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北京交通大学教师名录.pdf

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北京交通大学教师名录.pdf

ISET Journal of Earthquake Technology, Paper No. 467, Vol. 43, No. 1-2, March-June 2006, pp. 1-9 SCATTERING OF SEISMIC WAVES FROM A CIRCULAR CAVITY WITH A PARTIALLY DEBONDED LINER Gui-Lan Yu and Yue-Sheng Wang School of Civil Engineering and Architecture Beijing Jiaotong University Beijing 100044, China ABSTRACT The scattering of seismic waves by a circular cavity with a partially debonded liner is studied by using the wave function expansion method and singular integral equation technique. The debonding region is modeled as an arc-shaped interface crack. For simplicity, the interaction between the crack edges is neglected. By expanding the wave fields in both liner and matrix as Fourier-Bessel series, the mixed boundary conditions lead to a set of simultaneous dual series equations, which may be further converted to Hilbert singular integral equations. Dynamic stress intensity factors describing the strength of dynamic interface traction at the ends of the bonding region and the scattering cross section are calculated by solving the singular integral equations numerically. The results show a distinguishing feature, the low frequency resonance, of such a problem. KEYWORDS: Scattering, Seismic Wave, Interface Debonding, Liner INTRODUCTION Scattering of seismic waves from a cavity with a liner is an interesting problem in earthquake engineering and civil engineering and has received considerable attention. The problem is customarily treated on the assumption that the liner is perfectly bonded to the matrix. For instance, Mal et al. (1968) solved the scattering of single objects within an infinite medium or with free surface based on quasianalytical methods in the frequency domain. However, perfect bonding is not always true in practical cases. For example, partial debonding usually occurs on the interface and may result in catastrophic failure of structures. In the past several decades a large number of valuable results were obtained. The scattering of elastic waves from a partially debonded inclusion was analyzed by Coussy (1984, 1986), Yang and Norris (1992). In the work by Wang and Meguid (1999), the dynamic interaction between a matrix crack and an inclusion subjected to anti-plane incident wave was discussed. The boundary element method (BEM) has also been used to study the scattering of elastic waves by a partially debonded inclusion (Sato and Shindo, 2002). A comprehensive review of BEMs applied to wave propagation phenomena including cracked media is due to Manolis and Beskos (1988), while an extensive study about the interaction of elastic waves with cracks was presented by Zhang and Gross (1998). Wang and Wang (1994a) have analytically studied the scattering of an SH wave by a cavity with a partially debonded liner by using the wave function expansion method and singular integral equation technique. Here, in the present paper, scattering of a P or SV wave is examined by using a similar method. The scattering of a plane wave by a partially debonded rigid or elastic cylindrical inclusion has been analyzed by Wang and Wang (1994b, 1996). PROBLEM FORMULATION Consider the problem shown in Figure 1. An elastic circular liner, with inner radius r1 and outer radius r0 , is partially bonded to the matrix. λ , µ , ρ are, respectively, the Lame’s constant, shear modulus and mass density. The subscripts “0” and “1” in this paper correspond to the matrix and liner respectively. The polar coordinate (r-θ) system is used. The debonding region is modeled as an interface crack with non-contacting faces, and is denoted by (a, b). An incident plane wave (P or SV) propagates in the direction of θ 0 . The entire motion is harmonic in time with frequency ω , and the term eiωt will be omitted throughout the paper. For the present in-plane problem, we use the displacement potentials ϕ 2 Scattering of Seismic Waves from a Circular Cavity with a Partially Debonded Liner and ψ (Pao and Mow, 1973). For the incident P-wave, the potential is assumed to be ϕ0( i ) = Aeik r cos(θ −θ ) , and for the SV-wave incidence, ψ 0(i ) = Beik r cos(θ −θ ) , where A and B are the amplitudes; K L = ω / cL and KT = ω / cT are the longitudinal wave number and shear wave number L0 0 T0 with cL = (λ + 2 µ ) / ρ and cT = 0 µ/ρ . Fig. 1 Scattering of an in-plane wave from a partially bonded liner The analysis here will focus on the P-wave incidence. The total potentials in the matrix and liner can be decomposed as {ϕ ,ψ } = (1 − j ) {ϕ , 0} + {ϕ ,ψ } + {ϕ ,ψ } j (i ) j j (0) j (0) j (1) j (1) j (1) where the quantities with superscript “(0)” refer to the scattered fields for a perfectly bonded liner (Pao and Mow, 1973), and those with superscript “(1)” to the additional scattered fields due to debonding. Using the wave function expansion method, we obtain ∞ {ϕ ,ψ } = ∑ { A H ( K r ), B H ( K r )} e (1) 0 (1) 0 m =−∞ 0m (1) m L0 0m (1) m − imθ (2) T0 ∞ {ϕ ,ψ } = ∑ {[ A J ( K r ) + A Y ( K r )],[ B J ( K r ) + B Y ( K r )} e (1) 1 (1) 1 m =−∞ 1m m L1 1m m L1 1m m T1 1m m − imθ T1 (3) where J m , Ym , H m(1) are Bessel functions (Abramowitz and Stegun, 1965). The associated displacement { } and {σ ,τ } , are of the same forms as those for the case of cylindrical inclusion (Wang and Wang, 1994b, 1996). The quantities, {σ ,τ } , in the liner are and stress components in the matrix, u0(1) , v0(1) (1) r0 (1) rθ 0 (1) r1 (1) rθ 1 ∞  (1) − imθ ru1 = ∑  A1m K L1rJ m′ ( K L1r ) − iB1m mJ m ( KT 1r ) + A1m K L1rYm′ ( K L1r ) − iB1m mYm ( KT 1r )  e  m =−∞  ∞ rv (1) = −  B1m KT 1rJ m′ ( KT 1r ) + iA1m mJ m ( K L1r ) + B1m KT 1rYm′ ( KT 1r ) + iA1m mYm ( K L1r )  e − imθ ∑ 1  m =−∞ (4) ∞  2 (1)  A1mT11(1) ( K L1r ) + B1mT12(1) ( KT 1r ) + A1mT11(1) ( K L1r ) + B1mT12(1) ( KT 1r )  e − imθ = r σ µ ∑ 1  r1  m =−∞  ∞ (1) (1) (1) (1) r 2τ (1) = µ   − imθ 1 ∑  A1mT21 ( K L1r ) + B1mT22 ( K T 1r ) + A1mT21 ( K L1r ) + B1mT22 ( KT 1r )  e  rθ 1 m =−∞ (5) ISET Journal of Earthquake Technology, March-June 2006 3 with T (1) ( K r ) = (2m 2 − K 2 r 2 ) J ( K r ) − 2 K rJ ′ ( K r ) L0 T0 m L0 L0 m L0  11 T (1) ( K r ) = 2im[ J ( K r ) − K rJ ′ ( K r )] 12 T0 m T0 T0 m T0  T21(1) ( K L 0 r ) = 2im[ J m ( K L 0 r ) − K L 0 rJ m′ ( K L 0 r )]  (1) T22 ( KT 0 r ) = −(2m 2 − KT20 r 2 ) J m ( KT 0 r ) + 2 KT 0 rJ m′ ( KT 0 r ) (6) Here, Tij(1) is the same as Tij(1) , with J m replaced by Ym . That the total tractions vanish on the inner (1) surface of the liner, i.e. σ r(1) 1 ( r1 , θ ) = τ rθ 1 ( r1 , θ ) = 0, yields δ A1m = X 1 A1m + X 2 B1m  δ B1m = X 3 A1m + X 4 B1m where δ = T11(1) ( K L1r1 )T22(1) ( KT 1r1 ) − T21(1) ( K L1r1 )T12(1) ( KT 1r1 ) , Appendix. Substitution of (7) into (4) and (5) gives (7) X i (i = 1, 2,3, 4) can be found in the ∞  (1) − imθ  ru1 ( r , θ ) = ∑  A1m K L1rZ1m (r ) − iB1m mZ1m (r )  e  m =−∞  ∞ rv (1) ( r , θ ) = −  B1m KT 1rZ 2 m (r ) + iA1m mZ 2 m (r )  e − imθ ∑  1 m =−∞ (8) ∞  2 (1) (1) (1)   − imθ r σ ( r , θ ) µ = 0 ∑  A1m S11 ( r ) + B1m S12 ( r )  e  r1  m =−∞  ∞ (1) (1) r 2τ (1) (r , θ ) = µ   − imθ rθ 1 0 ∑  A1m S 21 ( r ) + B1m S 22 ( r )  e  m =−∞ (9) where Z im , Zim , Sij(1) (i, j = 1, 2) are as given in the Appendix. The mixed boundary conditions at the interface r = r0 can be written as u0(1) (r0 ,θ ) − u1(1) (r0 ,θ ) = ∆u (θ ), v0(1) (r0 , θ ) − v1(1) (r0 ,θ ) = ∆v(θ )  (1) (1) (1) (1) σ r 0 (r0 , θ ) = σ r1 (r0 ,θ ), τ rθ 0 (r0 ,θ ) = τ rθ 1 (r0 ,θ )  (1) (0) (i ) (0) σ r 0 (r0 , θ ) = −σ r1 (r0 ,θ ) = −[σ r 0 (r0 ,θ ) + σ r 0 (r0 , θ )]; θ ∈ (a, b) τ (1) (r ,θ ) = −τ (0) (r , θ ) = −[τ (i ) (r , θ ) + τ (0) (r ,θ )]; θ ∈ (a, b) rθ 1 0 rθ 0 0 rθ 0 0  rθ 0 0 (10) Here, ∆u and ∆v are crack opening displacements which are zero beyond the crack. SINGULAR INTEGRAL EQUATIONS We expand ∆u (θ ) and ∆v(θ ) in the form of Fourier series: ∞ ∞ m =−∞ m =−∞ ∆u (θ ) = ∑ ∆um e − imθ , ∆v(θ ) = ∑ ∆vm e− imθ (11) with 1 b ∆v (ς )eimς d ς (12) ∫ a 2π Then Ajm and B jm can be expressed in terms of ∆um and ∆vm by considering Equations (8) and the ∆um = 1 b ∆u (ς )eimς dς , ∫ a 2π ∆vm = first two of Equations (10). Substituting the results into (9) and taking into account the last two of Equations (10), we obtain 4 Scattering of Seismic Waves from a Circular Cavity with a Partially Debonded Liner  m =∞ (11) (12) − imθ = −σ r(0) 1 ( r0 , θ )  µ0 ∑ [ N m ∆um + N m ∆vm ]e  m =−∞ ; θ ∈ ( a, b)  m =∞ im θ − (21) (22) (0) µ = −τ rθ 1 (r0 ,θ ) [ N m ∆um + N m ∆vm ]e  0 m∑ =−∞ (13) where N m( ij ) is expressed as (1) (0) (2)  N m( j1) = r0−1 Dm−1 [T j(0) 1 ( K L 0 r0 )U 0 m + T j 2 ( K T 0 r0 )U 0 m ]  ( j 2) −1 −1 (0) (1) (0) (2)  N m = r0 Dm [T j1 ( K L 0 r0 )V0 m + T j 2 ( KT 0 r0 )V0 m ] with Dm = (14) T11(0) ( K L 0 r0 ) T21(0) ( K L 0 r0 ) T12(0) ( KT 0 r0 ) T22(0) ( KT 0 r0 ) − S11(1) (r0 ) − S 21(1) (r0 ) − S12(1) (r0 ) − S 22(1) (r0 ) K L 0 r0 H m(1)′ ( K L 0 r0 ) −imH m(1) ( KT 0 r0 ) − K L1 r0 Z1m (r0 ) imZ1m (r0 ) −imH m(1) ( K L 0 r0 ) − KT 0 r0 H m(1)′ ( KT 0 r0 ) imZ 2 m (r0 ) KT 1 r0 Z 2 m (r0 ) U (jmk ) = D3,k + 2 j , V jm( k ) = D4,k + 2 j ; and j = 0,1 k = 1, 2 (15) (16) Here, Di , j denotes the algebraic complement of the element of the ith row and jth column of Dm . Outside the debonding region, we have m =∞ ∑ ∆u e m =−∞ − imθ m = 0, m =∞ ∑ ∆v e θ = 0; θ ∉ (a, b) m =−∞ − im (17) m Equations (13) and (17) are indeed a set of dual series equations. Introducing the following crack dislocation density functions (Wang and Wang, 1994b, 1996), ϕ (θ ) = 1 ∂ 1 ∂ (∆u ), ψ (θ ) = ( ∆v ) r0 ∂θ r0 ∂θ (18) Equations (13) reduce to  i b ∞ (11) (12) im (ζ −θ ) dς = −σ r(0) 1 ( r0 , θ )  2π ∫a ∑ [ M m ϕ (ς ) + M m ψ (ς )]e  m =−∞ ; θ ∈ ( a, b)  ∞ (21) (22) (0) im (ζ −θ )  i b dς = −τ rθ 1 (r0 ,θ ) [ M m ϕ (ς ) + M m ψ (ς )]e  2π ∫a m∑ =−∞ with M 0( st ) = i µ0 r0 N 0( st ) [ς − (a + b) / 2] and M m( st ) = µ0 r0 N m( st ) / m ; s, t = 1, 2 . Considering (19) the asymptotic behavior of Bessel functions, J m , Ym , H m(1) , as m → ±∞ (Abramowitz and Stegun, 1965), we have M m(11) , M m(22) ~ β − α / m + O(m −2 ); m → ±∞ (20) where α and β are the two important parameters defined by Dundurs (1969) to characterize the bimaterial system. With the relations given in (20), we can transform Equations (19), as in Wang and Wang (1994b, 1996), into a set of singular integral equations of the second type: b  β b  ς −θ  ψ θ ϕ ς ς a ( ) ( ) cot d [ϕ (ς ) P11 +ψ (ς ) P12 ]dς = −σ r(0) − − + 1 ( r0 , θ )    ∫ ∫ a a 2π   2  ; θ ∈ (a, b) (21)  b b − β ς θ   (0) aψ (θ ) − ψ (ς ) cot   dς + ∫a [ϕ (ς ) P21 +ψ (ς ) P22 ]dς = −τ rθ 1 (r0 ,θ ) ∫ a  2π  2  with ISET Journal of Earthquake Technology, March-June 2006 5 Pst (ς , θ ) = ∞  i   st  α  st    M 0 + 2i ∑  M m − β sgn(m) +  sin m(ς − θ ) − iα [π sgn(ς − θ ) − (ς − θ ) ]  ; s = t m m =−∞    2π   (22)  ∞      st β    ς −θ   (−1)t i  −iα + 2 M m + (−1) s i  α −   cos m(ς − θ ) + 2iβ ln 2sin   ∑  ; s ≠ t   π 2 m 2       =−∞ m       It follows from Equations (17) that b ∫ {φ (ς ),ψ (ς )} dς = 0 (23) a Introducing substitutions (θ , ς ) = c(ξ ,η ) + d with c = (b − a ) / 2, d = (b + a ) / 2 and  f (η )  i −1 ϕ (cη + d )    = [ R]   , Pst (η , ξ ) = Pst (cη + d , cξ + d ) β  g (η )  ψ (cη + d )  (24) i −i   , Equations (21) can be rewritten as a set of standard Cauchy singular integral 1 1  with [ R ] =  equations:  −γ 0  1 0   f (ξ )  1 1 1 0   f (η )  dη  Q11 Q12   f (η )  σ (ξ )  + + = c d η         ; ξ < 1 (25)      γ   g (ξ )  π i −∫1  0 1   g (η )  η − ξ −∫1 Q21 Q22   g (η )  τ ( ξ )   Here, we have γ = α / β , and P  Q11 Q12  −1  11 = [ ] R Q  P  21 Q22   21 (0) P12  [ I ]  c(η − ξ ) 2  σ (ξ )  [ R]−1 σ r1 (cξ + d )  [ R] + cot − ,  =−   P22  2π i  2 c(η − ξ )  τ (ξ )  i β τ r(0) θ 1 (cξ + d )  (26) The fundamental solution matrix of Equations (25) is W f (ξ )  (1 − ξ )α (1 + ξ ) β  α   −1/ 2 − iλ  1  1+ γ  , ln  with   =  λ =  =    β α W ξ ( ) i 1/ 2 − + β λ 2 π  1− λ       g  (1 − ξ ) (1 + ξ )  (27) Then the solution of Equations (25) can be expressed as a series of Jacobi polynomials: 0   A j Pj(α , β ) (ξ )   f (ξ )  ∞ W f (ξ )   = ∑   Wg (ξ )   B j Pj( β ,α ) (ξ )   g (ξ )  j =1  0   (28) which, when substituted into (25), yields an infinite system of linear algebraic equations. Solving these equations by truncating the infinite series to j = N, where N is big enough to ensure the convergence, we can obtain the unknown coefficients A j and B j . For details, reference may be made to Wang and Wang (1996). NUMERICAL RESULTS AND DISCUSSIONS Debonding of the interface under stress waves depends on the interface traction near the ends of the crack, which may be described by the dynamic stress intensity factors (DSIFs). Here we follow the method in Wang and Wang (1994b, 1996) to calculate the DSIFs. We define the following equivalent stress components: {σ ,τ } = −iβ [ R] {σ ,τ } (e) r (e) T rθ −1 T −1 r rθ (29) They have following asymptotic behavior at the crack tips (e.g., at θ → b + , or equivalently at ξ → 1+ ): 6 Scattering of Seismic Waves from a Circular Cavity with a Partially Debonded Liner σ r( e ) (r0 , ξ )   K I(be ) (r0 c) −1/ 2 (ξ − 1)α (ξ + 1) β   (e)  ≈  (e)  ; ξ → +1 β α −1/ 2 r τ ξ ( , ) − + K r c ξ ξ ( ) ( 1) ( 1)  rθ 0   IIb 0  (30) where the equivalent DSIFs, K I(be ) and K II( eb) , can be computed by (Wang and Wang, 1994b, 1996) ∞ {K , K } i (1 − γ )r c ∑ { A P (e) Ib (e) IIb 2 0 j j =1 (α , β ) j } (1), B j Pj( β ,α ) (1) (31) The real DSIFs are given by { K , K } = i β [ R ]{ K , K } T Ib (e) Ib IIb (e) T IIb (32) The far-field solution is also of importance in practical cases. By using the asymptotic behavior of Bessel functions at r → ∞ (Abramowitz and Stegun, 1965), the scattered far-field displacements can be expressed as  (0) 8π i ( K L 0 r −π / 4) (0) (1) e [ Fr (θ , θ 0 ) + Fr(1) (θ ,θ 0 )] u0 (r ,θ ) + u0 (r ,θ ) ≈ iK L 0 K L0r  ; r →∞  8π i ( KT 0 r −π / 4) (0) v (0) (r , θ ) + v (1) (r ,θ ) ≈ iK e [ Fθ (θ ,θ 0 ) + Fθ(1) (θ ,θ 0 )] 0 T0  0 KT 0 r  (33) where F (0) is the scattered far-field pattern for a perfectly bonded liner (Pao and Mow, 1973); and F (1) is that due to debonding, which is given by ∞ {F (θ ,θ ), F (θ ,θ )} = (2π ) ∑ (−i) { A , B } e (1) r −1 (1) 0 θ 0 m =−∞ m m − imθ m (34) With the above results, we can calculate the total scattering cross-section (SCS). This is defined as σ (ω ) = P S / e0 where e0 is the time-average of the incident flux and P S is the total scattered energy flux given by (Pao and Mow, 1973) PS = ω * (1) (0) (1) * (0) (1)  + + + Im ∫ ( u0(0) + u0(1) ) (σ r(0) σ v v ) ( 0 0 0 ) (τ rθ 0 + τ rθ 0 )  ds r0 S  2 (35) with the asterisk representing conjugation. Choosing S to be a unit length cylindrical surface with infinitely large radius, we then have π 2 2 P S = 4πωµ0 KT20 ∫  Fr(0) + Fr(1) + Fθ(0) + Fθ(1)  dθ −π   (36) The DSIFs and SCS have been computed for different sizes of the debond and for different thicknesses of the liner. We take µ1 : µ0 = 20 :1 , ρ1 : ρ 0 = 5 :1, and Poisson’s ratio ν 1 = ν 0 = 0.333. The incident P-wave propagates along the x-axis (i.e., θ 0 = 0o ). The debond is supposed to be at the shadow side and symmetric about the x-axis, that is a + b = 0. In solving Equation (28) numerically, we should appropriately choose N not only to ensure an adequate level of accuracy, but also to avoid wastage of time in computations. To this end, we have computed the normalized DSIFs, SCS and displacement of point A (see Figure 1) at the inner surface of the liner with different values of N and listed the results in Table 1. It can be seen that N > 14 may give good accuracy. Therefore we choose N = 16 in the following calculations. The results are demonstrated in Figures 2 and 3 where α is the semi-angular width of the debond and τ = µ0 K L20 A. In Figures 2(a) and 3(a), the solid lines correspond to K I , and the dashed lines to K II . Figure 2 shows the influence of the debond size for r1 / r0 = 0.5. A “low-frequency resonance” phenomenon is observed in DSIFs, SCS, and displacement of point A at the inner surface of the liner. The resonance is more pronounced and appears at a low frequency for a large debond. This is understood by considering the fact that, with the value of r1 / r0 being given (i.e., the mass of the system being fixed), an increase in the debond size α leads to a decrease in the rigidity of the system and, thus, results in a lower ISET Journal of Earthquake Technology, March-June 2006 7 resonant frequency. This phenomenon has been discussed extensively by Wang and Wang (1994a, 1994b, 1996). Figure 3 shows the influence of the thickness of the liner for α = 150o. It is seen that the resonant frequency varies with the thickness of the liner. The resonance appears at a low frequency for a small ratio r1 / r0 . Figures 3(a) and 3(b) also show that the low-frequency resonance is more pronounced for a thicker liner. This implies that a thicker liner may fail more easily than a thinner one due to dynamic effects. The physical interpretation of this phenomenon is that, for a fixed value of the debond size α (i.e., for the fixed rigidity of the system), a decrease in the ratio r1 / r0 leads to an increase in the mass of the system and therefore results in a lower resonant frequency. However, the thickness of the liner has little influence on the resonant peak of the displacement as shown in Figure 3(c). Table 1: Normalized DSIFs, SCS and Displacement of Point A with Different Values of N for KT 0 r0 = 0.5, r1 r0 = 0.5, and α = 150o N 2 4 6 8 10 12 14 16 18 20 K I τ r0 0.9653 1.4074 3.1840 5.0948 4.1035 4.0827 3.9755 3.9313 3.9677 3.9720 K II τ r0 0.1572 1.6365 6.0761 3.4328 2.8332 2.8309 2.7651 2.8481 2.8647 2.8577 σ r0 1.9243 3.3562 8.6387 8.1502 7.7972 7.8077 7.8084 7.8172 7.8132 7.8095 u K L0 A 1.2368 1.6645 2.6572 2.4219 2.3238 2.3254 2.3274 2.3293 2.3288 2.3282 Fig. 2 DSIF, SCS and displacement of point A at the inner surface of the liner for different sizes of the debond with r1 r0 = 0.5 Fig. 3 DSIF, SCS and displacement of point A at the inner surface of the liner for different thicknesses of the liner with α = 150o 8 Scattering of Seismic Waves from a Circular Cavity with a Partially Debonded Liner These results can be verified by the fact that the present results for r1 / r0 → 0 are the same as those obtained by Wang and Wang (1996). Furthermore, the results of a perfectly bonded liner (Pao and Mow, 1973) may be recovered from the present analysis by taking the limit of α → 0. ACKNOWLEDGEMENTS This work was supported by the China National Science Foundation under Grant No. 10372001. The second author is also grateful to the support of the National Science Fund for Distinguished Young Scholars under Grant No. 10025211. APPENDIX X i (i = 1, 2,3, 4) in Equations (7) and Z im , Zim , Sij(1) (i, j = 1, 2) in Equations (8) and (9) are as follows: X 1 = T21(1) ( K L1r1 )T12(1) ( KT 1r1 ) − T11(1) ( K L1r1 )T22(1) ( KT 1r1 ) X 2 = T22(1) ( K L1r1 )T12(1) ( KT 1r1 ) − T12(1) ( K L1r1 )T22(1) ( KT 1r1 ) X 3 = T11(1) ( K L1r1 )T21(1) ( K L1r1 ) − T21(1) ( K L1r1 )T11(1) ( K L1r1 ) (A.1) (1) X 4 = T12(1) ( KT 1r1 )T21(1) ( K L1r1 ) − T2(1) 2 ( KT 1r1 )T11 ( K L1r1 ) Z1m (r ) = J m ( KT 1r ) + 1 K L1rYm′ ( K L1r )  − ( ) Y K r X X2  m T 1 4 im δ   (A.2) Z 2 m (r ) = J m ( K L1r ) + 1 KT 1rYm′ ( KT 1r )  + ( ) Y K r X X3  m L 1 1 im δ   (A.3) 1 imYm ( KT 1r )  Z1m (r ) = J m′ ( K L1r ) + Ym′ ( K L1r ) X 1 − X3  δ K L1r  (A.4) 1 imYm ( K L1r )  Z 2 m (r ) = J m′ ( KT 1r ) + Ym′ ( KT 1r ) X 4 + X2  δ K T 1r  (A.5) (1) Si(1) 1 ( r ) = Ti1 ( K L1r ) + (1) Si(1) 2 ( r ) = Ti 2 ( KT 1r ) + 1 Ti1(1) ( K L1r ) X 1 + Ti 2(1) ( KT 1r ) X 3  ; i = 1, 2 δ 1 Ti1(1) ( K L1r ) X 2 + Ti 2(1) ( KT 1r ) X 4  ; i = 1, 2 δ (A.6) (A.7) REFERENCES 1. 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