Existence of multi-pulses of the regularized short-pulse and Ostrovsky equations
Vahagn Manukian, Nick Costanzino, Christopher K.R.T. Jones, Bjorn, Sandstede

TL;DR
This paper proves the existence of multi-pulse solutions near orbit-flip bifurcations in singularly perturbed reversible systems, specifically applied to the regularized short-pulse and Ostrovsky equations, using geometric and analytical methods.
Contribution
It demonstrates the existence of multi-pulses in singularly perturbed systems near orbit-flip bifurcations, extending previous results to these specific equations.
Findings
Multi-pulses exist near orbit-flip bifurcations in the studied equations.
The sign of a geometric condition determines multi-pulse existence.
The methods combine geometric singular perturbation theory and Lyapunov--Schmidt reduction.
Abstract
The existence of multi-pulse solutions near orbit-flip bifurcations of a primary single-humped pulse is shown in reversible, conservative, singularly perturbed vector fields. Similar to the non-singular case, the sign of a geometric condition that involves the first integral decides whether multi-pulses exist or not. The proof utilizes a combination of geometric singular perturbation theory and Lyapunov--Schmidt reduction through Lin's method. The motivation for considering orbit flips in singularly perturbed systems comes from the regularized short-pulse equation and the Ostrovsky equation, which both fit into this framework and are shown here to support multi-pulses.
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