similar solution to the C\'ordoba-C\'ordoba-Fontelos equation. We show that our numerical framework is both robust and adaptable to various other equations.
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The spectral picture of self-similar collapse in the Constantin-Lax-Majda equation
On the origin-H2 realization, the CLM collapse linearization has essential spectrum Re λ = -1/2 and point spectrum {0,1}, hence a spectral gap 1/2; weaker L2 realizations fill the whole strip.
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