pith:JVWUNYB7
Orbital stability of black solitons for quasilinear Schr\"odinger equations with nonzero conditions at infinity
The black soliton is orbitally stable in the energy space for quasilinear Schrödinger equations when the Vakhitov-Kolokolov slope condition holds.
arxiv:2605.13629 v1 · 2026-05-13 · math.AP
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Claims
Our main result is the orbital stability of the black soliton in the energy space, provided that the Vakhitov-Kolokolov (VK) slope condition holds; namely, that the derivative of the momentum with respect to the speed is negative at zero.
The analysis of minimizing sequences for the variational problem (infimum not attained) together with the sufficient conditions on the quasilinear nonlinearities that ensure existence of the local soliton branch parameterized by speed.
Black solitons are orbitally stable in the energy space when the derivative of momentum with respect to speed is negative at zero speed.
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| First computed | 2026-05-18T02:44:17.775090Z |
|---|---|
| Builder | pith-number-builder-2026-05-17-v1 |
| Signature | Pith Ed25519
(pith-v1-2026-05) · public key |
| Schema | pith-number/v1.0 |
Canonical hash
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Canonical record JSON
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