Key examples — free energy & phase equilibria
Where the chapter’s machinery shows up across the bookshelf.
Example 1: homogeneous nucleation of a vapour bubble
A pure liquid under tension is thermodynamically unstable — vapour is the lower-free-energy phase. But to nucleate a vapour bubble requires creating a liquid-vapour interface, costing , which dominates at small . The barrier for water at room temperature with realistic tensions () is hundreds of . The Boltzmann-weighted rate is so small that homogeneous nucleation is essentially forbidden — the cavitation puzzle of Cavitation Ch 1.3. The resolution is heterogeneous nucleation at pre-existing crevices, where the geometry reduces the effective surface area and barrier.
Example 2: heterogeneous nucleation at a crevice
If a small gas-filled crevice on a surface exists, the meniscus inside it has a much smaller surface-area cost than a free-floating bubble. The barrier scales as where is the contact angle — and for hydrophobic crevices () the barrier vanishes. This explains the gap between the in-principle tensile strength of water (, from the intermolecular-forces chapter spinodal) and the measured tensile strength (, governed by the worst crevice in your sample). See Cavitation Ch 2.2.
Example 3: vapour pressure inside an oscillating bubble
The pressure of vapour inside a Rayleigh–Plesset bubble depends on temperature, and the temperature depends on the polytropic compression of the gas inside. The Clausius–Clapeyron equation closes the loop: rises exponentially in temperature, so a small temperature change during compression produces a large vapour-pressure shift, which in turn affects the next bubble-wall acceleration. This positive-feedback between and is what drives the violent collapse phase of sonoluminescence. See Cavitation Ch 3.2.
Example 4: MET-channel mechanotransduction
The mechanically gated MET channels in hair-cell stereocilia switch between open and closed states under tip-link tension. With the open-vs-closed energy difference linear in tip-link displacement (), the open probability is exactly the Fermi function from the chapter:
Measured stereocilia data fit this sigmoid quantitatively. The width parameter matches the actual displacement range over which hair-cell responses go from near-zero to saturation. See Hearing Ch 4.6.
Example 5: spinodal as the in-principle tensile limit of water
If you compress a liquid below its equilibrium density (apply tension), the pressure becomes increasingly negative — until , the spinodal, where mechanical stability is lost and homogeneous nucleation becomes barrierless. For water using a Lennard-Jones-like potential (intermolecular-forces chapter), this spinodal pressure is — roughly 1000× atmospheric. This is the bound the free-energy curvature argument places on what a perfect bubble-free sample of water could withstand. Real samples fail orders of magnitude earlier.
Example 6: polytropic gas inside the bubble — Clausius–Clapeyron at work
The vapour pressure enters the bubble interior equation of state. Small temperature swings during oscillation drive proportionally larger swings in , and the resulting effective gas equation of state is neither isothermal nor adiabatic but intermediate-polytropic. The Cavitation book’s bubble-contents chapter uses this combined polytropic + Clausius–Clapeyron model.
Cross-book backlinks
- Cavitation Ch 2.1 — homogeneous nucleation: the barrier from this chapter, kinetic prefactor.
- Cavitation Ch 2.2 — heterogeneous nucleation & crevices: the same barrier with geometric corrections.
- Cavitation Ch 1.2 — tensile strength in principle: spinodal as free-energy curvature limit.
- Cavitation Ch 3.2 — bubble contents: Clausius–Clapeyron + polytropic gas.
- Hearing Ch 4.6 — hair-cell transduction: MET-channel Fermi function.