Periodic orbits of the ABC flow with A=B=C=1

Abstract

In this paper, we prove that the ODE system align* x &= z+ y\\ y &= x+ z\\ z &= y + x, align* whose right-hand side is the Arnold-Beltrami-Childress (ABC) flow with parameters A=B=C=1, has periodic orbits on (2π T)3 with rotation vectors parallel to (1,0,0), (0,1,0), and (0,0,1). An application of this result is that the well-known G-equation model for turbulent combustion with this ABC flow on R3 has a linear (i.e., maximal possible) flame speed enhancement rate as the amplitude of the flow grows.

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