Recalculate Figure 1 of Thiele 2010
Open the author-hosted published article at section 2, equation (5) and Figure 1. Locate zero wavenumber, the crossing and the maximum. They mark mass conservation, the stability boundary and the fastest mode. The stable branch remains below zero.
Define and divide growth by . The unstable branch becomes a universal dimensionless curve for this linear model. At , its values are . These are newly calculated formula values, not digitized source points.
- Unstable film
- Stable film (separate rate scale)
Sources: U. Thiele
Why the thread relation has another time scale
Open the later repository copy of Eggers–Dupont’s 1994 paper, arXiv:physics/0110081v1. Section 2, equation (27), is quadratic in growth rate; equation (28) supplies its growing branch. Equations (30) and (31) check low- and high-viscosity limits. Retaining inertia requires an evolving velocity, unlike the overdamped film.
Use and . At zero Ohnesorge number, the reduced model selects , or wavelength . The paper contrasts this with about for the full inviscid cylinder. Even a successful reduced equation has approximation error.
Figure 1 instead compares nozzle-fed water-jet shapes at . Reproducing it requires inlet conditions, jet speed and alignment with photographs. The periodic experiment here tests equation (27); the nozzle figure is a separate reading task.
Sources: Eggers & Dupont
Figure 4 of Zhang 2024 shows spectra
Open arXiv:2406.08179v1 and its published counterpart, JFM 996, A19. Section 2 derives a stochastic strong-slip equation; section 4 explains the molecular wall model. Figure 3 calibrates slip using pressure-driven velocity profiles before the dewetting comparison.
Figure 4 fixes thickness at and compares slip lengths and . Symbols are root-mean-square height spectra from 40 independent molecular simulations. Lines are stochastic continuum predictions. A time-dependent spectrum is a different observable from the deterministic growth rate in Chapter 3.
Panel (a) also compares predictions with and without inertia. Strong slip changes the leading flow balance, making the inertial terms relevant for these conditions. The question becomes which velocity and noise model predicts the observed spectrum.
Sources: Yixin Zhang
Turn the next extension into a testable question
A first extension can remain deterministic: hold wetting energy, mean thickness and the continuous initial profile fixed, change the wall condition, and derive its appropriate flux. Compare early spectra and energy before adding thermal fluctuations. Strong slip also requires reconsidering inertia and long-wave scaling.
Continuous thermal forcing requires a stochastic flux, a fluctuation–dissipation relation and independent realizations. Random initial heights supply only one initial disturbance. Continuing through rupture additionally needs a treatment of changing topology; molecular calculations need independently checked interactions, system sizes and sampling errors.
For the next paper, write down geometry, conserved quantity, wall conditions, observable and averaging procedure before comparing curves. These choices turn an appealing figure into a calculation someone else can repeat.
Sources: Yixin Zhang · Eggers & Dupont