Blake threshold radius

The temperature is higher than 5000 K for bubbles of 0.28 3.5 pm in ambient radius. For the linear resonance radius of 11 pm, it is only about 1000 K. In Fig. 1.9b, the rate of production of chemical species is shown. It is above 10s s 1 for bubbles of 0.28 8 pm in ambient radius. The minimum ambient radius coincides with the Blake threshold radius (Rgiake) f°r transient cavitation (active bubbles). It is calculated by the following formula [6]. 

Fig. 1.10 The Blake threshold pressure (1.17) and the linear resonance frequency (1.18) as a function of ambient radius...

The fact that the pressure is negative implies that a negative pressure must be applied to overcome the cohesive forces of a liquid and produce a bubble of radius R. Writing P] = Pjj — Pg allows the estimation of Pg, (known as Blake threshold pressure), which is the negative (or rarefaction) pressure which must be applied in excess of the hydrostatic pressure (Pj ) to create a bubble of radius R. e.g. for large bubbles (i.e. 2a/R, Ph)... 

The Blake threshold can be represented in an Apfel diagram (Fig. 10),56 where the horizontal axis represents the ratio [applied acoustic pressure]/[hydrostatic pressure], and the vertical axis, the ratio [bubble radius]/[resonance radius]. The resonance radius can be determined by the Minneart equation (see below). In zone A, the bubble cannot grow due to an insufficient quasi-static reduction of the acoustic pressure, and zone B is the zone of explosive growth. 

Equation 3 assumes that the external pressure (Po), the vapor pressure (Pv), the surface tension (ct), and the equilibrium radius of the huhhle (i o) determine the required negative pressure in the liquid to start an explosive growth of a cavity (13). The Blake threshold pressure is based on a static approach and is only valid when the surface tension dominates all dynamic effects, eg, mass transfer and viscosity. 

By combining the Rayleigh-Plesset equation with a mass and energy balance over the bubble, the temperature and pressure in the bubble can be calculated (16,17). The model also describes the dynamic movement of the bubble wall, which results in a calculated radius of the cavitation bubble as a fimction of time (see Fig. 2). The explosive growth phase and the collapse phase of the bubble can clearly be distinguished. Moreover, in case dynamic effects are more important than the surface tension, the cavitation threshold can be calculated with the dynamic model, while the Blake threshold pressure cannot be used at these conditions. 

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