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The detection of sound begins when energy derived from an acoustic stimulus deflects the hair bundles on top of hair cells. As hair bundles move, the viscous friction between stereocilia and the surrounding liquid poses a fundamental physical challenge to the ear's high sensitivity and sharp frequency selectivity. Part of the solution to this problem lies in the active process that uses energy for frequency-selective sound amplification. Here we demonstrate that a complementary part of the solution involves the fluid-structure interaction between the liquid within the hair bundle and the stereocilia. Using force measurement on a dynamically scaled model, finite-element analysis, analytical estimation of hydrodynamic forces, stochastic simulation and high-resolution interferometric measurement of hair bundles, we characterize the origin and magnitude of the forces between individual stereocilia during small hair-bundle deflections. We find that the close apposition of stereocilia effectively immobilizes the liquid between them, which reduces the drag and suppresses the relative squeezing but not the sliding mode of stereociliary motion. The obliquely oriented tip links couple the mechanotransduction channels to this least dissipative coherent mode, whereas the elastic horizontal top connectors that stabilize the structure further reduce the drag. As measured from the distortion products associated with channel gating at physiological stimulation amplitudes of tens of nanometres, the balance of viscous and elastic forces in a hair bundle permits a relative mode of motion between adjacent stereocilia that encompasses only a fraction of a nanometre. A combination of high-resolution experiments and detailed numerical modelling of fluid-structure interactions reveals the physical principles behind the basic structural features of hair bundles and shows quantitatively how these organelles are adapted to the needs of sensitive mechanotransduction.  相似文献   
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Davier  JK 《世界科学》1989,11(1):14-15
对太阳系的探测表明,陨石撞击是行星表面的形成及日后演变的一个重要进程。例如,月亮表面满是陨痕累累的高地及低洼的、布满熔岩的盆地。遍布陨石坑的高地表明,最初的月球外壳及盆地是38亿年以前、月球形成最后阶段中所发生的巨大碰撞的结果。这些盆地是由直径为10~50公里的物体撞击出来的,后来,陨石坑为大熔岩所填充,就成了现在大家所熟知的平坦的玄武岩平原,即月球海。地球表面一定也曾发生过类似的碰撞。这些巨大的碰撞可能是地壳由早先的模样演变成现今海洋和大陆板  相似文献   
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