Rayleigh Surface Waves Problem in Thermoviscoelastic Medium With Voids
Rayleigh Surface Waves Problem in Thermoviscoelastic Medium With Voids
Rayleigh Surface Waves Problem in Thermoviscoelastic Medium With Voids
In this paper we study the propagation of the Rayleigh surface waves in an exponentially functionally
graded half-space filled by a thermoviscoelastic material with voids. We take into consideration the
dissipative character of the porous thermoviscoelastic models upon the propagation waves and study the
damped in time wave solutions. The eigensolutions of the dynamical system are explicitly obtained in
terms of the characteristic solutions.
Key Words: Rayleigh surface waves, Damped in time solutions, Porous thermoviscoelasticity
1
in B (0, ), the constitutive equations dissipation energy density, implies
tij = Cijrs ers + Bij + Dijk ,k ij + Sij , > 0, > 0, b2 < + 23 , > 0,
Hi = Aij ,j + Drsi ers + di ai + Hi , 1 2
g = Bij eij di ,i + m + g , > 0, > 0, T0 + < 4 k, (9)
2 T0
= ij eij + a + m + ai ,i , 1 2
k > 0, b + > + .
Qi = kij ,j + firs ers + bi + aij ,j , 4 3
(3)
3 Surface waves in an anisotropic
with Sij ,Hi , and g given by
thermoviscoelastic porous half-space
Sij = Cijrs ers + Bij + Dijk ,k + Mijk ,k , Throughout this section, we assume B to be the
Hi = Aij ,j + Grsi ers + di + Pij ,j , (4) half-space x2 0 filled by an anisotropic thermo-
g = Fij eij k ,k Rj ,j , viscoelastic porous material that is inhomogeneous
in the sense that the constitutive coefficients and the
and the geometrical relations density mass are exponentially varying with depth,
1
in the form
eij = 2 (ui,j + uj,i ) , (5)
0
Cijrs = Cijrs e x2 , ..., i = i0 e x2 , = %e x2 ,
in B [0, ). Here, ui are the components of the
0
displacement vector, is the void volume fraction, where Cijrs , ...%, and are real constants. If = 0,
is the variation of temperature from the uniform then we have a homogeneous material.
reference absolute temperature T0 > 0, tij are the In what follows, we consider a surface wave
components of stress tensor, Hi are the components that is propagating in the direction of x1 axis, in
of the equilibrated stress vector, g is the intrinsic the half-space x2 0. We assume that the half-
equilibrated force, Qi are the components of the space x2 0 is free of body forces, equilibrated
heat flux vector, is the equilibrated inertia, is body force, and heat supply, and on its surface
the entropy density per unit mass, is the mass x2 = 0 has zero traction, zero equilibrated traction,
density, fi are the components of the body force and zero heat flux. Moreover, we consider that the
vector, ` is the extrinsic equilibrated body force per body is free to exchange heat with the region x2 < 0.
unit mass, and S is the heat supply per unit mass. Thus, we have the following boundary conditions
In what follows, we assume that the internal
t2i (x1 , 0, x3 , t) = 0, H2 (x1 , 0, x3 , t) = 0,
energy density (10)
Q2 (x1 , 0, x3 , t) = 0, x1 , x3 R, t 0.
2W = Cijrs eij ers + Aij ,i ,j + 2 To these boundary conditions we have to adjoin the
(6)
+ Bij eij + Dijk eij ,k + di ,i , asymptotic conditions
lim (x, t) = 0, lim {tij , hi , g, qi }(x, t) = 0,
= Cijrs eij ers + 2 + Aij ,i ,j + T10 kij ,i ,j x2 x2
2
In view of the relations (12), we can write K=A e11 + pA e12 i de1 + p + i A e21 + pA e22
h i i de2 + i e1 + pe 2 i e %v 2 ,
i x1 vt+ p+ i
x2
tij = iTij (V, p, v)e h i , 0
L = P11 + pP120
+ i a01 + p + i 0
P21 + pP220
i x1 vt+ p+ i
x2
Hi = ihi (V, p, v)e h
+ i a02 + i R10 + pR20 + i m0 ,
i, h
i x1 vt+ p+ i
x2 (15) M = iv a011 + pa012 i b01 + p + i a021
g = iG(V, p, v)e ,i i
+ pa022 i b02 + iT0 a01 + pa02 i m0 ,
h
i x1 vt+ p+ i
x2
= i%N (V, p, v)e h i,
0
N = k11 0
+ pk12 + p + i k210 0
+ pk22 ivT 0 0
a ,
i x1 vt+ p+ i
x2
Qi = iqi (V, p, v)e , (20)
and
where
Qij = C
e1ij1 , Rij = C
e1ij2 , Sij = C
e2ij2 . (21)
Tij = C eijr1 + pC eijr2 Ur + D e ij1 + pD e ij2
Since we seek a non-trivial solution V =
i B eij + M 0 + pM 0 + i 0 , {U1 , U2 , U3 , , } of the homogeneous system of al-
ij1 ij2 ij
ei2 i dei gebraic equations (18), we must impose that
hi = G e r1i + pG e r2i Ur + A ei1 + pA
det H = 0,
+ P1i 0
+ pPi20
+ i a0i , (22)
h
G = (Fer1 + pFer2 )Ur + e1 + pe 2 i e where
i
+ R10 + pR20 + i m0 ,
H11 H12 H13 G1 T1
H21 H22 H23 G2 T2
%N = (r1 0 0
+ pr2 )Ur + a01 + pa02 i m0
H =
i a0 , H31 H32 H33 G3 T3
. (23)
I1 I2 I3 K L
0 0
qi = iv(fir1 + fir2 )Ur iv a0i1 + pa0i2 J1 J2 J3 M N
i b0i + (ki1
0 0
+ pki2 ), Further, we will denote by pn , n = 1, ..., 5, the eigen-
(16) values with Im(pn ) > 0, so that the asymptotic
C 0
emnpq = Cmnpq 0
ivCmnpq , dem = d0m ivd0 conditions (11) are satisfied. This assumption can
m,
0 0 0 0 always be fulfilled by means of appropriate con-
Bmn = Bmn ivBmn , Amn = Amn ivAmn ,
e e
e mnp = D0 ivD0 , 0 0
straints upon the constitutive coefficients and by
D mnp mnp em = dm ivm , taking some appropriate restrictions upon the wave
0
Femn = Bmn0
ivFmn , e = 0 iv 0 , speed and on the damping rate.
Gmnp = Dmnp ivG0
e 0
mnp .
(n) (n) (n)
Let V (n) = U1 , U2 , U3 , (n) , (n) be
(17) the eigensolution corresponding to the eigenvalue
According to the relations (12), (15), and (16), we pn , n = 1, ..., 5. Following [3], we seek solutions of
can write the evolution equations (1) and (2) in the the Rayleigh surface waves propagation problem, in
form the form
Hir Ur + Gi + Ti = 0,
5
Ir Ur + K + L = 0, (18) X
U(x1 , x2 , t) = n V (n) ei(x1 vt+pn x2 ) , (24)
Jr Ur + M + N = 0,
n=1
3
h
(5) iT0 b b)5 + b2 + w2
(14). It is not easy to see that the secular equa- U1 = b ) (b +
b(+2b
tion has such a solution for characterizing Rayleigh mbb
i
(5) (5) (5)
waves. However, for particular materials, the sec- 2 , U2 = p5 U1 , U3 = 0,
n h
ular equation can be solved by means of numerical = T
(5) 0
( )52 + w2 + b
b + 2b
2
b(+2b
b )
methods. i o
m2 (b + 2b ) 5 m2 w2 ,
4 Application for an isotropic h h
(5) = bT0 b (
b + 2b)52 + bw2 + (
b + 2b
)
thermoviscoelastic porous half-space
(+2b
b ) b i
2 + w2 bb2 5
b
In this section, we illustrate the above results for the b o
class of isotropic and homogeneous porous thermo- + w2 2 + w2 ,
viscoelastic media ( = 0). According to Eqs.(6,14), (31)
we can write the characteristic equation (23) in the with
form w = iv, (32)
(p2 + 1) v 2 ]2 (p, v) = 0,
[b (26) and
b = + w ,
b = + w , bb = b + wb ,
where
h in
b = + w , b = b + w , b = + w .
(p, v) =
b + 2b (p2 + 1) v 2 bk + iv
The implicit and explicit expression for the secular
h
(p2 + 1)2 + k 12 b v 2 iv bc + m equation was obtained in [8]. Also, some numerical
i h simulations were presented for a specific material.
mT0 (p2 + 1) iv c 12 b v 2
2
io n h Acknowledgment
+ m2T0 + 12 kbbb + iv b T0 (bb
io h This work was supported by a grant of the Roma-
+ b) (p2 + 1)2 + iv3 mT0 (bb + b) + bbbc nian National Authority for Scientific Research and
i
2 2 2 2 Innovation, CNCS-UEFISCDI, project number PN-
T0 ( v ) (p + 1).
b
(27) II-RU-TE-2014-4-0320.
We will denote by pi , i = 1, ..., 5, the solutions of the
Eq.(26) with Im(pi ) > 0. Like in [3], for p = p2 and References
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