Connection between nonlinear energy optimization and instantons

Daniel Lecoanet and Rich R. Kerswell
Phys. Rev. E 97, 012212 – Published 18 January 2018

Abstract

How systems transit between different stable states under external perturbation is an important practical issue. We discuss here how a recently developed energy optimization method for identifying the minimal disturbance necessary to reach the basin boundary of a stable state is connected to the instanton trajectory from large deviation theory of noisy systems. In the context of the one-dimensional Swift–Hohenberg equation, which has multiple stable equilibria, we first show how the energy optimization method can be straightforwardly used to identify minimal disturbances—minimal seeds—for transition to specific attractors from the ground state. Then, after generalizing the technique to consider multiple, equally spaced-in-time perturbations, it is shown that the instanton trajectory is indeed the solution of the energy optimization method in the limit of infinitely many perturbations provided a specific norm is used to measure the set of discrete perturbations. Importantly, we find that the key features of the instanton can be captured by a low number of discrete perturbations (typically one perturbation per basin of attraction crossed). This suggests a promising new diagnostic for systems for which it may be impractical to calculate the instanton.

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  • Received 1 July 2017
  • Revised 10 December 2017

DOI:https://doi.org/10.1103/PhysRevE.97.012212

©2018 American Physical Society

Physics Subject Headings (PhySH)

  1. Research Areas
  1. Physical Systems
Nonlinear DynamicsFluid Dynamics

Authors & Affiliations

Daniel Lecoanet

  • Physics Department, University of California, Berkeley, California 94720, USA; Astronomy Department and Theoretical Astrophysics Center, University of California, Berkeley, California 94720, USA; Princeton Center for Theoretical Science, Princeton University, Princeton, New Jersey 08544, USA; Department of Astrophysical Sciences, Princeton University, Princeton, New Jersey 08544, USA; and Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA

Rich R. Kerswell

  • Centre for Mathematical Sciences, Cambridge University, Cambridge CB3 0WA, United Kingdom; School of Mathematics, University of Bristol, Bristol BS8 1TW, United Kingdom; and Kavli Institute for Theoretical Physics, University of California, Santa Barbara, California 93106, USA

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Vol. 97, Iss. 1 — January 2018

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