scholarly journals Mathematical analysis of memory effects and thermal relaxation in nonlinear sound waves on unbounded domains

2021 ◽  
Vol 273 ◽  
pp. 172-218
Author(s):  
Vanja Nikolić ◽  
Belkacem Said-Houari
1981 ◽  
Vol 36 (7) ◽  
pp. 713-717
Author(s):  
Peter Križan ◽  
Ivan Kuščer

Abstract flu e n c e o f A d s o r p tio n u p o n S o u n d A t te n u a tio n in a T u b e * Sound waves propagating in a tube filled with gas are attenuated because of absorption in bulk, because of viscothermal effects, and possibly because the gas is adsorbed upon the wall. The latter effect is shown to depend upon a thermal relaxation time, the near-equilibrium desorption rate, and a phenomenological coefficient containing the sticking probability. In case of multilayer adsorption, especially upon metals, this data could be deduced from measurements of sound attenuation. An early experiment by Maurer is discussed in this light.


Previous experiments have shown that at low temperatures the acoustic impedance of liquid 3 He under the saturated vapour pressure rises by about 10% below about 0.092 °K. This rise is predicted by Landau’s theory of a Fermi liquid. It comes about because, at sufficiently low temperatures, sound waves in liquid 3 He are propagated as a new mode, the so-called zero sound. The present experiments study the dependence on pressure of the temperature and magnitude of the transition in the impedance. The transition temperature is shifted from 0.092 to about 0.07 °K on subjecting the liquid to a pressure of 12.5 atm, and the magnitude of the change considerably reduced. To interpret these results, measurements have also been made of the viscosity as a function of pressure. (These give information about the thermal relaxation times in the liquid.) All the results are in accord with the theory of zero sound in a Fermi liquid.


1967 ◽  
Vol 31 ◽  
pp. 313-317 ◽  
Author(s):  
C. C. Lin ◽  
F. H. Shu

Density waves in the nature of those proposed by B. Lindblad are described by detailed mathematical analysis of collective modes in a disk-like stellar system. The treatment is centered around a hypothesis of quasi-stationary spiral structure. We examine (a) the mechanism for the maintenance of this spiral pattern, and (b) its consequences on the observable features of the galaxy.


Author(s):  
Tim Oliver ◽  
Akira Ishihara ◽  
Ken Jacobsen ◽  
Micah Dembo

In order to better understand the distribution of cell traction forces generated by rapidly locomoting cells, we have applied a mathematical analysis to our modified silicone rubber traction assay, based on the plane stress Green’s function of linear elasticity. To achieve this, we made crosslinked silicone rubber films into which we incorporated many more latex beads than previously possible (Figs. 1 and 6), using a modified airbrush. These films could be deformed by fish keratocytes, were virtually drift-free, and showed better than a 90% elastic recovery to micromanipulation (data not shown). Video images of cells locomoting on these films were recorded. From a pair of images representing the undisturbed and stressed states of the film, we recorded the cell’s outline and the associated displacements of bead centroids using Image-1 (Fig. 1). Next, using our own software, a mesh of quadrilaterals was plotted (Fig. 2) to represent the cell outline and to superimpose on the outline a traction density distribution. The net displacement of each bead in the film was calculated from centroid data and displayed with the mesh outline (Fig. 3).


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