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LINEAR/NONLINEAR ACOUSTIC WAVE PROPAGATION THROUGH IDEAL FLUID WITH INCLUSION BY LIU GANG (B.Eng, Civil Engineering, Harbin Engineering University, July, 2003) (Ph.D, Solid Mechanics, Harbin Engineering University, July, 2007) A THESIS SUBMITTED FOR THE DEGREE OF MASTER OF ENGINEERING DEPARTMENT OF MECHANICAL ENGINEERING NATIONAL UNIVERSITY OF SINGAPORE 2011 Acknowledgements I wish to express my deep gratitude and sincere appreciation to my supervisor, Professor Khoo Boo Cheong, from the Department of Mechanical Engineering, NUS, for his inspiration, support and guidance throughout my research and study. His broad knowledge in many fields, priceless advices, and patience have played a significant role in completing this work successfully. I also wish to extend my sincere thanks to Dr. Pahala Gedara Jayathilake, from the Department of Mechanical Engineering, NUS, for the discussion on life and research issues. Special thanks are given to Mr. Karri Badarinath, Mr. Deepal Kanti Das, Mr. Chen Yu, Ms. Wang Li Ping, Ms. Shao Jiang Yan, from Fluid Laboratory, who shared their precious experience in life and offered generous support in my study at NUS. Finally, I would like to express my gratitude to the National University of Singapore for offering me the opportunity to study, and providing all the necessary resources and facilities for the research work. National University of Singapore September, 2011 Liu Gang i Table of Contents Acknowledgements i Table of Contents ii Summary iv List of Figures vii Chapter 1 IntroductionEquation Chapter 1 Section 1Equation Section 1 1 1.1 Problem Definition, Motivation and Scope of Present Work 1 1.2 Outline of contents 7 Chapter 2 Mathematical FormulationEquation Chapter 2 Section 1Equation Chapter 2 Section 1Equation Section (Next) 2.1 Conformal transformation 2.2 On Perturbation Method Chapter 3 Linear Acoustic Wave Scattering by Two Dimensional Scatterer with Irregular Shape in an Ideal FluidEquation Section (Next) 3.1 Governing equations of linear acoustic wave 8 8 14 22 22 3.2 Conformal transformations of Helmholtz equation and corresponding physical vector 24 3.3 Acoustic wave scattering by object with irregular across section 31 3.4 Results and Analysis 36 3.5 Conclusions 45 Chapter 4 An Analysis on the Second-order Nonlinear Effect of Focused Acoustic Wave Around a Scatterer in an Ideal FluidEquation Section (Next) 46 4.1 Second order nonlinear solution for Westervelt equation 46 4.2 Perturbative method with small parameter for the nonlinear acoustic wave 50 4.2.1 Mathematical formulation of the nonlinear acoustic wave 50 4.2.2 Non-dimensional formulation of the governing equations 53 4.3 Analytical solution for the one-dimensionless equation 56 4.3.1 Analytical solution for plane wave 56 4.3.2 Analytical solution for cylindrical wave 56 4.3.3 Analytical solution for spherical wave 56 4.4 Results and Discussions 57 4.5 Conclusions 67 Chapter 5 Overall Conclusions and Recommendations 5.1 Conclusions 68 68 ii 5.2 Recommendations 70 Bibliography 71 Appendix A 80 Partial Coding for Linear Acoustic Wave Propagation Relate to Conformal Mapping Method 80 Code 1: 80 Code 2: 80 Code 3: 81 Code 4 84 Appendix B 87 Analytical Solution for Plane wave 88 Analytical Solution for Cylindrical Wave 88 Analytical Solution for Spherical Wave 89 Appendix C 92 Analytical Solution for Plane Wave 92 Analytical Solution for Cylindrical Wave 93 Analytical Solution for Spherical Wave 94 Appendix D Partial Coding for the Nonlinear Acoustic Wave Propagation 97 97 Code 1: 97 Code 2: 98 Code 3: 99 Appendix E 101 iii Summary This work proposed several analytical model for the linear/nonlinear acoustic wave propagating through the ideal fluid with inclusion embedded. The conformal mapping together with the complex variables method were applied to solve the linear acoustic wave scattering by irregular shaped inclusion. Subsequently, we use the perturbation method to analytically solve the nonlinear acoustic wave interact with the regular shaped inclusion by expand the nonlinear governing equation into linear homogeneous/non-homogeneous equations. In general, these two methods are versatile to obtain the analytical solutions for two classes of problems: the linear problems with complex boundary conditions and the nonlinear problem with more complex governing equations. For the linear model, we analytically obtained the two dimensional general solution of Helmholtz equation, shown as Bessel function with mapping function as the argument and fractional order Bessel function, to study the linear acoustic wave scattering by rigid inclusion with irregular cross section in an ideal fluid. Based on the conformal mapping method together with the complex variables method, we can map the initial geometry into a circular shape as well as transform the original physical vector into corresponding new expressions in the mapping plane. This study may provide the basis for further analyses of other conditions of acoustic wave scattering in fluids, e.g. irregular elastic inclusion within fluid with viscosity, etc. Our calculated results have shown that the angle and frequency of the incident waves have significant iv influence on the bistatic scattering pattern as well as the far field form factor for the pressure in the fluid. Moreover, we have shown that the sharper corners of the irregular inclusion may amplify the bistatic scattering pattern compared with the more rounded corners. For the part of nonlinear acoustic wave propagation, we adopted two nonlinear models to investigate the multiple incident acoustic waves focused on certain domain where the nonlinear effect is not negligible in the vicinity of the scatterer. The general solutions for the one dimensional Westervelt equation with different coordinates (plane, cylindrical and spherical) are analytically obtained based on the perturbation method with keeping only the second order nonlinear terms. Separately, introducing the small parameter (Mach number), we applied the compressible potential flow theory and proposed a dimensionless formulation and asymptotic perturbation expansion for the velocity potential and enthalpy which is different from the existing (and more traditional) fractional nonlinear acoustic models (eg. the Burgers equation, KZK equation and Westervelt equation). Our analytical solutions and numerical calculations have shown the general tendency of the velocity potential and pressure to decrease w.r.t. the increase of the distance away from the focused point. At least, within the region which is about 10 times the radius of the scatterer, the non-linear effect exerts a significant influence on the distribution of the pressure and velocity potential. It is also interesting that at high frequencies, lower Mach numbers appear to bring out even stronger nonlinear effects for the spherical wave. Our approach with small parameter for the cylindrical and spherical waves could serve as an effective v analytical model to simulate the focused nonlinear acoustic near the scatterer in an ideal fluid and be applied to study bubble cavitation dynamic associated with HIFU in our future work. vi List of Figures Figure 2.1: Illustration of the conformal mapping that transforms the initial irregular geometry into a circular one 8 Figure 3.1: The model for scattering of acoustic wave by rigid inclusion with irregular across section 25 Figure 3.2: Illustration of the conformal mapping that transforms the initial irregular geometry into a circular one 26 Figure 3.3: The geometry for the canonical ellipse based on the mapping function w    R   p  q  , where r  1.0, R  0.75, p  1/3, q  1.0 37 Figure 3.4: The comparison of the present method with the T-matrix method at 2:1 aspect ratio ellipse for bistatic scattering pattern at (a) kr  2.0 and (b) kr  5.0 38 Figure 3.5: The comparison of the present method with the Fourier matching method at 2:1 aspect ratio ellipse for the far-field form function Figure 3.6: The geometries for the scatterer 38 based on the mapping function w    R   p  q  , where r  1.3, R  0.7 and q  1 p  1.0 (ellipse), 2.0 (leaf clover) and 3.0 (rounded corner square) 39 Figure 3.7: The far field form function for the acoustic wave scattering by ellipse cross section w    R   p  q  , where r  1.3, R  0.7, and q  1 p  1.0(a), 2.0(b) and 3.0(c) 40 vii Figure 3.8: The bistatic scattering pattern for the model of slender ellipse, leaf clover and approximate square at kr  2.0 and 5.0 42 Figure 3.9: The geometries for the scatterer based on the mapping function w      c1  n  c2  2 n 1  c3  3n  2 with n  2 43 Figure 3.10: The bistatic scattering pattern for the scatterer with n-fold axes of symmetry and sharp corners at kr  2.0 44 Figure 4.1: Schematic description of the model for multiple acoustic waves focused around a scatterer inside an ideal fluid 47 Figure 4.2: The ratio of the pressure second harmonic to the fundamental term v.s. the variation of the distance away from the focused point 58 Figure 4.3: The comparison between the analytical results of planar, cylindrical and spherical wave including the fundamental and the second harmonic 59 Figure 4.4: The variation of pressure amplitude v.s. the distance away from the focused point for the planar, cylindrical and spherical wave 60 Figure 4.5: The variation of the second order term of plane wave v.s. the variation of wave number k , Mach number  and the distance away from the focused point 62 Figure 4.6: The variation of the second order term for cylindrical wave v.s. the different wave number, Mach number and the distance away from the focused point63 Figure 4.7: The variation of the second order term for spherical wave v.s. the different wave number, Mach number and the distance away from the focused point 64 viii Figure 4.8: The velocity potential distribution near the scatterer (the summation of the first order term and the second order term) at k  2.0 and   0.3 65 ix Chapter 1 Introduction 1.1 Problem Definition, Motivation and Scope of Present Work A better understanding of the physics of linear/nonlinear acoustic wave interact with inclusion is important for a wide range of applications including underwater detection, biomedical and chemical processes. On the aspect of linear acoustic wave, considerable work has been done on the scattering by objects having regular cross section. For instance, the separation of variables approach for the Helmholtz equation has been shown for some particular shapes (Mclachlan 1954). For the two dimensional problem, however, only the cross sections of the inclusion which are circular (Liu et al. 2009; Liu et al. 2008), elliptic (Leon et al. 2004a) or parabolic in shape can be applied using this method. Apart from the separation of variables approach, there are other methods most of which are limited to certain class of surfaces. An analytical approach that is formally exact is the perturbation method (Skaropoulos & Chrissoulidis 2003; Yeh 1965). This may be used for the penetrable or impenetrable boundary conditions, but is only valid if the shape is close to one of the limited geometries employed in the above mentioned separation of variable approach. Mathematically, an alternative method named conformal mapping via the complex variables methods (Muskhelishvili 1975) has been applied to study these kinds of problems. These complex variable methods are 1 proved to be rather versatile and have been used not only for linear elastostatic problem involving cavities (Savin 1961), but also be used in, for example, thermopiezoelectric problems involving cavities (Qin et al. 1999), compressibility/shear compliance of pores having n-fold axes symmetry (Ekneligoda & Zimmerman 2006; Ekneligoda & Zimmerman 2008) and others. On the elastodynamic model, conformal mapping was applied to solve the in-plane elastic wave propagation through the infinite domain with irregular-shaped cavity and dynamic stress concentration (Liu et al. 1982), the anti-plane shear wave propagation via mapping into the Cartesian coordinates (Han & Liu 1997; Liu & Han 1991) and the anti-plane shear wave propagation via mapping of the inner/outer domain into polar coordinates for ellipse (Cao et al. 2001; Liu & Chen 2004). Separately, Fourier Matching Method (FFM) has been proposed which also involved mapping to study the sound scattering by cylinders of noncircular cross sections (Diperna & Stanton 1994), the non-Laplacian growth phenomena (Bazant et al. 2003), as well as on reinforcement layer bonded to an elliptic hole under a remote static uniform load (Chao et al. 2009). In order to solve the linear wave interaction problems with various surface that is not close to a geometry amendable to separation of variable approach, one may still need to resort to numerical technique. In general, the study of wave scattering by non-circular shaped object by numerical methods can be broadly classified into three groups: those concerned with elliptical cylinders based on expansions in Mathieu functions (Barakat 1963; Sato 1975), those based on the null field method for which 2 any noncircular cylindrical geometries can be considered (Raddlinski & Simon 1993), and those using Green’s function approach to obtain a governing Fredholm integral equation (Veksler et al. 1999). There are some numerical methods which are formally exact have been developed; those include the Mode Matching Method (Ikuno & Yasuura 1978), the T-matrix Method (Lakhtakia et al. 1984), the Boundary Element Method (Tobocman 1984; Yang 2002), as well as the Discontinuous Galerkin Methods (Feng & Wu 2009). On the aspect of engineering applications, the problems refer to linear sound wave scattering from inclusions have been the subject of several studies usually carried out either numerically or experimentally. For instance, the response of cylinder with circular cross section in water (Billy 1986; Faran 1951; Mitri 2010a; Rembert et al. 1992), and wave scattering from spherical bubble/shell (Chen et al. 2009; Doinikov & Bouakaz 2010; Mitri 2005). On the other hand, the theoretical aspect of acoustic study on inclusion with arbitrary cross sections in fluids are far fewer. Our proposed method is an attempt to meet the need for various geometries and extend the classical conformal mapping within the framework of complex variable methods for the acoustic wave scattering problem in fluids. Incorporation of the mapping technique into the scattering formulation allows one to analytically predict the far-field (scattered) pressure results for penetrable or impenetrable scatterers. In contrast to other methods, we only need to define the mapping functions for our approach, by which we can transform the initial different geometries into a circular one accordingly, together with the fractional order Bessel function (Liu et al. 3 2010) to satisfy the boundary conditions for other part of the geometry with regular curve. Next, the general formation of the scattered wave can be obtained and only the unknown coefficients need to be determined according to the different boundary conditions. The distinct advantages of our proposed approach based on conformal mapping with complex variables can be summarized as: (i) we can directly employ the scheme according to the method of separation of variables via the argument of the Bessel function for different curvilinear configurations in conjunction with the selected mapping functions, see (Liu et al. 1982) for example. (ii) It is very expedient for our method vis-à-vis some other numerical methods which need to discretize the full domain, especially the regions at those nodes on the boundaries to accommodate irregular curve. This leads to potential vast savings of computational resources and memory. Our approach is possibly one of the first few to calculate the linear acoustic wave scattering of noncircular cylinders with the use of conformal mapping within the context of the complex variables method in the fluid. The results obtained are validated against some special cases available in the literature, and then the effect of different geometries of the solid inclusion with sharp corners is studied. (It may also be remarked that our approach is based on the Schwarz-Christoffel mapping function with the first two and three terms for irregular polygons (Ekneligoda & Zimmerman 2006; Ekneligoda & Zimmerman 2008)). As is well known, linear acoustic theory is based on the assumption of small amplitude waves and linear constitutive theory of the fluid medium (Whitham 1974). Although these assumptions hold for many vibro-acoustic interactions, they become 4 inapplicable in sound fields with high amplitude pressure(Walsh & Torres 2007). Unlike the linear acoustic wave equation, the nonlinear counterpart can handle waves with large finite amplitudes, and allow accurate modeling of nonlinear constitutive models in the fluid. Interesting phenomena unknown in linear acoustics can be observed, for example, waveform distortion, formation of shock waves, increased absorption, nonlinear interaction (as opposed to superposition) when two sound waves are mixed, amplitude dependent directivity of acoustic beams, cavitation and sonoluminescence (Crocker 1998). As far as we are aware, there are various models to simulate the nonlinear characteristic of the acoustic wave propagating through the fluid. For instance, the one-dimensional Burgers equation has been found to be an excellent approximation of the conservation equations for plane progressive waves of finite amplitude in a thermoviscous fluid (Blackstock 1985). An effective model that combined effects of diffraction, absorption, and nonlinearity in directional sound beams (i.e. radiated from sources with dimensions that are large compared with the characteristic wavelength) are taken into account by the Khokhlov-Zabolotskaya-Kuznestov (KZK) parabolic wave equation (Bessonova & Khokhlova 2009; Liu et al. 2006). Several additional models have been developed, usually in response to specific needs. For example, the Westervelt equation is an almost incidental product of Westervelt’s discovery of the parametric arrays (Kim & Yoon 2009; Norton & Purrington 2009; Sun et al. 2006). In the past, much computational work have been done on nonlinear effects in beams based on the KZK equations(Kamakura 2004; Kamakura et al. 2004; Lee & 5 Hamilton 1995; Tjotta et al. 1990). The one dimensional case of Westervelt equation is studied extensively by finite element method (Pozuelo et al. 1999). However, when acoustic fields of more complex conditions are considered, advanced numerical calculation related to finite-differential becomes necessary (Vanhille & Pozuelo 2001; Vanhille & Pozuelo 2004). In this work, our interest is to develop an analytical solution of the multiple harmonic acoustic waves focused on the area near a scatterer where the second order nonlinear effect dominates. Our study has important implications for further work on bubble/nucleation cavitation by HIFU (high intensity focused ultrasound) and others. 6 1.2 Outline of contents This dissertation is divided into five chapters. Each of them consists of various subsections. A brief summary for each chapter is given as follows. In Chapter 1 (Introduction), the motivation and scopes of the present work are presented. There is a brief presentation on the background of linear/nonlinear acoustic wave propagation, in which attention is centered on using conformal mapping method for linear acoustic wave scattering by the inclusion with irregular across section and perturbation method for the nonlinear acoustic wave propagation. In Chapter 2, we outline the mathematical background for the conformal mapping method and perturbation method. In Chapter 3, the basic theory of conformal mapping is reiterated with sufficient details required for the development of the following section. Here, we present some results of our method for comparison with other methods in term of accuracy and efficiency. In Chapter 4, the mathematical background for the perturbation method is presented. Discussion on the second order nonlinearity shows clearly the nonlinear effect for acoustic wave propagation. Numerical results for several examples are presented to give the explicit comparison with linear condition. Finally, conclusions are drawn and the directions for future work are discussed in Chapter 5. 7 Chapter 2 Mathematical Formulation 2.1 Conformal transformation In this part, we will recall the basic properties of conformal transformation. A more detailed introduction of the relevant theoretical problems and the application to the mathematical theory of elasticity can be found in I.I. Privalov’s (Privalov 1948) or in the book of (Lavrentjev 1946) and Chapter 7 in (Muskhelishvili 1975). Assume  and  be two complex variables such that   w   , (2.1) b a      Medium I  Medium II Medium II Medium I Figure 2.1: Illustration of the conformal mapping that transforms the initial irregular geometry into a circular one where w   is a single valued analytic function in the region  in the   plane. The equation (2.1) establishes the relation of every point  in  to some definite point  in the   plane. Conversely, we can assume that each point  of  in Eq.(2.1), corresponds to a definite point in  . Consequently, we can said that Eq.(2.1) determines an invertible single-valued conformal transformation or conformal mapping of the region  into the region  (or conversely). In the sequel, when we 8 discuss about conformal transformation, it is always assumed to be reversible and single valued. The transformation is called conformal, because of the following property which is characteristic for relations of the form (2.1), where w   is a holomorphic function. In other words, if in  two linear elements be taken which extend from some point  and form between them an angle  , the corresponding elements in  will form the same angle  and the sense of the angle will be maintained which is the basic definition of conformal mapping (as also shown in Chapter 11 of (Chiang 1997)). Without special notification, the regions will be assumed to be rounded by one or several simple contours. The region  and  may be finite or infinite (one of them may be finite, while the other is infinite). If the region  is finite and  is infinite, the function w   must become infinite at some point of  (as otherwise there would not be some point of  corresponding to the point at infinity in  ). It is easily proved that w   must have a simple pole at that point, i.e. assuming for simplicity that    corresponds to   0 , then w    c   a holomorphic function, (2.2) where c is a constant and no singularities will occur inside the domain of  ; otherwise the transformation can not be deemed as reversible and single-valued. If  and  are both infinite and the points at infinity correspond to each other, the function w   must for the same reason have the form 9 w    R  a holomorphic function, (2.3) where R is a constant. It can be recalled that a function, holomorphic in an infinite region, is understood to be one which is holomorphic in any finite part of this region and which for sufficiently large c0  c1  c2  2  ... .  may be represented by a series as Further, it may be shown that the derivative w   cannot become zero in  ; otherwise the transformation would not be reversible and single valued. There also arises the following question: if two arbitrary regions  and  be given, is it always possible to find a function w   such that (2.1) gives a transformation of  into  ? Here, only some general remarks will be made. First of all, it is obviously impossible to obtain a (reversible and single-valued) transformation of a simply connected region into a multiply connected one. Consider the case when the two regions are simply connected and bounded by simple contours. Then the relationship as shown in form (2.1), mapping one region onto the other, can always be found and the function will be continuous up to the contours. In addition, the function w   may always be chosen so that an arbitrary given point 0 of  corresponds to an arbitrary given point  0 of  and that the directions of arbitrarily chosen linear elements, passing through 0 and  0 , correspond. These supplementary conditions will fully determine the function w   . For simplicity, suppose that  is the unit circle with its centre at the origin. Denote the circumference of the circle by  , so that one has on    1 . Since the 10 transformation is to be continuous up to the contours, the function w   will be continuous on  from the left (taking the anti-clockwise direction as positive); let its boundary values be denoted by w   , where   ei is a point of  . Hereby, the behavior of the derivative w   near and on  will be interesting; in particular, the question has to be considered whether w   vanishes at any point of the contour. If the coordinates of the points of the contour of  have continuous derivatives up to the second order along the arc (i.e. if the curvature of the contour changes continuously), the function w   is continuous up to  and, denoting its boundary values by w   , w    dw   . d (2.4) In addition, w    0 everywhere on  . (2.5) It is already known that w    0 inside  . Further, if the coordinates of the points of the contour of  have also continuous derivatives up to the third order, the second derivative w   will be continuous on  from the left and its boundary value w   is given by w    dw   . d (2.6) For this purpose it is sufficient to make the substitution   1 1 . In fact, when  covers the region   1 , 1 covers the infinite region with a circular hole 1  1 , 11 and hence, considering  as a function of 1 , one obtains the required transformation. So finite simply connected regions will almost always be mapped on to the circle   1 , and infinite simply connected regions on to the region   1 . In both cases one could limit oneself to transformations into the circle   1 , but the stated convention is somewhat more convenient in practical applications. Following on, a few remarks will be made regarding the condition of multiconnected regions. For example, a doubly connected region  (i.e. a region, bounded by two contours, regions of more general shape will not be considered here) may always be mapped on to a circular ring. It is different from the simply connected regions; this ring may not be chosen quite arbitrarily. The ratio between the radii of the inner and outer circles will depend on the shape of  . Two simple theorems will be stated here (Muskhelishvili 1975)*: (i) Let  be a finite or infinite (connected) region in the  plane, bounded by a simple contour  , and let w   be a function, holomorphic in  and continuous up to the contour. Further, let the points, defined by   w   , describe in the  plane (moving always in one and the same direction) some simple contour L , when  describes  ( where it is assumed that different points of  correspond to different point of L ). Then   w   gives the conformal transformation of the region  , contained inside L , on the region . * The more detailed characteristics of conformal mapping functions are introduced in the Chapter 7 of this reference 12 (ii) Let  be a finite or infinite (connected) region, bounded by several contour  1 ,  2 ,…,  k (having no points in common). Let w   be a function, holomorphic in  and continuous up to the boundary, and let the point  , defined by   w   , describe in the  plane the simple contours L1 , L2 , …, Lk (not having common points), bounding some (connected) regions  , when  describes the contour  1 ,  2 ,…,  k . When  describes the boundary of  in the positive direction (i.e. let  all the time on the left), the corresponding point  describes the boundary of  likewise in the positive direction. Under these conditions   w   represents the conformal transformation of  on to  . It is clear to us that, if  and  are conformally transformed into one another by a relation of the form (2.1), the point  will move in the positive direction along the boundary of  , when  describes the boundary of  in the positive direction. 13 2.2 On Perturbation Method For most of the real problems, the techniques of getting exact solutions are very restrictive. Definitely, those problems that the exact solutions can be obtained must be sufficiently idealized for the technique to be appreciable (Chiang 1997). For more practical models whereby either the boundary geometry or the governing equations are more complex, the approximate solutions become imperative. If the problem is close to one that is solvable, perturbation methods are effective methodologies to get the analytical answers. However, if the problem is very complicated to accord an exact solution, the numerical methods via discretization must be employed. Generally speaking, the analytical perturbation methods are much more versatile to gain qualitative insight, while numerical methods are much better to produce quantitative information. Sometimes the two categories of methods can be employed together to get the semi-analytical solutions for some problems with small departures from the real phenomenon. Subsequently, we will give brief introductions to the analytical perturbation methods. On the methodology, let us first outline the typical ideas and procedure for perturbation analysis. 1) Identify a small parameter. This is the important first step by which we can recognize the physical scales relevant to the problem. After that, we can normalize all variables with respect to these characteristic scales. In the normalized form, the governing equations will contain dimensionless parameters, each of which stands 14 for certain physical mechanisms. If one of the parameters, say  , is much smaller than unity (if the parameter happens to be large, we can choose the reciprocal as the small parameter), then  can be chosen as the perturbation parameter. 2) Expand the solution as an ascending series with respect to the small parameter  . For instance, a power series u  u0   u1   2u2  ..., where un is named as the nth-order term. The series may vary according to the manner that  appears in the equations. If  1 2 ,  ,… are present, we can employ a series in integral powers of  1 2 . If only  2 ,  4 ,… appear, try a series referring to integral powers of  2 ,etc. 3) Combine terms of the same order in the governing equations and auxiliary conditions, and get perturbation equations at each order. 4) Calculating from the lowest order, solve the equations at each order successively, up to certain order, at say O   m  . 5) By substituting the results for un , n  0,1, 2,... back into perturbative expansions u  u0   u1   2u2  ..., we can get the final solution, which is accurate to the desired order, say O   m  . This straightforward procedure mentioned above is generally known as regular perturbation. There are many problems where the regular perturbation series may fail in the independent variable. So, we will introduce the singular perturbation analysis, which involves the following additional steps: (i) Diagnose the reason why the regular expansion is unreasonable. Check 15 which of the original assumptions are incorrect so that failure occurs. Which are the terms that we initially supposed to be small or to be large? (ii) Choose new normalization parameters and accord the magnitudes to the terms that should be important and commence a new perturbation analysis. Sometimes the new solution may reveal the need to expand the solution with the ordering terms such as  ln  ,  2 ln  ,…, etc. The above procedures can be suitable for most problems. Generally speaking, the governing equations can be algebraic equations, ordinary or partial differential equations or integral equations. We need to emphasize that the importance of identifying the correct small parameter by finding the relevant scales of the physics. Without the physical foresight, it is very difficult for us to make effective use of the mathematics to simplify the real problem. In general, the execution of perturbation analysis can be tedious, however, for the mathematical elegancy, we should have a spirit to persist on this approach if this method is deemed feasible to handle the research problem. Subsequently, we would like to introduce the categories of perturbation method that can be widely applied. The first one is the regular perturbations of algebraic equations. Let us examine the quadratic equation: u 2  2 u  1  0, (2.7) where  is much smaller than unity. The exact solution is well known. We shall use this simple example to illustrate the procedure that can be extended to equations that 16 cannot be solved exactly. Let us propose to find the solution as a perturbation series u  u0   u1   2u2   3u3  ..., (2.8) and substitute this series into (2.7) u   u1   2u2   3u3  ...  2  u0   u1   2u2   3u3  ...  1  0, 2 0 (2.9) Expanding the square and collecting terms of equal powers, we get u 2 0  1    2u0  2u0u1    2  2u1  u12  2u0u2   ...  0, (2.10) With the coefficient of each power of  set to zero, a sequence of perturbation equations is obtained at various orders    0  : u02  1  0, (2.11)     : 2u0  2u0u1  0, (2.12)    2  : 2u0u2  u12  2u1  0, (2.13) From (2.11) the lowest order solution is u0  1, (2.14) With this result higher-order problems are solved successively u1  1, And u2   (2.15) u12  2u1 1   . Summarizing, the approximation up to    2  is 2u0 2 17 u  1    2 2  ... , (2.16) Clearly, this result confirms that the perturbation series will guarantee the accuracy. Note that the perturbation equation at the leading order for u  0  is still quadratic and has two solutions. Higher order solutions simply improve the accuracy of the two. This feature is typical of regular perturbations. Beyond the regular perturbations, there are another kind of perturbation method named as singular perturbation method. The following is the cubic equation: u  1  2 u 3 , (2.17) It can also be solved exactly. For small  let us try the straightforward expansion u  u0   u1   2u2   3u3 ... , (2.18) Substituting this series into (2.17) and expand the cubic term, we get u0   u1   2u2   3u3  O   4   1  2 u03   3u02u1   2  3u02u2  3u0u12   O   3   , (2.19) Equating like powers of  yields the perturbation equations O   0  : u0  1, (2.20) O    : u1  2u03 , (2.21) O   2  : u2  6u02u1 , (2.22) The solutions are obviously u0  1 , u1  2 , u2  12 , … , hence the final solution is 18 u  1  2  12 2  O   3  . (2.23) Why did the two other solutions of the original cubic equation disappear? The reason is that in (2.17) the term u 3 of highest power is multiplied by the small parameter. The straightforward perturbation series causes the highest power at the leading order to vanish, hence only one solution is left; higher order analysis merely improves the accuracy of this solution. In similar situations the problem is called singular, and the straightforward expansion is sometimes called the naive expansion. After checking the source of error, we seek a ‘cure’ by rescaling the unknown so as to shift the small parameter to a lower order term in the new equation. Let u  x m , where m is yet unknown. Equation (2.17) then becomes x m  1  2 x3 3m 1. (2.24) We now face several choices: (i) All three terms are equally important. This choice would require m  0 and 3m  1  0 , which cannot be satisfied at the same time. (ii) Only one of the three terms dominates. Clearly, the results are full of inconsistencies. (iii) Two out of three terms dominate over the remaining one. One must now identify the pair by trial and error. Let us assume that the second and third terms in (2.24) are more important than the first. Equating the powers of  , we get 3m  1  0 , implying that m   1 3 . But (2.24) becomes x 1 3  1  2 x3 , where the first term appears to be the greatest, thereby contradicting the original assumption. Hence the choice is not acceptable. The second choice that the first and second terms dominate must also be ruled out, since 19 this corresponds to the naïve expansion. The remaining choice is to balance the first and third. Equating their powers of  , we get m  3m  1 or m   1 2 . Equation (2.24) becomes x 1 2  1  2 x3 1 2 . (2.25) Indeed, the second term is much smaller. Substituting the new expansion x  x0   1 2 x1   x2   3 2 x3  ... (2.26) into (2.25) and collecting like powers of  , we get the perturbation equations O   1 2  : 2 x03  x0  0, (2.27) O   0  : 6 x02 x1  x1  1  0, (2.28) O   1 2  : 6 x02 x2  6 x0 x12  x2  0, (2.29)   The solutions at successive orders are x0  0, 2 2,  2 2 , x1   x2   1 6x 1 2 0 and 6 x0 x12 . To find x1 , x2 , … explicitly the three solutions for x0 must taken 6 x02  1 one at a time. For x0  0 , we have x1  1 and x2  0 , hence x   1 2  O   3 2  and u   1 2 x  1  O    (2.30) This result is just the solution found by naïve expansion. For the second root x0  2 2 , x1  1 2 and x2   3 2 8 , hence x  2 2  1 3 2 12 u   1 2 x  2 2  1 2     ... . 2 8 1 2 2  3 2  ... and 8 (2.31) 20 For the third x   2 2 1 2 2 root  x0   2 2 , x1  1 2 and x2  3 2 8 , hence 3 2  ... and 8 1 3 2 12 u   2 2  1 2     ... 2 8 (2.32) Improvement for all the roots can be calculated in the above procedures. There are some interesting applications of perturbation methods to heat transfer as shown in the book by Aziz and Na (Aziz & Na 1984). 21 Chapter 3 Linear Acoustic Wave Scattering by Two Dimensional Scatterer with Irregular Shape in an Ideal Fluid 3.1 Governing equations of linear acoustic wave The propagation of linear sound waves in a fluid can be modeled by the equation of motion (conservation of momentum) and the continuity equation (conservation of mass). With some simplifications by taking the fluid as homogeneous, inviscid, and irrotational, acoustic waves can serve to compress the fluid medium in an adiabatic and reversible manner. The linear acoustic wave equation is written as:  2  1  2 . c02 t 2 (3.1) The pressure p and small fluctuating on quantity of the static mass density  are expressed as: p   0    or    20 c0 t t where c0  (3.2) p  . Here, c0 is the wave speed in the fluid, 0 is the static mass density of the medium and  is the small fluctuating quantity of the static mass density. We set the Laplace variable as s    i , and as such the direct and inverse Laplace transforms are given by (Pablo & Felipe 2009): 22     i      t  e t   e  it dt , 0  t   et 2      i   eit d .  (3.3) (3.4) Here  is the angular frequency and  is a stability constant. It can be noted that when   0 , Eqs. (3.3) and (3.4) correspond to the Fourier transforms. In other words, the Laplace transform can be simply obtained by applying the Fourier integral to   t  exp   t  , i.e., a damped version of   t  . As such,  is also known as the damping constant. The integral transforms (Eqs.(3.3) and (3.4)) also provide a possible means to solve for the incident wave modeled as pulse, shock wave or any other prescribed waveform. By substituting (3.4) into Eq.(3.1), we can obtain the corresponding Helmholtz equation in the frequency domain as below:   i   .   2 2 2 c0 (3.5) Here, we will define   i  c0  ik , and the reduced Helmholtz equation becomes:  2  k 2  0, (3.6) where k can be reformulated as k    i  c0 . The solution of  in Eq.(3.1) can also be assumed as:     e i t . (3.7) Here  can stand for pressure, velocity or velocity potential, and we can choose the variables according to the facility for expressing the boundary conditions. Moreover, 23 if we set   0 , the wave number k will be the same as the harmonic wave k   c0 . In this paper, the outgoing scattered wave will be combined with Hankel function of the first kind and the time term e  i t . 3.2 Conformal transformations of Helmholtz equation and corresponding physical vector For the model of acoustic wave scattering by three dimensional inclusion with arbitrary geometry embedded inside the water, analytical approach is deemed rather restrictive and confined to simple geometry. However, it is conceivable to solve for the ‘degraded’ two dimensional model with irregular cross section by applying the method of conformal mapping in the complex plane. Firstly, we will introduce the degraded two dimensional Helmholtz equation in the Cartesian coordinates shown as:  2  2  2  k 2  0. 2 x y (3.8) Here, we shall introduce the complex variables   x  yi and   x  yi into the Helmholtz equation (3.6) and re-write as:  2 1  k 2  0.  4 (3.9) For wave scattering problems involving non-circular objects in the complex  ,   plane (as shown in Figure 3.1), it is possible to map the internal/external region of the irregular shaped object (in the  ,   plane) onto the inside/outside region of the circle (in the  ,  plane). In addition, it is taken that the conformal 24 mapping function w   should be an analytic function to ensure the configuration in the  plane is locally similar to its image in the mapped  plane. In other words, the first order derivative of the mapping function w   at any point is neither 0 and  . We also note that since d   w   d , when we transform the initial infinite-small element d  into d , there can be an expansion of length of   magnitude w   and a rotation of Arg w   . y x Solid Incident Acoustic wave Infinite fluid  Figure 3.1: The model for scattering of acoustic wave by rigid inclusion with irregular across section Consequently, the corresponding governing equation (3.9) in  ,  plane takes on the following form: w   w   2  2  k   0.  4 (3.10) Equation (3.10) is a general expression for the spatial linear acoustic wave in the  ,  plane. It needs to be pointed out that   x  yi , d   d ei ;   r  ei , d  d ei ;   w   , d  w   d , d  w'  d . That is, we can obtain the velocity components U x and U y as expressed by the mapping function 25 as well as mapping coordinates  ,  : Ux   1   , w    w'    1  1  1   Uy  i  w    w'     (3.11)  .   (3.12) The corresponding vector U r and U inside the mapping plane as expressed by the coordinates  ,  are: Ur    1     ,     r w'     (3.13) U        .    r w     (3.14) i ' b a      Medium II Medium II Medium I Medium I Figure 3.2: Illustration of the conformal mapping that transforms the initial irregular geometry into a circular one It should be noted that the mapping function can transform the initial geometry into a circular shape (as shown in Figure 3.2), and the corresponding physical vector is changed (shown as Eq.(3.13) and Eq.(3.14)) inside the mapping plane  ,  and is different from the original expressions for the physical vector as presented in Eq. 26 (3.11) and Eq. (3.12). As we know, Eq.(3.10) is the fundamental equation for solving acoustic wave scattering around a two dimensional object with any cross section. They can be solved by separation of variables   ,    1   2   (Liu et al. 1982), and this leads to Eq.(3.10) taking on the following:  1   2    w   w   2 k  1   2    0. 4 (3.15) The linear combination of  1   and  2   corresponding to various values of  (the separation constant) would then be the general solution of Eq.(3.10):     ,    A     exp ik   w    w     2 d  . W (3.16) The path W is any path of integration in the  plane, which makes the expression convergent. Furthermore, we can set   exp  it  , w    w exp  i   , where t is a complex variable, w is the norm and  is the phase angle of w   . Consequently, we can obtain the following expression for Eq.(3.16):   ,    a m  m eim  e im  ik w sin  W d (3.17) where   t     2 , and am are arbitrary constants. Here, m is an integer. Denoting the integral by  m   , we have  m  k w( )    e W im  ik w sin  d . (3.18) We can further express Eq.(3.17) as follows: 27  w      ,    am   m  k w( )     .  w    m     m (3.19) Expression (3.19) is the general solution of Eq.(3.10). It is possible to introduce the fractional order Bessel/Hankel function of Helmholtz equation via the method of separating variables without the mapping function. In our approach, we propose the formulation for the general solution of Helmholtz equation: the Bessel function with fractional order mp previously or the mapping function k w( ) as the argument, respectively, by which we may extend the analysis for the in-plane elastic wave propagating through the solid or acoustic wave transmitting through the fluid with complex boundary conditions. We would like to point out that the general solution depends on the choice of path for integration. Along certain path, the function can be Bessel or Hankel function. etc. In the case of circular region where polar coordinates are adopted, the expression (3.18) turns out to be the Bessel function; for the model of elliptical domain with elliptic coordinate system, it gives rise to the Mathieu functions. Moreover, one should take note that the singularity of the Hankel function at zero point allows the construction of the standing wave inside the circular/fan-shaped domain as expressed by Bessel function and ring-shaped domain by the Hankel function, respectively. For the acoustic wave propagating through the fluid medium without the transmission into the inclusion, the general mapping function for the numerical calculation can be cast as (Muskhelishvili 1975):   w    R   p  q  , R  0 ,0  p  1 q . (3.20)  The above mapping function thus map the outside of the curve in the  ,   plane on to the region   1 . For the condition of q  1 , the contour will be an ellipse; 28 when q  1 p  2 or q  1 p  3 , the corresponding contours have three or four cusps, respectively, and they resemble the shape of a triangle or square. Circles with radii r  1 in the transformed  plane correspond in the  plane to hypotrochoids, which likewise for r near 1 resemble triangles or squares with rounded corners. If in Eq.(3.20)  is replaced by 1  , one obtain the transformation of the region such that   1 with   w    R 1   p q  .  For the holomorphic series w     1   ck k , we can map the region k 1   outside of  in the  ,  plane into the interior of the unit circle in the  ,  plane. However, it is deemed not quite logical to cast the problem for the wave propagation through the fluid inside the scatterer in the transformed plane. Separately, it may be noted that in the method of Schwarz-Christoffel Formula (successive approximate solution(Mikhlin 1947)), by expanding the holomorphic mapping  function w   into the polynomial series w       ck  k , it is possible to map k 1   the region outside of  in the  ,  plane into the exterior of the unit circle in the  ,  plane. If there are only two non-zero terms in the mapping, i.e. w      cn  n , the hole is a hypotrochoid that is a quasi-polygon having n  1 equal ‘sides’(England 1971; Zimmerman 1986). In order for the mapping to be single-valued, and for  not to contain any self-intersections, cn must satisfy the restriction 0  cn  1 n . The choice of cn  0 gives rise to a circle, whereas the limiting value of cn  1 n gives a scatterer with n  1 pointed cusps. For the particular choice of cn  2 n  n  1 , the mapping coincides with the first two terms of 29 the Schwarz-Christoffel mapping for an  n  1 -sided equilateral polygon and resembles a polygon with slightly rounded corners (Levinson & Redheffer 1970; Savin 1961; Zimmerman 1991). In the literature, there are suggested mapping functions for the inclusion with sharp corners but these possess an  n  1 -fold axis of symmetry with the application of the Schwarz-Christoffel mapping function (see Ekneligoda etc. (Ekneligoda & Zimmerman 2006; Ekneligoda & Zimmerman 2008)). For our problem, we would like to propose the mapping function as below: w      c1  n  c2  2 n 1  c3  3n  2 . (3.21) For the mapping to be conformal, and for the contour not to have any self-intersections, it is clear that w    0 be avoided along the contour. This poses some restrictions on the allowable range of values for the ci coefficients. If w    0 for some values of  on the unit circle, as the ci values increase, this will first occur at  n  1 equally spaced points that include the point corresponding to   1 . Hence, the restrictions for the ci can be found by setting w 1  0 . For the two term mapping, this leads to the restriction that c1  1 n . For the three-term mapping, the condition is obtained as nc1   2n  1 c2  1 , and for the four-term mapping, the condition is provided as nc1   2n  1 c2   3n  2  c3  1 . (see also (Ekneligoda & Zimmerman 2006; Ekneligoda & Zimmerman 2008)). 30 3.3 Acoustic wave scattering by object with irregular across section Consider a rigid object with irregular cross section immersed in an ideal compressible fluid, such that both the viscous and thermal effects can be neglected. Here, we shall assume that there is no standing wave inside the rigid body. In other words, we are only concerned with the scattering wave generated by the impenetrable rigid body, from which we can calculate the radiation acting on the scatterer as well as the far field scattered pressure generated by the scattering. (For other conditions of acoustic wave scattering by elastic object immersed in Newtonian fluid, there will be the standing wave inside the elastic object and the linear shear force is generated by the movement of fluid. Under such assumptions, the unknown coefficients of the scattering wave and standing wave inside the elastic inclusion can be obtained through the continuity of stress and velocity along the interface. This is to be pursued in future work in which our proposed method is fully capable of solving.) For the plane acoustic wave equation in Eq.(3.6), the expression for acoustic waves in the complex plane as well as in the mapping plane is shown below ik  i   A0  eiknr  A0  eik  x cos  y sin    A0  e 2 as:  e  i  ei  ik  A0  e 2  w e  i  w ei  . (3.22) where  is the angle between the positive x -axis and the direction in which the wave travels. We can also use the Laurent expansion in the form of 31   exp     1  2   m  J m     m , and assume that   k   and   ie i  .  In this manner, we can obtain another format for the incident potential   i  expressed by the Bessel function as below:     A0  i  Jm  k     m   i m m   im m   e   A0  i  Jm k w  m     w   im   e .  w     m (3.23) According to the Sommerfield radiation condition, the outgoing scattered wave that is generated by the rigid body:  s  w      Bm  H m  k w( )     ,  w    m     m 1 (3.24) where H m1   is Hankel function of the first kind of order m th. The total velocity potential field in the fluid domain   t  should be the summation of the incident wave  i  and the scattered wave   s  . By substituting expressions (3.22) and (3.24) into (3.13) and (3.14), we can obtain the corresponding velocity components as follows: ' ' ikA0 ik2  w e i  w ei    w    i  w   i  e   e e , '  r w'    2 r w      (3.25) ' ' kA0 ik2  w e i  w ei    w    i  w   i   e  e  e , '  r w'    2 r w      (3.26) U r   i i  U  k  Ur    Bm  Hm1 1 k w 2 m    s   ik  U    Bm  Hm11 k w 2 m    s  m1   w  w'    Hm1 1 k w    w  r w'      w  w'    Hm1 1 k w   '  w  r w    m1    m1  w  w'   , (3.27)     w  r w'       m1  w  w'   . (3.28)     w  r w'      32 Here, the unknown coefficient Bm of the radiation velocity potential in Eq. (3.24) can be determined according to the radial component of the velocity U r set to be zero along the interface of the fluid and the rigid inclusion (i.e. a Neumann condition on the velocity potential U r t     t  ; see also (Mitri 2010b)): U r i  r a  U r s   0. r a (3.29) This assumption has been recognized to properly model the radiation force on liquid drops in air and under reduced gravity environments (Mitri & Fellah 2007). If the density of cylinder is taken as zero (or very small in comparison to the fluid density), the solution applies to the scattering by a soft cylinder (satisfying the Dirichlet condition on the pressure quantity P t     0   t  t  0 at the cylinder radius r  a ; see also (Flax et al. 1981)). Furthermore, this boundary condition with infinite series can be written as:  B m  m  m    0, (3.30) where m  Hm1  k w    1   iA0  e   w       w      ik w  e  i  w ei 2 m1  w     w'   1   Hm  1  k w       '  w    r w     m1   w'   , (3.31) r w'      w'   i  w'   i   e  e . '  r w'    r w      The periodic function can be expanded via the Fourier series (   (3.32)   n  where  n  1 2  2 0 n  ein ,   e  in d ). Similarly, the unknown coefficients Bm in Eq.(3.30) can be determined via Fourier series expansion of Eq.(3.30) in the matrix form where 33 n is equal to m ( ein on the both side are omitted):     B  n n m    n . (3.33) m  e in d , (3.34) nm n where nm  n  1 2 1 2  2 0  2 0   e in d . (3.35) Equation (3.33) could then be reduced to a series of algebraic equations by truncating to finite terms accordingly. The number of truncated terms employed depends on the frequency and accuracy requirement. The results obtained are calculated by a code written in MATLAB 7.0 interpreter language and employment of 19 terms in the Fourier series which means n and m range from -9 to 9. Based on the above coefficients Bm , we can substitute these into the expressions for the velocity as well as the pressure in the fluid domain as follows (the time term e  i t is omitted here for simplicity): m   ik    w ei wei  w     t  1 P  P  P  0  0   i  A0  e 2   Bm  Hm   k w()     .    t m  w     t   i  s (3.36) When the variable tends to infinity, the asymptotic expression of Hankel function is such that (Mow & Pao 1971): Hm1  k w()   2 2 m i k w( ) m 2 4 i k w( )  4 e   i   e .  k w()  k w() (3.37) 34 Consequently, we can obtain the expression for the far-field scattered pressure from the infinitely long non-circular cylinder due to an incident plane wave of unit amplitude:  fs P  w     .  w     m  2 i k w( )  4  0   i   Bm   i   e   k w() m m (3.38) The wave number of incident wave can be expressed as the ratio of the inclusion 2r to the wave length of the incident wave, namely, Wave number  kr    i  r c0  2 r  (3.39) which represents a dimensionless frequency 2 r  . In this work, the amplitude of the incident acoustic wave A0  1 , and the speed of the acoustic wave propagating through the fluid is c0  1480 m s . It is noted that the relations widely applied for the derivation of the complex variables together with mapping function are shown as below:    1 H m k w          1 H m k w             1 H m k w       m  w     k 1 k w      H  w     2 m 1     w         w     m   w       w          k H m1 1 k w    2   m  w     k 1      H m 1 k w     2  w        m 1  w'   ,  w         w     w       w      (3.40)  m 1  w'   , (3.41) m 1  w'  , (3.42) 35 m   w     k 1   1 H m k w     k w     H  w     2 m 1            w       w       m 1  w'  . (3.43) Furthermore, if we set w      z , the equations are reduced to the corresponding derivations found in the literature (Liu et al. 2010; Liu et al. 2009; Liu et al. 2008) which were obtained by the complex variable method without the local conformal mapping function. (In other words, those models can also stand for the mapping of the circular cavity into circular one). 3.4 Results and Analysis All results in this section were generated using the boundary condition summarized in Eq.(3.30) to Eq.(3.32), with Eq.(3.23) for the incident field and Eq.(3.24) for the scattered field. The pressure field given by Eq.(3.36) is applicable to the fluid domain as well as the far field expression for the scattered pressure shown in Eq.(3.38). The damping constant  (as shown in Eq.(3.3)) is assumed to be zero for the present model of ideal fluid. In order to verify the accuracy of the results obtained with our proposed employment of the conformal mapping in conjunction with the complex variables method, the computed results are to be compared to published work (Pillai et al. 1982) for kr ranging from 0.1 to 5. To this end, the following far-field form function f  is considered (Leon et al. 2004b): f   2daeff P s  a i P  2 (3.44) 36 with an effective radius aeff defined by aeff  a 2  b 2  2 . Here, d is the distance of observation, a stands for the major semi-axis of the ellipse, and b is the minor semi-axis. The major semi-axis of the ellipse is set to be a  1 and the minor semi-axis b  0.5 (as applied to the mapping function   w    R   p  q  ,where the employment of R   a  b  2 , p   a  b   a  b  and q  1 transforms the ellipse into a circle with the radius of one (as shown in Figure 3.3).We calculate the bistatic scattering pattern along the loop of the inclusion, as well as the equivalent far-field form factor f  . 2 Ellipse x/y=2.0 Y Axis 1 0 -1 -2 -2 -1 0 1 2 X Axis Figure 3.3: The geometry for the canonical ellipse based on the mapping   function w    R   p  q , where r  1.0, R  0.75, p  1/3, q  1.0. Figure 3.4 represents the polar plots of the bistatic scattering pattern at fixed frequencies of kr  2.0 and 5.0, respectively, with different incident angles at   00, 450, 900. It is evident that our results for the bistatic scattering pattern concur very well with the results obtained by T-matrix method† (Pillai et al. 1982)). † The detailed results from Pillai et al. 1982 can be found from the Appendix E 37 90 1.2 0.8 120 (a) =0 60 =90 0 2.0 120 (b) =0 60 1.5 1.0 0.4 0 =45 0 =90 0 30 150 0.5 0 180 0.0 180 0 0.5 0.4 0.8 90 0 30 150 0 =45 330 210 1.0 330 210 1.5 1.2 240 300 240 2.0 300 270 270 Figure 3.4: The comparison of the present method with the T-matrix method (Pillai et al. 1982) at 2:1 aspect ratio ellipse for bistatic scattering pattern at (a) kr  2.0 and (b) kr  5.0 If∞I 1 0.1 0.01 0.1 0 α =0 0 α =30 0 α =60 0 α =90 Diperna & Stanton 1 10 kr Figure 3.5: The comparison of the present method with the Fourier matching method (Diperna & Stanton 1994) at 2:1 aspect ratio ellipse for the far-field form function In Figure 3.5, we have plotted the far-field form function for wave incidences at 00 (along the major axis of the cross section), 300, 600 and 900 to the acoustically hard cylinder. It is evident that our results concur well with the Fourier matching method 38 (FMM) at the condition of   00 (Diperna & Stanton 1994). We also show the variation of incident angle with respect to the horizontal axis; it is interesting to note that the scattering far-field form factor for the hard cylinder with horizontal incidence   00 is slightly higher than that of oblique incidences (for instance,   300, 600, 900). The far-field form factor decreases with respect to the increase of the incident angle  . However, as the frequency increases the form factor becomes slightly higher for the condition of vertical incidence at   900. According to the mapping function   w    R   p  q  , we set R  0.7, q  1 p  1.0, 2.0 and 3.0 to take on the shape of ellipse, leaf clover and approximate square, respectively (see Figure 3.6). Here, we have assumed the mapped circle to be   r  ei with r  1.3, corresponding to the ellipse, triangle or square with rounded corners. 2 Ellipse Leaf Clover Approximate Square Y A x is 1 0 -1 -2 -2 -1 0 1 2 X Axis Figure 3.6: The geometries for the scatterer based on the mapping function w    R   p  q  , where r  1.3, R  0.7 and q  1 p  1.0 (ellipse), 2.0 (leaf clover) and 3.0 (rounded corner square) 39 If∞I 1 (a) 0.1 α α α α 0.01 0.1 1 0 =0 0 =30 0 =60 0 =90 10 kr If∞I 1 (b) 0.1 0.01 0.1 If∞I 1 1 10 1 10 kr (c) 0.1 0.01 0.1 kr Figure 3.7: The far field form function for the acoustic wave scattering by various cross section w    R   p  q  , where r  1.3, R  0.7 and q  1 p  (a) 1.0 (ellipse), (b) 2.0 (leafclover), (c) 3.0 (rounded corner square) Figure 3.7-a plots the far-field form factor for the (relatively more slender) ellipse, while Figure 3.7-b and Figure 3.7-c show the far-field form factor of the 40 incident acoustic wave scattering by the leaf clover and rounded corner square for various incident angles and frequencies, respectively. This scattered form function is plotted versus kr , where r is the radius of the circular rigid inside the mapping plane. It is clear that the distribution of the form factor takes on essentially the same variation for the scattering by the ellipse. However, there appears to exhibit a sharp decrease at around the wave number of kr  4 for the leaf clover (Fig.3.7-b) and square (Fig.3.7-c). Compared with previous published literature, our method is able to match better with the experimental results obtained from the physical optics approximation (Diperna & Stanton 1994). It is also observed that the general far-field form factor for the square and leaf clover shapes are larger than the slender ellipse which may be attributed to the smaller cross section of the latter. The bistatic scattering pattern at kr  2.0 and 5.0 for the model of slender ellipse, leaf clover and approximate square along the loop of the inclusion are calculated and shown in Figure 3.8. It is clear that the angle and frequency of the incident waves have significant influence on the bistatic scattering pattern. It is also obvious that the bistatic scattering pattern with solid line is symmetrical to the horizontal for the condition of incident angle at   00. In general, the increase of the incident frequency will result in higher bistatic scattering pattern for all the shapes examined. In particular, among the geometries, the slender ellipse seemingly can amplify relatively more the bistatic scattering pattern for these selected frequencies, which may be attributed to the relatively sharper corners on the left and right edge of the slender ellipse as compared to the leaf clover or square. 41 90 3 2 (a) Ellipse 120 kr=2.0 =0 60 90 0 =45 0 =90 0 2 30 150 1 0 330 210 240 2 120 3 (b) Leaf clover kr=2.0 =0 60 330 210 240 300 90 0 =45 0 =90 0 30 150 120 3 (e) Leaf clover kr=5.0 2 0 =0 60 0 =45 0 =90 30 150 1 0 180 0 0 180 1 0 1 330 210 3 240 2 (c) Square 120 3 kr=2.0 330 210 3 300 270 90 240 300 270 90 0 =0 60 =45 0 =90 0 30 150 (f) Square 120 3 kr=5.0 =0 60 0 0 =45 0 =90 2 1 30 150 1 0 180 0 1 3 0 270 1 2 0 30 150 3 300 270 90 2 0 =90 1 3 2 0 =45 0 180 1 2 =0 60 1 0 180 2 (d) Ellipse 120 3 kr=5.0 0 180 0 1 330 210 240 300 2 3 330 210 240 270 300 270 Figure 3.8: The bistatic scattering pattern for the model of slender ellipse, leaf clover and approximate square at kr  2.0 and 5.0 Next, we calculate the far-field form function f  for the irregular geometries with sharp corners based on the novel mapping function taken from Eq.(3.21) w      c1  n  c2  2 n 1  c3  3n  2 with the first two or three terms of the 42 Schwarz- Christoffel mapping function. Figure 3.9 show the irregular scatterer have threefold symmetry and sharp cornners (i.e. n  2 ). The calculated results depicted in Figure 3.10 correspond to the geometries illustrated in Fig.3.9. According to Fig.3.8-b and Fig.3.10-a1, we found that the bistatic scattering pattern are similar, though the mapping function applied are vastly different from each other. This attests to the viability and robustness of the present approach with the proper employment of conformal mapping with complex variables. From Figs.3.10-a3,b1,b2,b3, it is clear that the n-fold symmetric objects with sharp corners can greatly amplify the bistatic scattering pattern compare with the smooth corners as shown in Fig.3.10-a1,a2. Our calculations have clearly shown that the present method can easily take on geometrical shape possessing sharp corners. 2 2 (a) 1) 2) 3) 1 0 -1 -2 -2 1) 2) 3) (b) Y A x is Y A x is 1 c1=1/5,c2=0,c3=0 c1=1/3,c2=0,c3=0 c1=1/2,c2=0,c3=0 c1=1/3,c2=1/15,c3=0 c1=1/6,c2=2/15,c3=0 c1=1/9,c2=7/45,c3=0 0 -1 -1 0 X Axis 1 2 -2 -2 -1 0 1 2 X Axis Figure 3.9: The geometries for the scatterer based on the mapping function w      c1  n  c2  2 n 1  c3  3n  2 with n  2 43 90 3 2 (a1) 120 =0 60 90 0 =45 0 =90 0 2 30 150 1 0 330 210 240 (a2) 2 120 =0 60 0 0 =90 0 330 210 240 300 (b2) 120 =0 60 0 0 =45 0 =90 30 150 1 0 180 0 0 1 2 330 210 240 240 300 120 300 270 270 90 (a3) 330 210 3 3 =0 60 =45 =90 0 3 2 30 150 90 0 0 (b3) 120 =0 60 0 =45 0 =90 0 30 150 1 1 0 180 0 0 180 0 1 1 3 3 2 30 150 1 2 =90 0 0 =45 0 180 2 0 270 90 1 3 =45 30 150 3 300 270 90 2 0 1 3 2 =0 0 180 1 3 (b1) 60 1 0 180 2 3 120 330 210 2 3 240 330 210 300 270 240 300 270 Figure 3.10: The bistatic scattering pattern for the scatterer with n-fold axes of symmetry and sharp corners at kr  2.0 44 3.5 Conclusions In this study, we have analytically obtained the two dimensional general solution of Helmholtz equation, shown as Bessel function with mapping function as the argument and fractional order Bessel function, to study the linear acoustic wave scattering by rigid inclusion with irregular cross section in an ideal fluid. Based on the conformal mapping method together with the complex variables method, we can map the initial geometry into a circular shape as well as transform the original physical vector into corresponding expressions in the mapping plane. This study may provide the basis for further analyses of other conditions of acoustic wave scattering in fluids, e.g. irregular elastic inclusion within fluid with viscosity, etc. Our calculated results have shown that the angle and frequency of the incident waves have significant influence on the bistatic scattering pattern as well as the far field form factor for the pressure in the fluid. Moreover, we have shown that the sharper corners of the irregular inclusion may amplify the bistatic scattering pattern compared with the more rounded corners. 45 Chapter 4 An Analysis on the Second-order Nonlinear Effect of Focused Acoustic Wave Around a Scatterer in an Ideal Fluid 4.1 Second order nonlinear solution for Westervelt equation The widely used linear wave equation used to describe the small signal (infinitesimal amplitude) propagation is the Helmholtz equation(Liu et al. 2009): 2  1  2  0. c2 t 2 (4.1) Here,  can be pressure, velocity or velocity potential in the field of fluids, or displacement and displacement potential for solids (Liu et al. 2010); c is the small signal sound speed since there are no shear waves inside the ideal fluid. For the linear wave propagation in elastic solids, the in-plane longitudinal and transverse waves (Liu et al. 1982) as well as anti-plane transverse wave (Liu et al. 2008) can co-exist and governed by the same Helmholtz equation. If we neglect the time term in Eq.(4.1), the Laplace equation is also widely employed for the incompressible ideal fluid (Doinikov & Zavtrak 1995; Wang et al. 1996) and static linear solid mechanics (Ballarini 1990). In the past, much computational work have been done on nonlinear effects in acoustic wave beams based on the KZK equations (Kamakura 2004; Kamakura et al. 2004; Lee & Hamilton 1995; Tjotta et al. 1990). The one dimensional case of Westervelt 46 equation is studied extensively by finite element method (Pozuelo et al. 1999). However, when acoustic fields of more complex conditions are considered, advanced numerical calculation related to finite-differential becomes necessary (Vanhille & Pozuelo 2001; Vanhille & Pozuelo 2004). In this work, our interest is to develop the analytical solution of the multiple harmonic acoustic waves focused on the area near a scatterer where the second order nonlinear effects dominate (see Figure 4.1). Our study has important implications for further work on bubble/nucleation cavitation by HIFU (high intensity focused ultrasound) and others. O Rs Re Multiple incident acoustic waves Figure 4.1: Schematic description of the model for multiple acoustic waves focused around a scatterer inside an ideal fluid On the problem of multiple acoustic waves focusing on intensive area, one model governing the dynamics is the Westervelt equation, 2 p  1 2 p   2 p 2  3 p   4 3  0. c2 t 2  c4 t 2 c t (4.2) Here, the third term is the nonlinear term and the forth term stands for the 47 thermoviscous effect.  is the static medium density, c is the wave speed of the acoustic wave in the undisturbed liquid,      1 2 is the coefficient of nonlinearity, and  is defined as the ratio of specific heats of the gas.         1 Pr  is the diffusivity associated with sound absorption where    is the kinematic viscosity,   4 3   B  is the viscosity number,  B is named as the bulk viscosity coefficient and Pr is the Prandtl number. If we consider the case of ideal fluid, the forth term can be set equal to zero, and the reduced Westervelt equation is, 2 p  1 2 p  2 p2   0. c2 t 2  c4 t 2 (4.3) To solve the second-order nonlinear equation, the successive approximations method can be applied. This method assumes a solution for the acoustic pressure consisting of the addition of two terms in the form of p  p1  p2 where p1 represents the first order approximation and p2 the second order correction, p2 being much smaller than p1  p2  p1  . Neglecting the terms of third and higher orders, we can obtain the approximate equation as: 2 1   p1  p2    2 p12   p1  p2   2   0. c  c4 t 2 t 2 2 (4.4) According to Eq.(4.4), the second order solution for the acoustic wave can be written as p  P1 exp  it   P2 exp  2it  . The correct analytical solutions of the one dimensional Eq.(4.4) for plane, cylindrical 48 and spherical waves are obtained, respectively, as shown below. It is pointed out, however, that the coefficients on the right hand side of the initial governing equation for the second-order nonlinear term shown as Eq.10 in (Pozuelo et al. 1999) are deemed incorrect. In particular, Eq.10 in reference (Pozuelo et al. 1999) is shown with the term 2k 2  4k 2   c  . 2    c  2   , which we reckoned should be reflected as Therefore, the analytical results that follow for the second-order nonlinearity given in Eq.16, Eq.27 and Eq.19 for plane wave p p , cylindrical wave pc and spherical wave ps , respectively, in (Pozuelo et al. 1999) may contain some errors/ inaccuracies. Finally, we substituted the derived solutions reflected as Eqs. 16, 27 and 19, correspondingly for p p , pc and ps into Eq.10 of reference (Pozuelo et al. 1999) and found some degree of inconsistency. Shown in Appendix B are the details for our derivations in which the results are given below as: p p  P0 e ikx  eit  pc  P0  P02 1  2ikx  e2ikx  e 2it , 2  2  c 2  i kr  e   kr  2  P0  H 0  kr   e i t 4  eit  4i  P02 i 2 2ikr 2it e e e 0c2 2 2i  krP02  2   H kr  e 2it   0 2  c   P0 ikr it i  kP02  ln r   1  n  2  !  2ikr 2it e e   e .  e  c2  r n  2  4ik n 1 r n  r (4.5) (4.6) n ps  (4.7) It is clear that the first term in Eqs. (4.5), (4.6) and (4.7) are the general solutions for the one dimensional linear acoustic wave with time harmonic condition, and the 49 second terms are the approximate solutions for the second-order nonlinearity which satisfy the Sommerfield radiation condition at the far field. Here, P0 stands for harmonic excitation of the wave amplitude, and k   c  2  , where  is the circular frequency of the incident wave, and  stands for the wave length. 4.2 Perturbative method with small parameter for the nonlinear acoustic wave 4.2.1 Mathematical formulation of the nonlinear acoustic wave The analytical solutions in Section 4.1 for the one dimensional Westervelt equation are obtained by the perturbation method without any small parameter. Furthermore, we can only get the pressure inside the fluid domain without the explicit results for the velocity and velocity potential. Below, we will propose a novel mathematical formulation and a different model for the nonlinear acoustic wave that goes beyond the traditional models based on Burgers equation, KZK equation and Westervelt equation. The compressible potential flow theory is invoked together with the dimensionless formulation and asymptotic perturbation expansion referring to the small parameter Mach number. It is to be found that our approach allows the decoupling of the potential and enthalpy terms to the second order, and which accord much flexibility for the calculation of the other physical quantities inside the fluid domain. For our model, we shall take the liquid as inviscid and compressible. As such, 50 the liquid flow is governed by the equation of mass conservation:       u   0, t (4.8) and the momentum conservation equation: u 1  u u   p. t  (4.9) In many fluid dynamic problems, significant liquid compressibility due to high speed motion occurs when thermal effects in the liquid are unimportant. We therefore assume that thermal effects in the liquid are insignificant. With this assumption, the liquid state is defined by a single thermodynamic variable. The sound speed c and the enthalpy h of the liquid can be defined as follows(Wang & Blake 2010): c2  p dp dp , h , p   d where the reference pressure (4.10) p is the pressure in the undisturbed liquid (hydrostatic pressure). By assuming that the flow is irrotational, we may introduce a velocity potential  such that u   . By applying c 2  dp d  , c 2  p  , c 2  p  , u   , where the dot “  ” stands for differential w.r.t time, we can re-write Eq.(4.8) as:  2  1  h    h   0. 2  c  t  (4.11) Similarily for Eq.(4.9), the integration leads to the unsteady Bernoulli equation,  1 2     h  h . t 2 (4.12) 51 Here, h may be set equal to zero since the enthalpy is referenced to the undisturbed fluid at infinity. To find the expressions for the sound of speed c and enthalpy h , we use the Tait model equation of state to relate the pressure and density as follows (Lezzi & Prosperetti 1987; Prosperetti & Lezzi 1986): p p  B n  n  B. (4.13) The values B  3049.13 bars, n  7.15 give an excellent fit to experimental pressure-density relation for water up to 105 bars (Fujikawa & Akamatsu 1980). Here, p and  are the pressure and density in the undisturbed liquid (hydrostatic model). From Eq.(4.13) together with c 2  dp d  , we get c2  n p  B   n   p  B   p  B  1/ n n 1 / n (4.14) and  n 1 / n  c 2  c2 c2   p  B      1 , h   n 1 n  1   p  B    where the definition of c2  n  p  B   (4.15) is the wave speed of the acoustic wave in the undisturbed liquid. Then we expand the enthalpy h and the sound speed c around the equilibrium pressure p using a Taylor series expansion as follows (Prosperetti & Lezzi 1986): h p  p  2 1  p  p   2   ..., 2c    (4.16) 52 1 1 p p  2   n  1 4   .... 2 c c c  4.2.2 Non-dimensional (4.17) formulation of the governing equations We would like to introduce two typical scales Rs and U , where Rs denotes the radius of the scatterer and U   p   1/ 2 stands for the liquid velocity near the scatterer. The dimensionless quantities indicated by asterisk, are given as below: r Rs  r* , t  Rs t* ,   RsU * , h  U 2 h* U c  c c* , p  p   U 2 p* (4.18) (4.19) where the Mach number   U c (is also the small parameter to be used for the perturbation analysis). It is evident that   0 , or otherwise the dimensionless formulation in Eq.(4.18) will have a singularity. From the above, we have: 2   *   *  2 2 U  *  , , U2  U  2 2 Rs r* r r r* t t* (4.20) h U 2 h* h U 3 h*   , . r Rs r* t Rs t* (4.21) Then substituting Eqs.(4.20), (4.21) and (4.19) into (4.11) and (4.12), respectively, we obtain the governing equations in terms of dimensionless variables:  2 * 1  h*  * h*   2 2  0 2 r* r* r*  c*  t* (4.22) 53 2  * 1 2  *    h*  0. t* 2 r* (4.23) We stress that the dimensionless variable r* also stands for the space vector dependent on the dimensional coordinates system be planar, cylindrical or spherical. Next, from Eq.(4.15), the dimensionless speed of sound of the liquid is, c*2  1   2  n  1 h* , (4.24) and the dimensionless enthalpy of the liquid in Eq.(4.15) is given by  n 1 / n  1  p  B   h*  2  1 .    n  1   p  B    1 (4.25) Substituting p  p   U 2 p* and h  U 2 h* into Eq.(4.16) and Eq. (4.17), and referring to the Taylor series expansion, we can get 1 h*  p*   2 p*2  o   2  , 2 (4.26) 1  1   n  1  2 p*  o   2  . 2 c* (4.27) By substituting Eq.(4.26) and Eq.(4.27) into Eq.(4.22), we obtain:   h  2 * h* h     2  *  *   n  1 h* *   o   2   0. 2 r* t* t*   r* r* (4.28) Next, the perturbation expansions for the potential  * and enthalpy h* are defined as follows:  *  r* , t*    *0  r* , t*    2 *1  r* , t*   o   4  , (4.29) h*  r* , t*   h*0  r* , t*    2 h*1  r* , t*   o   4  (4.30) 54 where they are introduced into Eq.(4.23) and Eq.(4.28), respectively. We can get the separate governing equations for the first and second order w.r.t.  2 :  *0  h*0  0 t* (4.31) 2  *1 1  *0   h*1  o   4   0 2 r* t* (4.32)  2 *0 h*0  0 r*2 t* (4.33) h  2 *1 h*1  *0 h*0      n  1 h*0 *0  o   4   0. 2 r* t* r* r* t* (4.34) By combining Eq.(4.31) and Eq.(4.33), Eq.(4.32) and Eq.(4.34), we obtain the fundamental equation for the second order nonlinear acoustic wave (dimensionless formulation) as  2 *0   *0  0 t*2 2 * *2 *1  (4.35)  *0  2 *0  2 *1 1   2        n   o   4   0. (4.36)    1     * *0 * *0 * *0 2 2 t* t* t* t* 2 t* where the Hamilton operator * is defined in terms of r* . As elucidated before, the parameter n is assumed to reasonably match the experimental pressure-density relation for water up to 105 bars at n  7.15 (Fujikawa & Akamatsu 1980). 55 4.3 Analytical solution for the one-dimensionless equation 4.3.1 Analytical solution for plane wave The analytical solutions for the dimensional second-order nonlinear plane wave are shown below (the detailed derivation to obtain the analytical solutions are provided in the Appendix C):  0  A  cos  kr   eit 1  A cos  2kr   e2it  (4.37) i A2  n 1  n 1 kr sin  2kr   cos  2kr   n  3  e2it , 2  8U  4  (4.38) where A , k ,  are the amplitude, wave number, frequency, respectively. 4.3.2 Analytical solution for cylindrical wave The analytical solutions for the dimensional second-order nonlinear cylindrical wave are shown as below:  0  A  H 0 2  kr   eit 1  A  H0 2  2kr   e2it (4.39)          J 2kr  n 1 H  2 kr 2  2 H  2 kr 2  Y 2kr  rdr     0    0  1   2it i A23 2  0   e , 2 2 2U 4   2  2   Y0  2kr     n 1 H0  kr   2 H1  kr   J0  2kr   rdr      (4.40) 4.3.3 Analytical solution for spherical wave The analytical solutions for the dimensional second-order nonlinear spherical wave are shown as below: 56 0  ARs  cos  kr   eit , r ARs  cos  2kr   e 2it r    r   2it i A2 Rs2  kr  n  1  Ci  4kr   2Ci  2kr   ln  sin  2kr  Rs   2 2 2  e . 8U  r   2   kr  n  1  Si  4kr   2Si  2kr   cos  2kr   8cos  kr   (4.41) 1  (4.42) By substituting Eqs.(4.37) and (4.38), Eqs.(4.39) and (4.40), and Eqs.(4.41) and (4.42) into    0   2 1  O   4  , respectively, we obtain the asymptotic expression for the velocity potential up to and including O   2  . 4.4 Results and Discussions The obtained analytical solutions are analyzed with regard to the nonlinear effects around the area where the multiple incident waves are focused. It is important to emphasize that the initial interactions among the multiple sources will not be taken into account since each source is not sufficiently large intensity to induce nonlinear deformation. If one assume the scatterer to be the equilibrium bubble, the Rayleigh-Plesset equation (Franc & Michel 2004) or modified Rayleigh model (Gong et al. 2010) as well as the relationship between the pressure in the fluid and the gas pressure inside the bubble (Matula et al. 2002) (where the nonlinear effects have not taken into account previously), can be employed to describe the bubble cavitation/deformation. Alternatively, we may use the general dimensionless equation dr dt   together with Eqs.(4.41) and (4.42) to construct and express the nonlinear variation of the bubble radius as well. In this work, we shall assume the 57 radius of the scatterer Rs  1 . Since we know that the nonlinear acoustic wave effect will only dominate especially the fluid region and its vicinity outside the scatterer, the distance defined as x or r should larger than the radius of the scatterer ( Rs  1 ); in Second harmonic to fundamental ratio the subsequent analysis the effective distance Re will range from 1 to 100. 0.12 0.09 Planar coordinate Cylindrical coordinate Spherical coordinate 0.06 0.03 0.00 1 2 3 4 Distance from the focused point 5 Figure 4.2: The ratio of the pressure second harmonic to the fundamental term v.s. the variation of the distance away from the focused point By using the analytical solutions for the one dimensional Westervelt equation, the pressure distribution around the scatterer for the fundamental and the second order harmonic of planar, cylindrical and spherical coordinates in water are calculated. Here, in our calculation, the wave speed c is assumed to be 1500m/s, water density   is 1000 kg/m3, nonlinear coefficient  is 3.5, initial pressure P0 is 4 105 Pa, and frequency is f  15000 hz (Pozuelo et al. 1999). (For example, one can interpret the presence of four incident waves at pressure intensity of Pi  105 Pa each. As such, there is the multiple incident waves focusing with linear superposition giving rise to P0  4 105 Pa at the vicinity of the scatterer.) The calculated results for the ratio 58 between the second order harmonic to fundamental (first order term) are displayed in Figure 4.2. It is evident that the general variation depicted in Fig.4.2 are only similar in trend but not in magnitude to that found in reference (Pozuelo et al. 1999). From Eq.(4.5) and Figure 4.2, it is observed that the ratio between second harmonic to first order harmonic for plane wave increase linearly with increasing distance away from the focused point. For the second harmonics of spherical and cylindrical waves, the increase with distance from the focused point, is less important for the waves for the same vibration amplitude of the excitation source. 280 Pressure amplitude(dB) 260 Fundamental-planar Fundamental-cylindrical Fundamental-spherical Second order-planar Second order-cylindrical Second order-spherical 240 220 200 180 160 140 20 40 60 80 Distance from the focused point 100 Figure 4.3: The comparison between the analytical results of planar, cylindrical and spherical wave including the fundamental and the second harmonic Figure 4.3 presents a more explicit comparison between the fundamental and the second order harmonic pressure amplitudes in planar, cylindrical and spherical coordinates. According to the definition of the pressure level (dB) set at 20 log10  p / preference  , we can plot the pressure level distribution w.r.t. the distance 59 away from the focused point (the reference pressure is assumed to be 10-6 Pa). The calculated pressure amplitude variation shown in Fig. 4.3 can be compared to the results obtained by (Pozuelo et al. 1999). From Fig.4.3, it is observed that the second order harmonic distribution for the planar wave will increase, the second order harmonic distribution of cylindrical wave seems to be constant while the second order for the harmonic spherical wave will initially increase slightly and then decrease with the increment of the distance away from the focused point. The results from (Pozuelo et al. 1999) indicate fairly similar trend but the respective magnitudes are quite different. Pressure amplitude(dB) 250 240 230 Summation for planar wave Summation for cylindrical wave Summation for spherical wave 220 210 200 190 20 40 60 80 Distance from the focused point 100 Figure 4.4: The variation of pressure amplitude v.s. the distance away from the focused point for the planar, cylindrical and spherical wave The summation of the fundamental and the second order term are shown in Figure 4.4. It is observed that the amplitude for the cylindrical and spherical wave decrease monotonically. On the contrary, the pressure amplitude will increase with 60 distance away the focused point for the model of planar wave. Hence, accordingly, it is deemed not reasonable to describe the focused HIFU around the scatterer by the planar wave. It is clear that within the distance of less than 10, the decrease of the aggregate pressure amplitudes of cylindrical and spherical wave appear to be very fast and the tendency to moderate beyond this point for the region between 10 to 100. Being so, one can suggest that the domain encompassing less than ten times of the radius of the scatterer, the non-linear effect exert a significant influence on the focused high intensity acoustic wave. Next, we shall discuss the nonlinear effect for the focused acoustic wave with the small parameter Mach number by compressible potential flow theory. We will assume the amplitude of velocity potential A  1 , and radius of the scatter Rs  1 (the details for the planar, cylindrical and spherical wave can be found in the Appendix C). As interpreted earlier, *r*  kr is defined as the dimensionless wave number and the velocity potential is only depend on the variable U in the frequency domain and the small parameter   U c ( c is a constant at 1500m/s ). For the numerical calculations, we shall take the dimensionless wave number as kRs  1.0, 3.0 and 5.0 and the small parameter Mach number  as 0.1, 0.3 and 0.5, so that U   c becomes 150, 450 and 750, respectively. Figure 4.5 shows the variation of the second order term of plane wave w.r.t. the increase of the distances from the focused point for different parameters. It is evident that with the increase of the wave number k (shown as the horizontal columns), we can find that the general tendency of the amplitude for the second order term to increase and the variation takes on shorter 61 periodic time. For the fixed low wave number of k  1.0 (first column in Fig.4.5), the increase of the Mach number (   0.1, 0.3 and 0.5) can bring about comparatively large amplitude for the second order term. However, the maximum amplitude for each second term appears to be constant without any variation w.r.t. the increase of distance from the focused point. This phenomena can be interpreted as that the low frequency stands for quasi-static model, and thus the variation of the distances have lesser influence on the second-order nonlinear term. At the high frequency of k  5.0 (third column in Fig.4.5), the maximum amplitudes tend to increase w.r.t. the position away from the focused point. 0.35 0.20 0.15 0.10 0.30 0.25 0.20 0.15 0.10 0.05 0.05 0.00 0.00 20 0.40 k=1.0, =0.3 0.35 0.30 0.25 0.20 0.15 0.10 0.05 0.00 0.40 20 0.20 0.15 0.10 0.05 5 10 15 Distance from the focused point 20 0.00 0.40 k=3.0, =0.3 0.30 0.25 0.20 0.15 0.10 0.00 0.40 k=1.0, =0.5 0.35 0.30 S e con d o rde r term S e co n d o rd e r te rm 0.35 0.25 0.35 0.05 5 10 15 Distance from the focused point 0.25 0.20 0.15 0.10 0.15 0.10 0.00 20 20 20 k=5.0, =0.3 0.30 0.25 0.20 0.15 0.10 0.00 0.40 k=3.0, =0.5 0.20 0.05 5 10 15 Distance from the focused point 5 10 15 Distance from the focused point 0.25 0.00 5 10 15 Distance from the focused point 0.05 0.30 0.05 k=5.0, =0.1 0.30 0.35 S econ d o rd er term 0.35 5 10 15 Distance from the focused point 0.35 S ec on d ord er te rm 0.25 k=3.0, =0.1 S e c o n d o rd e r te rm S ec o nd o rd e r te rm 0.30 0.40 S eco nd o rd er term k=1.0, =0.1 S econ d o rd er term S econ d o rd e r te rm 0.35 0.40 0.40 0.40 5 10 15 Distance from the focused point 20 k=5.0, =0.5 0.30 0.25 0.20 0.15 0.10 0.05 5 10 15 Distance from the focused point 20 0.00 5 10 15 Distance from the focused point 20 Figure 4.5: The variation of the second order term of plane wave v.s. the variation of wave number k , Mach number  and the distance away from the focused point. 62 Second order term 0.15 (a) 0.10 0.05 0.00 Second order term 0.15 5 10 15 Distance from the focused point (b) 20 k=3.0, =0.1 k=3.0, =0.3 k=3.0, =0.5 0.10 0.05 0.00 5 10 15 Distance from the focused point 0.15 (c) Second order term k=1.0, =0.1 k=1.0, =0.3 k=1.0, =0.5 20 k=5.0, =0.1 k=5.0, =0.3 k=5.0, =0.5 0.10 0.05 0.00 5 10 15 Distance from the focused point 20 Figure 4.6: The variation of the second order term for cylindrical wave v.s. the different wave number, Mach number and the distance away from the focused point. 63 1.0 (a) Second order term 0.8 k=1.0, =0.1 k=1.0, =0.3 k=1.0, =0.5 0.6 0.4 0.2 0.0 5 10 15 Distance from the focused point 7 (b) Second order term 6 5 20 k=3.0, =0.1 k=3.0, =0.3 k=3.0, =0.5 4 3 2 1 0 7 Second order term 6 5 5 10 15 Distance from the focused point (c) 20 k=5.0, =0.1 k=5.0, =0.3 k=5.0, =0.5 4 3 2 1 0 5 10 15 Distance from the focused point 20 Figure 4.7: The variation of the second order term for spherical wave v.s. the different wave number, Mach number and the distance away from the focused point. Figure 4.6 illustrate the variation of the nonlinear effect for cylindrical wave at different wave number, Mach number and distance away from the focused point. The 64 general tendency is that with the increase of the distance away from the focused point, this result in ever smaller amplitude for the second order term. For the fixed wave number k , the increase of the Mach number will bring about a larger amplitude for the second order term. With the fixed higher Mach number (   0.5), the increment of the wave number can also weaken the amplitude for the second order term. Velocity potential distribution 2.5 2.0 Summation of planar wave Summation of cylindrical Summation of spherical 1.5 1.0 0.5 0.0 5 10 15 Distance from the focused point 20 Figure 4.8: The velocity potential distribution near the scatterer (the summation of the first order term and the second order term) at k  2.0 and   0.3 Figure 4.7 shows the variation of the nonlinear effect for the spherical wave for the different wave number, Mach number and distance away from the focused point. Similar to that observed for the cylindrical wave, the general tendency is that the increase of the distance away from the focused point will result in smaller amplitude for the second order term. At the fixed low frequency of k  1.0, the increase of the Mach number (   0.1, 0.3 and 0.5) will bring about a larger amplitude for the second order term. Conversely, at the higher frequencies of k  3.0 and 65 k  5.0, a lower Mach number results in stronger nonlinear effects and this trend is very different from the cylindrical wave. Finally, Figure 4.8 give the total velocity potential (the summation of the first order term and the second order term) at k  2.0 and   0.3. We can observe the variation of the velocity potential for both the cylindrical wave and spherical wave appear to be consistent with the conclusion from the Westervelt model for the pressure distribution. The general tendency of the velocity potential will decrease w.r.t. the increase of the distance away from the focused point while the amplitude of the velocity potential for the planar wave seem to be periodic constant. For the spherical wave, since our analytical solution is expressed by cosine/sine function (or cosine/sine integral function) rather than the exponential function, a characteristic feature of this functional is a periodic rather than monotonic curve as from the Westervelt equation. 66 4.5 Conclusions In this study, we adopted two nonlinear models to investigate the multiple incident acoustic waves focused on certain domain where the nonlinear effect is not negligible in the vicinity of the scatterer. The general solutions for the one dimensional Westervelt equation with different coordinates (plane, cylindrical and spherical) were analytically obtained based on the perturbation method with keeping only the second order nonlinear terms. By introducing the small parameter (Mach number), we applied the compressible potential flow theory and proposed a novel dimensionless formulation and asymptotic perturbation expansion for the velocity potential and enthalpy which is different from the existing fractional nonlinear acoustic models (eg. the Burgers equation, KZK equation and Westervelt equation). Our analytical solutions and numerical calculations have shown the general tendency of the velocity potential and pressure to decrease w.r.t. the increase of the distance away from the focused point. At least, within the region which is about 10 times the radius of the scatterer, the non-linear effect exerts a significant influence on the distribution of the pressure and velocity potential. It is also interesting that at high frequencies, lower Mach numbers appear to bring out even stronger nonlinear effects for the spherical wave. Our novel approach with a small parameter for the cylindrical and spherical waves could serve as an effective analytical model to simulate the focused nonlinear acoustic near the scatterer in an ideal fluid and be applied to study bubble cavitation dynamic associated with HIFU in our future work. 67 Chapter 5 Overall Conclusions and Recommendations 5.1 Conclusions In this thesis, we analytically applied two novel methods shown as conformal mapping and perturbation to solve linear/nonlinear acoustic wave propagating through ideal fluid with inclusion inside. The robustness and versatility of our methods were verified by comparing with some calculated results from other published literatures. The major contributions of this thesis can be summarized as below: First of all, we analytically obtained the two dimensional general solution of Helmholtz equation, shown as fractional order Bessel function with mapping function as the argument, to study the linear acoustic wave scattering by rigid inclusion with irregular cross section in an ideal fluid. Based on the conformal mapping method together with the complex variables method, we can map the initial geometry into a circular shape as well as transform the original physical vector into corresponding new expressions in the mapping plane. This study may provide the basis for further analyses of other conditions of acoustic wave scattering in fluids, e.g. irregular elastic inclusion within fluid with viscosity, etc. Our calculated results have shown that the angle and frequency of the incident waves have significant influence on the bistatic scattering pattern as well as the far field form factor for the pressure in the fluid. Moreover, we have shown that the sharper corners of the irregular inclusion may amplify the bistatic scattering pattern compared with the more rounded corners. 68 Separately, we further use the perturbation method to solve the one dimensional nonlinear acoustic wave propagating through the infinite domain with a submersible inclusion. In fact, we adopted two nonlinear models to investigate the multiple incident acoustic waves focused on certain domain where the nonlinear effect is not negligible in the vicinity of the scatterer. The general solutions for the one dimensional Westervelt equation with different coordinates (plane, cylindrical and spherical) are analytically obtained based on the perturbation method with keeping only the second order nonlinear terms. By introducing the small parameter (Mach number), we applied the compressible potential flow theory and proposed a novel dimensionless formulation and asymptotic perturbation expansion for the velocity potential and enthalpy which is different from the existing more fractional nonlinear acoustic models (eg. the Burgers equation, KZK equation and Westervelt equation). Our analytical solutions and numerical calculations have shown that the general tendency of the velocity potential and pressure to decrease w.r.t. the increase of the distance away from the focused point. At least, within the region which is about 10 times the radius of the scatterer, the non-linear effect exerts a significant influence on the distribution of the pressure and velocity potential. It is also interesting that at high frequencies, lower Mach numbers appear to bring out even stronger nonlinear effects for the spherical wave. Our approach with small parameter for the cylindrical and spherical waves could serve as an effective analytical model to simulate the focused nonlinear acoustic near the scatterer in an ideal fluid and be applied to study bubble cavitation dynamic associated with HIFU in future work. 69 5.2 Recommendations To the best of our knowledge, we would like to point out that the conformal mapping together with complex variables method can only handle the two dimensional problem, however, it may be an effective approach to solve the geometries with sharp corners. On the perturbation method, it is an effective means to obtain the asymptotic solution of some complex problem, in particularly, to provide the physical analysis to give qualitative insight. At this stage, we would like to propose several interesting and possible works to be done in the future: 1. 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Amsterdam, The Netherlands: Elsevier. 79 Appendix A Partial Coding for Linear Acoustic Wave Propagation Relate to Conformal Mapping Method Code 1: clear; T=1.0; R=1.0; % 0.7 r=1.0; % 1.3 q=2; p=1/2; b=5; a=1/b; d=6; c=1/d; liu=0; for sita=0:0.01:2*pi; liu=liu+1 S(liu)=sita/2/pi*360; w(liu)=abs(R*(r*exp(i*sita)+p/(r*exp(i*sita))^q)); M(liu)=real(R*(r*exp(i*sita)+p/(r*exp(i*sita))^q)); N(liu)=imag(R*(r*exp(i*sita)+p/(r*exp(i*sita))^q)); w1(liu)=abs(R*(r*exp(i*sita)+a/(r*exp(i*sita))^b)); M1(liu)=real(R*(r*exp(i*sita)+a/(r*exp(i*sita))^b)); N1(liu)=imag(R*(r*exp(i*sita)+a/(r*exp(i*sita))^b)); w2(liu)=abs(R*(r*exp(i*sita)+c/(r*exp(i*sita))^d)); M2(liu)=real(R*(r*exp(i*sita)+c/(r*exp(i*sita))^d)); N2(liu)=imag(R*(r*exp(i*sita)+c/(r*exp(i*sita))^d)); end Code 2: clear; r=1.0; c1=1/2; % 1/9 , 1/5, 1/3, 1/2 80 a1=1/3; % 1/3, 1/6 ,1/9 a2=1/15; % 1/15, 2/15, 7/45 liu=0; for sita=0:0.01:2*pi; liu=liu+1 S(liu)=sita/2/pi*360; w(liu)=abs((r*exp(i*sita))^(-1)+c1*(r*exp(i*sita))^2); M(liu)=real((r*exp(i*sita))^(-1)+c1*(r*exp(i*sita))^2); N(liu)=imag((r*exp(i*sita))^(-1)+c1*(r*exp(i*sita))^2); w1(liu)=abs((r*exp(i*sita))^(-1)+a1*(r*exp(i*sita))^2+a2*(r*exp(i*sita))^5); M1(liu)=real((r*exp(i*sita))^(-1)+a1*(r*exp(i*sita))^2+a2*(r*exp(i*sita))^5); N1(liu)=imag((r*exp(i*sita))^(-1)+a1*(r*exp(i*sita))^2+a2*(r*exp(i*sita))^5); w2(liu)=abs((r*exp(i*sita))^(1)+c1*(r*exp(i*sita))^(-2)); M2(liu)=real((r*exp(i*sita))^(1)+c1*(r*exp(i*sita))^(-2)); N2(liu)=imag((r*exp(i*sita))^(1)+c1*(r*exp(i*sita))^(-2)); w3(liu)=abs((r*exp(i*sita))^(1)+a1*(r*exp(i*sita))^(-2)+a2*(r*exp(i*sita))^(-5)); M3(liu)=real((r*exp(i*sita))^(1)+a1*(r*exp(i*sita))^(-2)+a2*(r*exp(i*sita))^(-5)); N3(liu)=imag((r*exp(i*sita))^(1)+a1*(r*exp(i*sita))^(-2)+a2*(r*exp(i*sita))^(-5)); end Code 3: clear; fpi=0; % sita angle mk=300; % the division of the angle hh=2*pi/mk; % the step w0=1; % pressure amplitude mu=0.0; % damping constant rou=1.0; % stands for the density of the fluid nn=2.0; %%%%%%%%%%%%%%%%% incident wave number kd=nn; % nn*pi; % K of the function oumiga=kd*1480; % incident frequency a0=3*pi/4; %%%%%%%%%%%%%%%%% incident angle pi, 3*pi/4, pi/2 R=1.0; % 0.75; q=2; % 2; 3 p=1/q; % 1/q; % canonical ellipse R=0.75 p=1/3; r=1.0; % radius of the circle 1.0 or 1.3 a=100; nnn1=7; %terms of the series 81 for n=1-nnn1:nnn1-1; for m=1-nnn1:nnn1-1; z=r*exp(i*fpi); wz=R*(z+p/z^q); sz=R*(1-p*q/z^(q+1)); xx11=kd*abs(wz); t=0; t1=(besselh(m-1,xx11)*(wz/abs(wz))^(m-1)*exp(i*fpi)*sz/abs(sz)-besselh(m+1,xx11)*(wz/abs( wz))^(m+1)*exp(-i*fpi)*conj(sz)/abs(sz))*exp(-i*n*fpi)/(2*pi); for k=1:mk; ct=fpi+k*hh; z=r*exp(i*ct); wz=R*(z+p/z^q); sz=R*(1-p*q/z^(q+1)); xx11=kd*abs(wz); t2=(besselh(m-1,xx11)*(wz/abs(wz))^(m-1)*exp(i*ct)*sz/abs(sz)-besselh(m+1,xx11)*(wz/abs( wz))^(m+1)*exp(-i*ct)*conj(sz)/abs(sz))*exp(-i*n*ct)/(2*pi); tt=(t1+t2)/2; t=t+tt*hh; t1=t2; end; slb(n+nnn1,m+nnn1)=t; end end % for n=1-nnn1:nnn1-1; z=r*exp(i*fpi); wz=R*(z+p/z^q); sz=R*(1-p*q/z^(q+1)); t=0; t1=-i*w0*exp(i*kd/2*(wz*exp(-i*a0)+conj(wz)*exp(i*a0)))*(exp(i*fpi)*sz/abs(sz)*exp(-i*a0)+exp( -i*fpi)*conj(sz)/abs(sz)*exp(i*a0))*exp(-i*n*fpi)/(2*pi);% for k=1:mk; ct=fpi+k*hh; z=r*exp(i*ct); wz=R*(z+p/z^q); sz=R*(1-p*q/z^(q+1)); t2=-i*w0*exp(i*kd/2*(wz*exp(-i*a0)+conj(wz)*exp(i*a0)))*(exp(i*ct)*sz/abs(sz)*exp(-i*a0)+exp(i*ct)*conj(sz)/abs(sz)*exp(i*a0))*exp(-i*n*ct)/(2*pi);% tt=(t1+t2)/2; 82 t=t+tt*hh; t1=t2; end; srb(n+nnn1)=-t; end bn=slb\srb'; %%%%%%%% below is the velocity and pressure inside the fluid Q=0; for ppii=0:0.1:360; % the azimuthal along the solid surface Q=Q+1 ppi=ppii/180*pi; liu(Q)=ppii; gang(Q)=ppi; f=a*exp(i*ppi); wf=R*(f+p/f^q); sf=R*(1-p*q/f^(q+1)); xx22=kd*abs(wf); usitai=-w0/2*kd*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0)))*(exp(i*ppi)*sf/abs(sf)*exp(-i*a0) -exp(-i*ppi)*conj(sf)/abs(sf)*exp(i*a0)); pai=rou*(i*oumiga+mu)*w0*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0))); faii=w0*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0))); usitas=0; pas=0; fpas=0; fais=0; for m=1-nnn1:nnn1-1; usitas=usitas+i*kd/2*bn(m+nnn1).*(besselh(m-1,xx22)*(wf/abs(wf))^(m-1)*exp(i*ppi)*sf/abs(sf) +besselh(m+1,xx22)*(wf/abs(wf))^(m+1)*exp(-i*ppi)*conj(sf)/abs(sf)); pas=pas+rou*(i*oumiga+mu)*bn(m+nnn1).*besselh(m,xx22)*(wf/abs(wf))^m; fpas=fpas+rou*(i*oumiga+mu)*bn(m+nnn1).*(-i)^m*(2/(pi*kd*abs(wf)))^(1/2)*exp(i*(kd*abs(wf) -pi/4)); fais=fais+bn(m+nnn1).*besselh(m,xx22)*(wf/abs(wf))^m; end usita(Q)=abs((usitai+usitas)/kd/w0); pa(Q)=abs(pai+pas); coeff(Q)=abs(pas/pai); fpa(Q)=abs(fpas); fai(Q)=abs(faii+fais); end 83 Code 4 clear; fpi=0; mk=300; hh=2*pi/mk; w0=1; mu=0.0; rou=1.0; nn=2.0; kd=nn; oumiga=kd*1480; a0=pi/2; %%%%%%%%%%%%%%%incident angle pi, 3*pi/4, pi/2 c1=1/3; % 1/5, 1/3, 1/2, 1/3, 1/6, 1/9 c2=1/15; c3=0; % 0, 0, 0, 1/15, 2/15, 7/45 %0 r=1.0; a=100; nnn1=7; for n=1-nnn1:nnn1-1; for m=1-nnn1:nnn1-1; z=r*exp(i*fpi); wz=z+c1*z^(-2)+c2*z^(-5)+c3*z^(-8); sz=1-2*c1*z^(-3)-5*c2*z^(-6)-8*c3*z^(-9); xx11=kd*abs(wz); t=0; t1=(besselh(m-1,xx11)*(wz/abs(wz))^(m-1)*exp(i*fpi)*sz/abs(sz)-besselh(m+1,xx11)*(wz/abs( wz))^(m+1)*exp(-i*fpi)*conj(sz)/abs(sz))*exp(-i*n*fpi)/(2*pi); for k=1:mk; ct=fpi+k*hh; z=r*exp(i*ct); wz=z+c1*z^(-2)+c2*z^(-5)+c3*z^(-8); sz=1-2*c1*z^(-3)-5*c2*z^(-6)-8*c3*z^(-9); xx11=kd*abs(wz); t2=(besselh(m-1,xx11)*(wz/abs(wz))^(m-1)*exp(i*ct)*sz/abs(sz)-besselh(m+1,xx11)*(wz/abs( wz))^(m+1)*exp(-i*ct)*conj(sz)/abs(sz))*exp(-i*n*ct)/(2*pi); tt=(t1+t2)/2; t=t+tt*hh; t1=t2; end; slb(n+nnn1,m+nnn1)=t; end end 84 for n=1-nnn1:nnn1-1; z=r*exp(i*fpi); wz=z+c1*z^(-2)+c2*z^(-5)+c3*z^(-8); sz=1-2*c1*z^(-3)-5*c2*z^(-6)-8*c3*z^(-9); t=0; t1=-i*w0*exp(i*kd/2*(wz*exp(-i*a0)+conj(wz)*exp(i*a0)))*(exp(i*fpi)*sz/abs(sz)*exp(-i*a0)+exp( -i*fpi)*conj(sz)/abs(sz)*exp(i*a0))*exp(-i*n*fpi)/(2*pi); for k=1:mk; ct=fpi+k*hh; z=r*exp(i*ct); wz=z+c1*z^(-2)+c2*z^(-5)+c3*z^(-8); sz=1-2*c1*z^(-3)-5*c2*z^(-6)-8*c3*z^(-9); t2=-i*w0*exp(i*kd/2*(wz*exp(-i*a0)+conj(wz)*exp(i*a0)))*(exp(i*ct)*sz/abs(sz)*exp(-i*a0)+exp(i*ct)*conj(sz)/abs(sz)*exp(i*a0))*exp(-i*n*ct)/(2*pi); tt=(t1+t2)/2; t=t+tt*hh; t1=t2; end; srb(n+nnn1)=-t; end bn=slb\srb'; %%%%%%%%%%%%%%%% below is the velocity and pressure inside the fluid Q=0; for ppii=0:0.1:360; Q=Q+1 ppi=ppii/180*pi; liu(Q)=ppii; gang(Q)=ppi; f=a*exp(i*ppi); wf=f+c1*f^(-2)+c2*f^(-5)+c3*f^(-8); sf=1-2*c1*f^(-3)-5*c2*f^(-6)-8*c3*f^(-9); xx22=kd*abs(wf); usitai=-w0/2*kd*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0)))*(exp(i*ppi)*sf/abs(sf)*exp(-i*a0) -exp(-i*ppi)*conj(sf)/abs(sf)*exp(i*a0)); pai=rou*(i*oumiga+mu)*w0*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0))); faii=w0*exp(i*kd/2*(wf*exp(-i*a0)+conj(wf)*exp(i*a0))); usitas=0; pas=0; fpas=0; fais=0; for m=1-nnn1:nnn1-1; 85 usitas=usitas+i*kd/2*bn(m+nnn1).*(besselh(m-1,xx22)*(wf/abs(wf))^(m-1)*exp(i*ppi)*sf/abs(sf) +besselh(m+1,xx22)*(wf/abs(wf))^(m+1)*exp(-i*ppi)*conj(sf)/abs(sf)); pas=pas+rou*(i*oumiga+mu)*bn(m+nnn1).*besselh(m,xx22)*(wf/abs(wf))^m; fpas=fpas+rou*(i*oumiga+mu)*bn(m+nnn1).*(-i)^m*(2/(pi*kd*abs(wf)))^(1/2)*exp(i*(kd*abs(wf) -pi/4)); fais=fais+bn(m+nnn1).*besselh(m,xx22)*(wf/abs(wf))^m; end usita(Q)=abs((usitai+usitas)/kd/w0); pa(Q)=abs(pai+pas); coeff(Q)=abs(pas/pai); fpa(Q)=abs(fpas); fai(Q)=abs(faii+fais); end 86 Appendix B Neglecting the terms of third or higher orders, we can obtain the approximate formulate of Westervelt equation as below:  2  p1  p2   2 1   p1  p2    2 p12   0. t 2 c2  c4 t 2 (B1) Here, we can set two separated governing equations for the first linear solution of p1 and following inhomogeneous equation with second order correction p2 :  2 p1  1  2 p1  0, c2 t 2 (B2)  2 p2  1  2 p2   2 p12 .    c4 t 2 c2 t 2 (B3) Here, we can take the harmonic problem into account and assume p1  P1 exp  it  , p2  P2 exp  2it  , so we can obtain the reduced governing equation as below:  2 P1  k 2 P1  0,  2 P2  4k 2 P2  (B4) 4k 2  2 P .  c2 1 (B5) In summary, we need to obtain the solutions of the above Eq. (B5) and get the detail expressions for P1 and P2 , and the total pressure will be shown as p  P1 exp  it   P2 exp  2it  . 87 Analytical Solution for Plane wave The simplest and best studies case is the plane wave propagation. Various explicit solutions can be found in the literatures. For the condition of one dimensional problem in Cartesian coordinates, the governing equation can be reduced into: d 2 P1  k 2 P1  0, dx 2 (B6) d 2 P2 4k 2  2 2   4 k P P . 2 dx 2  c2 1 (B7) For the harmonic excitation of amplitude P0 , the acoustic pressure is assumed to be an addition of two terms. The analytical solutions which have the form were obtained: P1  P0  e  ikx , P2   P02  1  2ikx   e 2ikx . 2   c2 (B8) (B9) Analytical Solution for Cylindrical Wave The acoustic wave propagation expansion in the polar coordinate with one-dimensional will make the governing equation as below: d 2 P1 1 dP1   k 2 P1  0, dr 2 r dr (B10) d 2 P2 1 dP2 4k 2  2 2    4 k P P . 2 dr 2 r dr  c2 1 (B11) It is easy to find that Eq.(B10) is the zero order Bessel function with the variable as kr , and the solution is that: 88 P1  P0  J 0  kr  or P0  H 0  kr  . (B12) According to this certain problem, we can assume the particular solution basing on the time term as exp  it  : P1  P0  H 0 2  kr  , (B13) when r   , the asymptotic expression of Eq.(B13) will turn to be: P1  P0  2  i kr  4  e  .  kr (B14) Substituting Eq.(B14) into Eq.(B11), we can obtain: 8k  P02 e 2i kr  d 2 P2 1 dP2 2    4 k P 2 dr 2 r dr  c2 r 4 , (B15) Subsequently, we need to get the analytical solution of the second-order correction as shown in Eq.(B15). Here, it is straight forward for us to obtain the analytical solution as below: P2  4i  P02 i 2 2ikr e e .  c2 (B16) Analytical Solution for Spherical Wave For the condition of one dimensional problem in spherical coordinates, the governing equation can be reduced into: d 2 P1 2 dP1   k 2 P1  0, 2 dr r dr (B17) d 2 P2 2 dP2 4k 2  2 2   4k P2  P . dr 2 r dr  c2 1 (B18) 89 The solution of Eq.(B17) in spherical coordinate can be shown as below: P1  P0  ikr e . r (B19) Where P0 is the amplitude of the incident pressure. It is also easy to observe that when r   , the pressure P1 gradually decreased into infinitesimal. Substituting Eq.(B19) into the non-homogeneous term, the following wave equation for the second order correction P2 is obtained: 4 k 2 P02 2ikr d 2 P2 2 dP2 2   4k P2  e , dr 2 r dr  c2 r 2 (B20) The following solution was proposed to satisfy Eq.(B20):  ln r   n  n P2    n2 r  r  2ikr e ,  (B21) By substituting Eq.(B21) into Eq.(B20), we can obtain the approximate solutions of the unknown coefficients  and  n can be:  i  kP02 ,  c2 (B22)  1  n  2 ! , n   n 1  4ik  n (B23) So we can obtain the approximated analytical solution for the second order Eq.(B20) as below: n i  kP02  ln r   1  n  2  !  2ikr  P2   e .  c2  r n  2  4ik n 1 r n  (B24) 90 Actually, this solution is asymptotic one, and when n   as well as the increase of the r will make the solution to be more accurate. 91 Appendix C Analytical Solution for Plane Wave For the one dimensional plane wave, the governing equations are (the higher order small terms will be omitted subsequently):  2 *0  2 *0   0, r*2 t*2 (C1) 2  *0  2 *0  2 *1  2 *1 1    *0   *0  2 *0 n 1 .          2 t*  r*  r*2 t*2 r* r*t* t* t*2 (C2) Here, we would like to point out that r* can be directly insteaded by the Cartesian coordinate x* for the plane wave. We propose the one dimensionless solution for the linear acoustic wave in Eq.(C1) as below:  *0  A* cos  k*r*    ei t  A* cos *r*   ei t ** ** (C3) where A* , k* , * are the dimensionless amplitude, wave number, frequency, respectively, and defined as: A*  R A  U , k*  Rs k , *  s  , r*  r , t*  t. RsU Rs Rs U (C4) It is evident that Eq.(C3) is a solution of Eq.(C1). By substituting Eq.(C3) into Eq.(C2) and assuming that  *1  *1  r*   e 2i*t* , we obtain the simplified second-order non-homogeneous differential equation as:  2*1  4*2*1  2iA*2*3 sin 2 *r*   i  n  1 A*2*3 cos 2 *r*  . 2 r* (C5) 92 The general analytical solution for this second-order non-homogeneous Eq.(C5) is: *1  C1 cos  2*r*   e2i t  C2 sin  2*r*   e2i t **  ** i* A*2  n 1  cos  2*r*   n  3  e2i*t* .   n 1 *r* sin  2*r*   8  4  (C6) where, C1 and C2 are unknown coefficients to be determined by the imposed boundary conditions. For simplicity in the discussion below, the coefficients for the second-order nonlinear terms can be reasonably assumed as C1  A* , C2  0 without loss of generality. Analytical Solution for Cylindrical Wave For the one dimension cylindrical wave, the governing equations are:  2 *0 1  *0  2 *0    0, r* r* r*2 t*2 (C7) 2  *0  2 *0  2 *1 1  *1  2 *1 1    *0   *0  2 *0 .      n  1    r* r* 2 t*  r*  r*2 t*2 r* r*t* t* t*2 (C8) The proposed solution for the linear acoustic wave (second kind of Hankel function with zero order) is assumed as:  *0  A* H 0 2 *r*   ei t (C9) ** By substituting Eq.(C9) into Eq.(C8) and assuming  *1  *1  r*   e 2i*t* , we obtain the simplified second-order non-homogeneous differential equation as: 2 2 2*1 1 *1  2  2 2 2 3 2 3 4 2 iA H r i n 1 A H r ,                  * *1 * * 1 ** * * 0 ** r*2 r* r*     (C10) and the analytical solution is (the softwave named MAPLE will be used here): 93 *1  C1  J0  2*r*   e2i t  C2 Y0  2*r*   e2i t **  **         J 2 r  n 1 H  2  r 2  2 H  2  r 2 Y 2 r  r dr   * *    0  * * 1  * * 0 * * * *  (C11) i A  0   e2i*t* .   2 2 2   2  2   Y0  2*r*     n 1 H0 *r*   2 H1 *r*   J0  2*r*   r*dr*    3 2 * *   Here, J 0   is the Bessel function of order zero, Y0   is the second kind of Bessel 2 function of order zero, and H 0     J 0    iY0   is second kind Hankel function with order zero. For ease of discussion and without loss of generality, one can reasonably assumed that C1  A* and C2  iA* . Analytical Solution for Spherical Wave For the one dimension spherical wave, the governing equations are:  2 *0 2  *0  2 *0    0, r* r* r*2 t*2 (C12) 2  *0  2 *0  2 *1 2  *1  2 *1 1    *0   *0  2 *0 .      n  1    r* r* 2 t*  r*  r*2 t*2 r* r*t* t* t*2 (C13) Again, the solution for the linear acoustic wave is assumed as:  *0  A* cos *r*   ei*t* . r* (C14) By substituting Eq.(C14) into Eq.(C13) and assuming  *1  *1  r*   e 2i*t* , we have: 2 2*1 2 *1   4*2*1  2iA*2*  r*2 cos*r*   r*1* sin *r*   i  n 1 A*2*3r*2 cos2 *r*  , (C15) 2 r* r* r* In which the analytical solution is: 94  *1  C1 C cos  2*r*   e 2i*t*  2 sin  2*r*   e 2i*t* r* r* (C16)  i* A*2  *r*  n  1  Ci  4*r*   2Ci  2*r*   ln r*  sin  2*r*  2 i*t*  e  . 8r*2  *r*  n  1  Si  4*r*   2 Si  2*r*   cos  2*r*   8cos 2 *r*     where Ci and Si stand for the Cosine Integral and Sine Integral function, respectively. As before, C1 and C2 are unknown coefficients to be solved based on imposed boundary conditions. For simplicity, we shall assume C1  A* and C2  0 . Since we have assumed r  p  p  U 2 p* , A*  Rs  r* , t  Rs t* ,   RsU * , h  U 2 h* , c  c c* , U R A U  U  t , r*  r ,   , *  s  , t*  , k , the c c RsU Rs Rs U waves above can be transformed accordingly to the one dimensional plane wave as:  0  A cos  kr   eit 1  Acos  2kr   e2it  (C17) i A2  n 1  n 1 kr sin  2kr   cos  2kr   n  3  e2it , 2  8U  4  (C18) the one dimensional cylindrical wave as  0  A  H 0 2  kr   eit 1  A  H0 2  2kr   e2it (C19)          J 2kr  n 1 H  2 kr 2  2 H  2 kr 2  Y 2kr  rdr     0    0  1   2it i A    0   e , 2 2 2U 4   2  2   Y0  2kr     n 1 H0  kr   2 H1  kr   J0  2kr   rdr    2 3 2   (C20) and the one dimensional spherical wave as 0  ARs cos  kr   eit , r (C21) 95 ARs cos  2kr   e2it r    r   2it i A2 Rs2  kr  n  1  Ci  4kr   2Ci  2kr   ln  sin  2kr  Rs   2 2 2  e . 8U  r   2  kr  n  1  Si  4kr   2Si  2kr   cos  2kr   8cos  kr   1  (C22)   The total velocity potential is then    0   2 1  O  4 . 96 Appendix D Partial Coding for the Nonlinear Acoustic Wave Propagation Code 1: clear; p0=4*10^5; c=1500; f=15000; w=2*pi*f; k=w/c; rou=1000; bt=3.5; t=0; liu=0; for x=1.01:0.1:5.01; liu=liu+1 gang(liu)=x; pp1(liu)=abs(p0*exp(-i*k*x)*exp(i*w*t)); pp2(liu)=abs(bt*p0^2/2/rou/c^2*(1+2*i*k*x)*exp(-2*i*k*x)*exp(2*i*w*t)); pp(liu)=abs(p0*exp(-i*k*x)*exp(i*w*t)+bt*p0^2/2/rou/c^2*(1+2*i*k*x)*exp(-2*i*k*x)*exp(2*i*w*t)) ; Rapp(liu)=abs(pp2/pp1); ppc1(liu)=abs(p0*besselh(0,2,k*x)*exp(i*w*t)); % k*(x-1.0) ppc2(liu)=abs(2*i*bt*k*x/rou/c^2*(p0*besselh(0,2,k*x)*exp(i*w*t))^2); ppc(liu)=abs(p0*besselh(0,2,k*x)*exp(i*w*t)+2*i*bt*k*x*p0^2/rou/c^2*(besselh(0,2,k*x))^2*exp( 2*i*w*t)); Rappc(liu)=abs(ppc2/ppc1); s=0; for n=2:1:100; s=s+(-1)^n*gamma(n-1)/(4*i*k)^(n-1)/x^n; end LL(liu)=s; ps1(liu)=abs(p0/x*exp(-i*k*x)*exp(i*w*t)); ps2(liu)=abs(i*bt*k*p0^2/rou/c^2*(log(x)/x+LL(liu))*exp(-2*i*k*x)*exp(2*i*w*t)); ps(liu)=abs(p0/x*exp(-i*k*x)*exp(i*w*t)+i*bt*k*p0^2/rou/c^2*(log(x)/x+LL(liu))*exp(-2*i*k*x)*exp 97 (2*i*w*t)); Raps(liu)=abs(ps2/ps1); end Code 2: clear; p0=4*10^5; c=1500; f=15000; w=2*pi*f; k=w/c; rou=1000; bt=3.5; t=0; liu=0; for x=1.01:0.1:5.01; liu=liu+1 gang(liu)=x; pp1(liu)=abs(p0*exp(-i*k*x)*exp(i*w*t)); pp2(liu)=abs(bt*p0^2/2/rou/c^2*(1+2*i*k*x)*exp(-2*i*k*x)*exp(2*i*w*t)); pp(liu)=abs(p0*exp(-i*k*x)*exp(i*w*t)+bt*p0^2/2/rou/c^2*(1+2*i*k*x)*exp(-2*i*k*x)*exp(2*i*w*t)) ; Rapp(liu)=abs(pp2/pp1); ppc1(liu)=abs(p0*besselh(0,2,k*x)*exp(i*w*t)); % k*(x-1.0) ppc2(liu)=abs(2*i*bt*k*x/rou/c^2*(p0*besselh(0,2,k*x)*exp(i*w*t))^2); ppc(liu)=abs(p0*besselh(0,2,k*x)*exp(i*w*t)+2*i*bt*k*x*p0^2/rou/c^2*(besselh(0,2,k*x))^2*exp( 2*i*w*t)); Rappc(liu)=abs(ppc2/ppc1); s=0; for n=2:1:100; s=s+(-1)^n*gamma(n-1)/(4*i*k)^(n-1)/x^n; end LL(liu)=s; ps1(liu)=abs(p0/x*exp(-i*k*x)*exp(i*w*t)); ps2(liu)=abs(i*bt*k*p0^2/rou/c^2*(log(x)/x+LL(liu))*exp(-2*i*k*x)*exp(2*i*w*t)); ps(liu)=abs(p0/x*exp(-i*k*x)*exp(i*w*t)+i*bt*k*p0^2/rou/c^2*(log(x)/x+LL(liu))*exp(-2*i*k*x)*exp (2*i*w*t)); Raps(liu)=abs(ps2/ps1); 98 end Code 3: clear; A=1.0; Rs=1.0; k=2.0; U=450; c=1500; e=U/c; w=k*c; t=0; n=7.15; %%%%%%%%%%%%%%%%%%%%%%%% the integrations for the cylindrical wave x=1.02; tt=0; gg=0; tt1=((n-1)*besselh(0,2,k*x)^2-2*besselh(1,2,k*x)^2)*bessely(0,2*k*x)*x; for x=1.03:0.01:20.01; tt2=((n-1)*besselh(0,2,k*x)^2-2*besselh(1,2,k*x)^2)*bessely(0,2*k*x)*x; ttt=(tt1+tt2)/2; tt=tt+ttt*0.01; tt1=tt2; end gg1=((n-1)*besselh(0,2,k*x)^2-2*besselh(1,2,k*x)^2)*besselj(0,2*k*x)*x; for x=1.03:0.01:20.01; gg2=((n-1)*besselh(0,2,k*x)^2-2*besselh(1,2,k*x)^2)*besselj(0,2*k*x)*x; ggg=(gg1+gg2)/2; gg=gg+ggg*0.01; gg1=gg2; end %%%%%%%%%%%%%%%%%%%%%%%% liu=0; for x=1.02:0.01:20.01; % the distance away from the original point liu=liu+1 gang(liu)=x; % plane wave 99 fai0(liu)=abs(A*cos(k*x)*exp(i*w*t)); fai1(liu)=e^2*abs(A*cos(2*k*x)*exp(2*i*w*t)-i*w*A^2/8/U^2*((n+1)*k*x*sin(2*k*x)+(n+1)/4*cos( 2*k*x)+n-3)*exp(2*i*w*t)); fai(liu)=fai0(liu)+fai1(liu); Ratiofai(liu)=fai1(liu)/fai0(liu); % cylindrical wave cai0(liu)=abs(A*besselh(0,2,k*x)*exp(i*w*t)); cai1(liu)=e^2*abs(A*besselh(0,2,2*k*x)*exp(2*i*w*t)+i*pi*A^2*w^3*e^2/2/U^4*(besselj(0,2*k*x) *tt-bessely(0,2*k*x)*gg)*exp(2*i*w*t)); cai(liu)=cai0(liu)+cai1(liu); Ratiocai(liu)=cai1(liu)/cai0(liu); % spherical wave pai0(liu)=abs(A*Rs/e/x*cos(k*x)*exp(i*w*t)); pai1(liu)=e^2*abs(A*Rs/e/x*cos(2*k*x)*exp(2*i*w*t)-i*w*A^2*Rs^2/8/U^2/e^2/x^2*(k*x*(n+1)*(c osint(4*k*x)+2*cosint(2*k*x)+log(e*x/Rs))*sin(2*k*x)-k*x*(n+1)*(sinint(4*k*x)+2*sinint(2*k*x))*c os(2*k*x)-8*cos(k*x)^2)*exp(2*i*w*t)); pai(liu)=pai0(liu)+pai1(liu); Ratiopai(liu)=pai1(liu)/pai0(liu); end 100 Appendix E The calculated results from Pillai et al. 1982: 101 [...]... Linear Acoustic Wave Scattering by Two Dimensional Scatterer with Irregular Shape in an Ideal Fluid 3.1 Governing equations of linear acoustic wave The propagation of linear sound waves in a fluid can be modeled by the equation of motion (conservation of momentum) and the continuity equation (conservation of mass) With some simplifications by taking the fluid as homogeneous, inviscid, and irrotational, acoustic. .. present work are presented There is a brief presentation on the background of linear /nonlinear acoustic wave propagation, in which attention is centered on using conformal mapping method for linear acoustic wave scattering by the inclusion with irregular across section and perturbation method for the nonlinear acoustic wave propagation In Chapter 2, we outline the mathematical background for the conformal... linear acoustic wave equation, the nonlinear counterpart can handle waves with large finite amplitudes, and allow accurate modeling of nonlinear constitutive models in the fluid Interesting phenomena unknown in linear acoustics can be observed, for example, waveform distortion, formation of shock waves, increased absorption, nonlinear interaction (as opposed to superposition) when two sound waves are...  y x Solid Incident Acoustic wave Infinite fluid  Figure 3.1: The model for scattering of acoustic wave by rigid inclusion with irregular across section Consequently, the corresponding governing equation (3.9) in  ,  plane takes on the following form: w   w   2  2  k   0  4 (3.10) Equation (3.10) is a general expression for the spatial linear acoustic wave in the  ,  plane... Mitri 2005) On the other hand, the theoretical aspect of acoustic study on inclusion with arbitrary cross sections in fluids are far fewer Our proposed method is an attempt to meet the need for various geometries and extend the classical conformal mapping within the framework of complex variable methods for the acoustic wave scattering problem in fluids Incorporation of the mapping technique into the... model, conformal mapping was applied to solve the in-plane elastic wave propagation through the infinite domain with irregular-shaped cavity and dynamic stress concentration (Liu et al 1982), the anti-plane shear wave propagation via mapping into the Cartesian coordinates (Han & Liu 1997; Liu & Han 1991) and the anti-plane shear wave propagation via mapping of the inner/outer domain into polar coordinates... 23 if we set   0 , the wave number k will be the same as the harmonic wave k   c0 In this paper, the outgoing scattered wave will be combined with Hankel function of the first kind and the time term e  i t 3.2 Conformal transformations of Helmholtz equation and corresponding physical vector For the model of acoustic wave scattering by three dimensional inclusion with arbitrary geometry embedded... acoustic beams, cavitation and sonoluminescence (Crocker 1998) As far as we are aware, there are various models to simulate the nonlinear characteristic of the acoustic wave propagating through the fluid For instance, the one-dimensional Burgers equation has been found to be an excellent approximation of the conservation equations for plane progressive waves of finite amplitude in a thermoviscous fluid. .. possibly one of the first few to calculate the linear acoustic wave scattering of noncircular cylinders with the use of conformal mapping within the context of the complex variables method in the fluid The results obtained are validated against some special cases available in the literature, and then the effect of different geometries of the solid inclusion with sharp corners is studied (It may also be remarked... Problem Definition, Motivation and Scope of Present Work A better understanding of the physics of linear /nonlinear acoustic wave interact with inclusion is important for a wide range of applications including underwater detection, biomedical and chemical processes On the aspect of linear acoustic wave, considerable work has been done on the scattering by objects having regular cross section For instance, ... Linear Acoustic Wave Scattering by Two Dimensional Scatterer with Irregular Shape in an Ideal Fluid 3.1 Governing equations of linear acoustic wave The propagation of linear sound waves in a fluid. .. conditions of acoustic wave scattering in fluids, e.g irregular elastic inclusion within fluid with viscosity, etc Our calculated results have shown that the angle and frequency of the incident waves... background of linear /nonlinear acoustic wave propagation, in which attention is centered on using conformal mapping method for linear acoustic wave scattering by the inclusion with irregular across

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