Tracing the nonlinear formation of an interfacial wave spectral cascade from one to few to many
Far-from-equilibrium phenomena unveil the intricate principles of complex systems, including snowflake growth and fluid turbulence, with broad applications ranging from foreign exchange trading to climate modeling. A recurring feature across these systems is the emergence of a spectral cascade, wher...
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Zusammenfassung: | Far-from-equilibrium phenomena unveil the intricate principles of complex
systems, including snowflake growth and fluid turbulence, with broad
applications ranging from foreign exchange trading to climate modeling. A
recurring feature across these systems is the emergence of a spectral cascade,
where energy is transferred across the system's length scales, following a
simple power law. The statistical theory of weak wave turbulence, in which only
leading order interactions are considered, successfully predicts scaling laws
for stationary states in idealised scenarios. Realistic conditions, such as
finite size and amplitude effects, and strong dissipation, remain beyond our
current understanding. Lacking comprehensive theoretical insight, we
experimentally trace the formation of a spectral cascade under these
conditions. Using an externally driven fluid-fluid interface, we successfully
resolve individual wave modes and track their real-time evolution from one to
few to many. This process culminates in a steady state whose power spectral
density is fully characterised by a power-law scaling. We further quantify
specific interactions through statistical correlations to reveal a hierarchy in
the wave-mixing order, thus confirming a key assumption of weak-wave
turbulence. We present a comprehensive time-evolution analysis that is crucial
in identifying critical points where the interface undergoes significant
changes. Our findings validate that the interfacial dynamics can be effectively
modelled using a weakly nonlinear Lagrangian theory, enabling us to explore its
applicability to other out-of-equilibrium systems. Notably, we uncover
intriguing connections to reheating scenarios following cosmic inflation in the
early universe. |
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DOI: | 10.48550/arxiv.2410.08842 |