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Instability of converging shock waves and sonoluminescence

机译:会聚冲击波和声致发光的不稳定性

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摘要

We study the problem of the stability of a nearly spherical converging shock wave in a van der Waals gas and consider the implications for sonoluminescence. An approximate geometrical theory of shock propogation, due to Whitham [Linear and Non-linear Waves (Wiley, New York, 1974); J. Fluid. Mech. 2, 146 (1957); 5, 369 (1959)], is used. A first-order treatment of deviations from spherical symmetry, similar to one performed by Gardner, Brook, and Bernstein [J. Fluid. Mech. 114, 41 (1982)] for an ideal gas, shows that these deviations are unstable, coming to dominate the shape of a shock wave as it converges. The instability is weak, although not as weak as in an ideal gas. Perturbations grow as a small inverse power of the radius. The mechanism for concentration of energy in sonoluminescence involves a spherical converging shock. The validity of the theory given here is checked by comparing the results for spherically symmetric shocks with a simulation by Kondic, Gersten, and Yuan [Phys. Rev. E 52, 4976 (1995)]. We then estimate the degree of bubble symmetry necessary for sonoluminescence and relate this result to the experimental robustness of sonoluminescence.
机译:我们研究了范德华气体中近球形会聚冲击波的稳定性问题,并考虑了声致发光的意义。由于Whitham [线性和非线性波(Wiley,纽约,1974年); Whisham提出的近似的几何理论。 J.流体。机甲2,146(1957); 5,369(1959)]。与球形对称性偏差的一阶处理,类似于Gardner,Brook和Bernstein所进行的处理[J.体液。机甲[114,41(1982)]对理想气体的研究表明,这些偏差是不稳定的,并随着冲击波的收敛而支配了冲击波的形状。尽管不如理想气体中那样弱,但不稳定性很弱。扰动随着半径的反幂而增大。声致发光中的能量集中机制涉及球形会聚冲击。通过将球形对称冲击的结果与Kondic,Gersten和Yuan [Phys。 Rev 52,4976(1995)]。然后,我们估计声致发光所必需的气泡对称度,并将此结果与声致发光的实验鲁棒性相关联。

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