ASYMPTOTIC BEHAVIOR FOR A NONLINEAR VISCOELASTIC PROBLEM WITH A VELOCITY-DEPENDENT MATERIAL DENSITY NASSER-EDDINE TATAR Received 22 September 2004 and in revised form 10 May 2005 We consider a nonlinear viscoelastic problem and prove that the solutions are uniformly bounded and decay exponentially to zero as time goes to infinity. This is established under weaker conditions on the relaxation function than the usually used ones. In particular, we remove the assumptions on the derivative of the kernel. In fact, our kernels are not necessarily differentiable. 1. Introduction The problem we would like to investigate is the following: ρ ut utt − ∆u − ∆utt + t 0 g(t − s)∆u(s)ds − γ∆ut = 0 in Ω × (0, ∞), u = 0 on Γ × (0, ∞), (1.1) ut (x,0) = u1 (x) in Ω, u(x,0) = u0 (x), where Ω is a bounded domain in Rn , n ≥ 1, with a smooth boundary Γ. The real number ρ is assumed to satisfy 0 < ρ ≤ 2/(n − 2) if n ≥ 3 or ρ > 0 if n = 1,2. The function g(t) is positive and will be specified further below. This model appears in viscoelasticity. We are in the case where the material density depends on ut (see [5, 11]). In [1], Cavalcanti et al. studied this nonlinear problem (ρ > 0) and proved well posedness as well as a uniform decay result. It has been shown that solutions go to zero in an exponential manner provided that the kernel g(t) is also exponentially decaying to zero. Namely, the following assumptions were assumed: (H1) g : R+ → R+ is a bounded C 1 -function such that 1− ∞ 0 g(s)ds = l > 0, (1.2) (H2) there exist positive constants ξ1 , ξ2 such that −ξ1 g(t) ≤ g (t) ≤ −ξ2 g(t) for all t ≥ 0. Copyright © 2005 Hindawi Publishing Corporation International Journal of Mathematics and Mathematical Sciences 2005:10 (2005) 1497–1506 DOI: 10.1155/IJMMS.2005.1497 (1.3) 1498 Asymptotic behavior for a viscoelastic problem These two assumptions are in fact frequently used also in the linear case (ρ = 0) (see [3, 4, 5, 6, 7, 8] and also [10, 13]). In [9], the present author with Messaoudi have improved the result in [1] by showing that the same asymptotic behavior occurs also for the case γ = 0. This means that the convolution term produces a weak dissipation which is able to drive solutions to the equilibrium state in an exponential manner. We do not need the strong damping. In [6], the present author with Furati proved that for “sufficiently small” g and g , we also have exponential decay (in case ρ > 0). Namely, we need eαt g(t) and eαt g (t) to have “small” L1 -norms for some α > 0. The conditions in (H2) are not imposed. In particular, g is not necessarily always negative. Here in this work, we intend to improve further this latter result by removing the condition on g . To this end, we combine the multiplier technique with some appropriate estimations and some new “Lyapunov-type” functionals. These functionals are somewhat similar in spirit to the one introduced by the author in [12]. The plan of the paper is as follows. In the next section, we state an existence theorem, introduce our functionals, and prove some useful propositions for our result. Section 3 is devoted to the exponential decay theorem. 2. Preliminaries We start by stating an existence result due to Cavalcanti et al. [1] (see also [2]). ∞ Theorem 2.1. Assume that the kernel g : R+ → R+ satisfies 1 − 0 g(s)ds = l > 0. Let u0 ,u1 ∈ H01 (Ω) and γ ≥ 0. Then, problem (1.1) possesses at least one weak solution u : Ω × (0, ∞) → R in the class u ∈ L∞ 0, ∞;H01 (Ω) , u ∈ L∞ 0, ∞;H01 (Ω) , u ∈ L2 0, ∞;H01 (Ω) . (2.1) We point out here that the differentiability of g is not needed to prove local existence. In this paper, we consider γ = 0. We may assume that γ = 1. The (classical) energy associated to problem (1.1) is defined by E(t) := 1 ρ+2 Ω ρ+2 ut dx + 1 2 Ω |∇u|2 dx + 1 2 Ω ∇ut 2 dx. (2.2) If we differentiate E(t) with respect to t along solutions of (1.1), we get E (t) = Ω ∇u t t 0 g(t − s)∇u(s)dsdx − Ω ∇ut 2 dx. (2.3) This expression is of an undefined sign, and therefore the boundedness (and the dissipativity) of the energy functional E(t) is not clear. In the prior works, the authors defined (g ∇u)(t) := t Ω 0 2 g(t − s)∇u(t) − ∇u(s) dsdx (2.4) Nasser-Eddine Tatar 1499 and observed that Ω ∇u t t 1 1 g(t − s)∇u(s)dsdx = (g ∇u)(t) − (g ∇u) (t) 2 2 0 t 1 d ∇ut 2 dx − 1 g(t) ∇ut 2 dx. g(s)ds + 2 dt 2 0 Ω Ω (2.5) Then, considering the modified energy functional t ρ+2 1 ut dx + 1 1 − g ds ρ+2 Ω 2 0 2 1 1 ∇ut dx + (g ∇u)(t), + 2 Ω 2 Ᏹ(t) = Ω |∇u|2 dx (2.6) it appears that Ᏹ (t) = − Ω ∇ut 2 dx + 1 (g ∇u)(t) − 1 g(t) 2 2 Ω |∇u|2 dx. (2.7) At this point, they use the fact that g (t) ≤ 0 to obtain uniform boundedness. In our case, we do not have this assumption. To overcome this, a new functional has been proposed in [6]. An exponential decay result has been obtained under some “smallness” condition on g(t) and g (t). It is our objective here to remove the smallness condition on g (t). In fact, even the differentiability of g is not required. We will need the assumptions (G1) g : R + → R+ is a bounded continuous function such that 1− ∞ 0 g(s)ds = l > 0, (2.8) (G2) g(t)eαt ∈ L1 (0, ∞) for some α > 0. We will use repeatedly the following inequality. Lemma 2.2. For any a,b ∈ R and δ > 0, ab ≤ δa2 + 1 2 b. 4δ (2.9) We denote ḡ := +∞ 0 g(s)ds, ḡα := +∞ 0 eαs g(s)ds. (2.10) Next, we prove the uniform boundedness of the classical energy. Proposition 2.3. Assume that (G1) and (G2) hold. If g is such that ḡα ≤ α/2, then E(t) ≤ E(0) for all t ≥ 0. (2.11) 1500 Asymptotic behavior for a viscoelastic problem Proof. We have Ω ∇u t t t g(t − s)∇u(s)dsdx = 0 0 + t 0 1 d ∇ut ∇udx = 2 dt Ω g ds g(s)ds t 0 Ω t ∇u t 0 Ω ∇ut ∇udx 1 |∇u| dx − g(t) 2 Ω 2 g ds (2.12) g(t − s) ∇u(s) − ∇u(t) dsdx, Ω |∇u|2 dx. (2.13) From (2.12) and Lemma 2.2 with δ = 1/4, we find Ω ∇u t t 0 g(t − s)∇u(s)dsdx ≤ 1 4 ∇ut 2 dx − 1 g(t) |∇u|2 dx 2 Ω t 1 d g(s)ds |∇u|2 dx . + ḡ(g ∇u)(t) + 2 dt Ω 0 (2.14) Ω Considering e(t) := 1 ρ+2 Ω t ρ+2 1 ut dx + 1 1 − g ds ∇ut 2 dx, |∇u|2 dx + 2 2 Ω 0 Ω (2.15) a simple computation shows, with the help of (2.14), that e (t) ≤ − 3 4 Ω |∇u|2 dx + ḡ(g ∇u)(t). (2.16) Next, we introduce the functional Φ(t) := t Ω 0 2 Gα (t − s)∇u(t) − ∇u(s) dsdx =: Gα ∇u (t) (2.17) with Gα (t) := e−αt +∞ t eαs g(s)ds (2.18) for some α > 0. A differentiation of (2.17) yields Φ (t) = −αΦ(t) − (g ∇u)(t) + 2 Ω ∇u t t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx. (2.19) By Lemma 2.2 with δ = 1/8λ, for some λ > 0 to be determined, we have Ω ∇u t t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx 1 ≤ 8λ Ω ∇ut 2 dx + 2λ t 0 Gα (s)ds Gα ∇u (t). (2.20) Nasser-Eddine Tatar 1501 Notice that t Gα (s)ds ≤ 0 1 α ∞ eαs g(s)ds = 0 ḡα . α (2.21) Therefore, 1 4λ Φ (t) ≤ −αΦ(t) − (g ∇u)(t) + ≤ − α− Ω ∇ut 2 dx + 4λḡα Φ(t) 4λḡα 1 Φ(t) − (g ∇u)(t) + α 4λ α Ω ∇ut 2 dx. (2.22) We define V (t) := e(t) + λΦ(t). (2.23) Clearly, by (2.16) and (2.22), we have V (t) ≤ − 1 2 Ω ∇ut 2 dx + (ḡ − λ)(g ∇u)(t) − λ α − 4λḡα Φ(t). α (2.24) If ḡα ≤ α/2, then it is possible to choose λ so that λ ≥ ḡα (notice that ḡα > ḡ) and λ ≤ α2 /4ḡα . Hence, V (t) ≤ 0. Consequently, e(t) and thereafter E(t) are uniformly bounded for all t ≥ 0 by e(0). This proposition will be used in a crucial manner in our main result. However, the functional V (t) is still not suitable to work with. We introduce Ψ(t) : = 1 ρ+1 χ(t) : = Ω Ω ρ ut ut udx + ∆ut − ρ t u t u t ρ+1 0 Ω ∇u∇ut dx, (2.25) Gα (t − s) u(t) − u(s) dsdx. Then, we form the expression W(t) := V (t) + ε Ψ(t) + χ(t) , t ≥ 0, (2.26) for some ε > 0 to be determined later. The next proposition will show, in particular, that the result we will derive for W(t) will also hold for the classical energy. Proposition 2.4. There exist an ε0 , m, and M > 0 such that mE(t) ≤ W(t) ≤ M E(t) + Φ(t) , for all λ ≥ ḡα and 0 < ε ≤ ε0 . t ≥ 0, (2.27) 1502 Asymptotic behavior for a viscoelastic problem Proof. We begin by the left inequality. Observe first that by the embedding H01 (Ω) L2(ρ+1) (Ω) for 0 < ρ ≤ 2/(n − 2) if n ≥ 3 or ρ > 0 if n = 1,2, we can write Ω 2(ρ+1) u t dx ≤ Ce Ω ∇ut 2 dx ρ+1 , (2.28) where Ce > 0 is the embedding constant (the subscript “e” is for embedding). Further, in virtue of Proposition 2.3, we get Ω 2(ρ+1) ρ u t dx ≤ Ce 2e(0) Ω ∇ut 2 dx = C Ω ∇ut 2 dx, (2.29) where C = Ce (2e(0))ρ . This relation, together with Lemma 2.2, implies that Ω ρ ut ut udx ≤ δ2 2(ρ+1) Cp u t dx + |∇u|2 dx 4δ2 Ω C 2 ∇ut 2 dx + p ≤ Cδ |∇u|2 dx, 4δ2 Ω Ω Ω (2.30) δ2 > 0, where C p is the Poincaré constant (the subscript “p” is for Poincaré), and Ω ρ u t u t t ≤ δ3 C 0 Gα (t − s) u(t) − u(s) dsdx Ω ∇ut 2 dx + C p ḡα Gα ∇u (t), 4δ3 α Gathering (2.30), (2.31), (2.20) with δ1 and Ω ∇u∇ut dx ≤ δ4 Ω ∇ut 2 dx + 1 4δ4 (2.31) δ3 > 0. Ω |∇u|2 dx, δ4 > 0, (2.32) we obtain from (2.25) and (2.26) that 1 W(t) ≥ ρ+2 Ω ρ+2 ut dx + 1 l − ε 2 Cp 1 + 2 δ2 (ρ + 1) δ4 Ω |∇u|2 dx δ2 + δ3 C 1 ∇ut 2 dx − ε δ 1 + δ4 + 2 ρ+1 Ω Cp εḡα 1 + λ− + Φ(t). 4α δ1 δ3 (ρ + 1) (2.33) + δ4 = 3/4l, and ε suffiTaking for instance δ1 = 1/5, δ2 = 3C p /4(ρ + 1)l, δ3 = (ρ + 1)/5C, ciently small, 2 l (ρ + 1)2 l 2α(ρ + 1)2 ε ≤ ε0 := min , , , 5 3 3C p C (ρ + 1)2 + C p C (2.34) we find that W(t) ≥ mE(t), for all t ≥ 0, for some positive constant m. The right-hand side inequality may be proved easily by taking for instance all the δi , i = 1,2,3,4, equal to 1/2 and summing up the inequalities in (2.30), (2.31), (2.34), and (2.20) with their respective coefficients in the expression of W(t). Nasser-Eddine Tatar 1503 3. Long-time behavior In this section, we state and prove our main result. Observe that assuming the hypotheses in Proposition 2.3, we have uniqueness of the weak solution. The solution corresponding to E(0) = 0 is the trivial one and is included in our next result. Theorem 3.1. Assume that the kernel g satisfies (G1) and (G2). Then, the √ weak solution of (1.1) decays exponentially to zero, in the energy norm, provided that ḡα ≤ α 2/4. Proof. We differentiate W(t) (see (2.26)) along solutions of (1.1), we obtain from (2.26) and (2.24) that W (t) ≤ − 1 2 ∇ut 2 dx + (ḡ − λ)(g ∇u)(t) − λ α − 4λḡα Φ(t) + εΨ (t) + εχ (t), α Ω (3.1) with Ψ (t) = − + χ (t) = Ω ∇u t 0 + + Ω Ω 0 ∇u t α ρ+1 1 + ρ+1 − 1 ρ+1 Ω ∇ut 2 dx + Ω ∇u t t ∇u 1 ρ+1 0 g(t − s)∇u(s)dsdx − Ω Ω ρ+2 ut dx, ∇u∇ut dx (3.2) 0 t 0 Ω Ω t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx g(t − s) ∇u(t) − ∇u(s) dsdx − ρ u t u t ρ u t u t t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx g(t − s)∇u(s)ds Ω |∇u| dx + t Ω t Gα (t − s) ∇u(t) − ∇u(s) dsdx + (1 + α) − 2 t 0 t 0 0 Gα (s)ds Ω ∇ut 2 dx (3.3) Gα (t − s) u(t) − u(s) dsdx g(t − s) u(t) − u(s) dsdx Gα (s)ds t Ω ρ+2 ut dx. We estimate some terms in the expressions of Ψ (t) and χ (t) separately. We denote by t G0 the value G0 := 00 Gα (s)ds for some t0 > 0 (selected so that E(t0 ) > 0, and thereafter by Proposition 2.4, W(t0 ) > 0). Applying Lemma 2.2 with δ = l/4, δ = l/4(1 + ḡ), δ = G0 /4(1 + α), and δ = G0 /4, we obtain Ω ∇u t 0 ≤ ḡ g(t − s)∇u(s)dsdx Ω |∇u|2 dx + Ω ∇u t 0 g(t − s) ∇u(s) − ∇u(t) dsdx 1504 Asymptotic behavior for a viscoelastic problem ≤ Ω ∇u t 0 l + ḡ 4 Ω Ω ∇u t t 0 Ω ∇u t t 0 |∇u|2 dx + Ω 1 + ḡ ḡα Gα ∇u (t), lα Ω ∇ut 2 dx + (1 + α)ḡα Gα ∇u (t), αG0 g(t − s) ∇u(t) − ∇u(s) dsdx G0 4 ≤ Gα (t − s) ∇u(t) − ∇u(s) dsdx G0 4(1 + α) ≤ Gα (t − s) ∇u(t) − ∇u(s) dsdx l ≤ 4(1 + ḡ) ḡ l |∇u|2 dx + (g ∇u)(t), Ω ∇ut 2 dx + ḡ (g ∇u)(t), G0 (3.4) respectively. We also have t Ω 0 t g(t − s)∇u(s)ds 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx t 2 1 g(t − s) ∇u(s) − ∇u(t) ds dx ≤ 2 Ω 0 (3.5) t 2 1 Gα (t − s) ∇u(t) − ∇u(s) ds + dx 2 Ω t + 0 0 g(s)ds Ω ∇u t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx. Therefore, t Ω 0 ≤ t g(t − s)∇u(s)ds ḡ (g ∇u)(t) + ḡ 2 + 0 Ω Gα (t − s) ∇u(t) − ∇u(s) dsdx ∇u t 0 Gα (t − s) ∇u(t) − ∇u(s) dsdx (3.6) ḡα Gα ∇u (t). 2α By Lemma 2.2 again with δ = l/4, we find Ω ∇u∇ut dx ≤ l 4 Ω |∇u|2 dx + 1 l Ω ∇ut 2 dx. (3.7) Nasser-Eddine Tatar 1505 Finally, by virtue of the embedding stated at the beginning of the proof of Proposition 2.4 (see (2.29)), we can deduce that Ω ρ u t u t t 0 Gα (t − s) u(t) − u(s) dsdx p CC (ρ + 1)G0 ≤ ḡα Gα ∇u (t) + (ρ + 1)G0 4α Ω (3.8) ∇ut 2 dx. Here we have used Lemma 2.2 with δ = αC/(ρ + 1)G0 . With δ = C/(ρ + 1)G0 , we find that Ω ρ u t u t t 0 g(t − s) u(t) − u(s) dsdx p ḡ CC (ρ + 1)G0 ≤ (g ∇u)(t) + (ρ + 1)G0 4 Ω (3.9) ∇ut 2 dx. Taking into account all the above estimates (3.4), (3.6), (3.7), (3.8), (3.9), (3.2), and (3.3) in (3.1), we entail that for t ≥ t0 , 1 C + C p 1 W (t) ≤ − −ε 1+ + 2 l 2(ρ + 1) Ω 1 1 1 − λ − ḡ − εḡ + + + 2 − λ α− l G0 ∇ut 2 dx − εl 4 C p C (ρ + 1)2 G0 Ω |∇u|2 dx (g ∇u)(t) − εG0 ρ+1 p 4λḡα εḡα (1 + ḡ)2 (1 + α)2 1 α2 CC + + + − α α l G0 2 G0 We must point out here that, to avoid a contradiction, the term in appears in the derivative of Ψ(t) (see (3.2)) has been estimated by ε ρ+1 Ω ρ+2 ut dx ≤ Ω ρ+2 ut dx Gα ∇u (t). (3.10) ρ+2 dx Ω |ut | ε 1 ut 2(ρ+1) dx + C p ∇ut 2 dx ρ+1 2 Ω 2 Ω ε ∇ut 2 dx. ≤ C + Cp 2(ρ + 1) Ω which (3.11) From (3.10), it is clear that for sufficiently small ε and ḡα ≤ α2 /8λ, there exists C1 > 0 such that W (t) ≤ −C1 E(t) + Φ(t) . (3.12) The right-hand side inequality in Proposition 2.4 implies that W (t) ≤ − C1 W(t). M (3.13) From this, we infer that W(t) ≤ W t0 e−C1 (t−t0 )/M , t ≥ t0 . (3.14) 1506 Asymptotic behavior for a viscoelastic problem Then, the left-hand side inequality in Proposition 2.4 allows us to conclude that E(t) ≤ W t0 −C1 (t−t0 )/M , e m This completes the proof of the theorem. t ≥ t0 . (3.15) Acknowledgments The author would like to thank the anonymous referee for valuable comments. The author is also grateful for the financial support and the facilities provided by King Fahd University of Petroleum and Minerals. References [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] [11] [12] [13] M. M. Cavalcanti, V. N. Domingos Cavalcanti, and J. 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Math. 8 (2003), no. 1, 1–12. Q. Tiehu, Asymptotic behavior of a class of abstract semilinear integrodifferential equations and applications, J. Math. Anal. Appl. 233 (1999), no. 1, 130–147. Nasser-Eddine Tatar: Department of Mathematical Sciences, College of Sciences, King Fahd University of Petroleum and Minerals, Dhahran 31261, Saudi Arabia E-mail address: tatarn@kfupm.edu.sa