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1 J. Differential Equations 49 (010) Contents lists available at ScienceDirect Journal of Differential Equations Pattern formation (I): The Keller Segel model Yan Guo a, Hyung Ju Hwang b, a Division of Applied Mathematics, Brown University, Providence, RI 091, USA b Department of Mathematics, Pohang University of Science and Technology, Pohang , Republic of Korea article info abstract Article history: Received 19 September 005 Keywords: Keller Segel Chemotaxis Pattern formation Instability Nonlinear dynamics We investigate nonlinear dynamics near an unstable constant equilibrium in the classical Keller Segel model. Given any general perturbation of magnitude δ, we prove that its nonlinear evolution is dominated by the corresponding linear dynamics along a fixed finite number of fastest growing modes, over a time period of ln 1 δ. Our result can be interpreted as a rigorous mathematical characterization for early pattern formation in the Keller Segel model. 010 Elsevier Inc. All rights reserved. 1. Growing modes in the Keller Segel model The goal of this section is to review the well-known instability criterion for the classical Keller Segel model, which describes directed movement of microorganisms and cells stimulated by the chemical which they produce themselves. The Keller Segel system takes the form U t = ( μ U + χ U V ), V t = (D V ) + fu kv, (1.1) where U(x, t) is the cell density, V (x, t) the chemo-attractant, μ > 0 the amoeboid motility, χ > 0 the chemotactic sensitivity, D > 0 the diffusion rate of camp, f > 0 the rate of camp secretion per unit density of amoebae, k > 0 the rate of degradation of camp in environment. * Corresponding author. addresses: guoy@dam.brown.edu (Y. Guo), hjhwang@postech.ac.kr (H.J. Hwang) /$ see front matter 010 Elsevier Inc. All rights reserved. doi: /j.jde
2 150 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) We assume Neumann boundary conditions for U(x, t) and V (x, t), inad-dimensional box x = (0, π) d, d = 1,, 3, i.e., A uniform constant solution U = V = 0, at x i = 0,π, for 1 i d. (1.) x i x i U(x, t) Ū, V (x, t) V forms a homogeneous steady state provided In this article, we study the nonlinear evolution of a perturbation f Ū = k V. (1.3) u(x, t) = U(x, t) Ū, v(x, t) = V (x, t) V around [Ū, V ], which satisfies the equivalent Keller Segel system: u t = μ u χ Ū v χ (u v), (1.4) v t = D v + fu kv. (1.5) The corresponding linearized Keller Segel system then takes the form We use [, ] to denote a column vector, and let u t = μ u χ Ū v, (1.6) v t = D v + fu kv. (1.7) w(x, t) [ u(x, t), v(x, t) ]. Let q = (q 1,...,q d ) Ω = (N 0}) d and let e q (x) d cos(q i x i ). i=1 Then e q (x)} q Ω forms a basis of the space of functions in that satisfy Neumann boundary conditions (1.). We look for a normal mode to the linear Keller Segel system (1.6) and (1.7) of the following form: w(x, t) = r q exp(λ q t)e q (x), (1.8) where r q is a vector depending on q. Plugging (1.8) into (1.6) (1.7) yields ( ) μq χ Ūq λ q r q = f Dq r k q,
3 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) where q = d i=1 q. A nontrivial normal mode can be obtained by setting i ( ) λq + μq χ Ūq det f λ q + Dq = 0. + k This leads to the following dispersion formula for λ q : λ q + q (μ + D) + k } λ q + q μ ( Dq + k ) χ Ūf } = 0. (1.9) Thus we deduce the following well-known aggregation (i.e., linear instability) criterion by requiring there exists a q such that μ ( Dq + k ) χ Ūf< 0, (1.10) to ensure that (1.9) has at least one positive root λ q. This clearly implies that μk χ Ūf< 0, and an elementary computation of the discriminant yields q (μ + D) + k } 4q μ ( Dq + k ) χ Ūf } = q 4 (μ D) + k + q (μ + D)k + 4q μk + χ Ūf} > 0 for q. Therefore, there exist two distinct real roots for all q to the quadratic equation (1.9), which we denote λ (q)<λ + (q). We denote the corresponding (linearly independent) eigenvectors by r (q) and r + (q), such that Clearly, for q large, [ λ± (q) + Dq ] + k r ± (q) =, 1. (1.11) f μ ( Dq + k ) χ Ūf> 0. Hence there are only finitely many q such that λ + (q)>0. We therefore denote the largest eigenvalue by λ max > 0 and define Ω max q Ω such that λ + (q) = λ max }. It is easy to see that there is one q (possibly two) having λ + q (q ) = λ max when we regard λ + q function of q.wealsodenoteν > 0 to be the gap between the λ max and the rest. Given any initial perturbation w(x, 0), we can expand it as as a w(x, 0) = w q e q (x) = w q r (q) + w q Ω q Ω + q r +(q) } e q (x),
4 15 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) so that w q = w q r (q) + w + q r +(q). (1.1) Theuniquesolutionw(x, t) =[u(x, t), v(x, t)] to (1.6) (1.7) is given by w(x, t) = q Ω w q r (q) exp ( λ q t) + w + q r +(q) exp ( λ + q t)} e q (x) e Lt w(x, 0). (1.13) For any u(, t) [L ( )],wedenote u(, t) u(, t) L. Our main result of this section is Lemma 1. Assume the instability criterion (1.10) is valid. Suppose w(x, t) = [ u(x, t), v(x, t) ] e Lt w(x, 0) as in (1.13) is a solution to the linearized KS system (1.6) (1.7) with initial condition w(x, 0). Then there exists a constant C 1 1 depending on k, Ū, D, μ, f, χ,suchthat w(, t) C 1 exp(λ max t) w(, 0), for all t 0. Proof. We first consider the case for t 1. By analyzing (1.9), for q large, we have λ ± q lim q q = μ, D respectively. Notice that from the quadratic formula for (1.9), From solving (1.1) we deduce that for t 1 and q large, λ + q λ q μk + χ Ūf. q q w ± 1 q r± (q) w q det[r (q), r + (q)] Cq w q, w ± q r ± (q) exp ( λ ± q t) Cq w q exp ( minμ, D}q t ) C w q. Thus we deduce the lemma on the linear growth rate for t 1 by the formula (1.13). On the other hand, for finite time t 1, it suffices to derive the standard energy estimate in L. From the Neumann boundary conditions, we can take u (1.6) and add Av of (1.7) to get 1 d dt u + A v } + μ u + AD v χ Ū v u } + Ak v = Afuv.
5 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) The integrand of the second integral can be chosen non-negative μ u + AD v χ Ū v u μ u + (Ūχ) v 0, (1.14) μ if the constant A is A = (Ūχ) Dμ. (1.15) It thus follows that 1 d u + A v } Af u + v }, dt and the Gronwall inequality implies w(, t) C exp(ct) w(, 0), for some C > 0. This immediately implies our lemma when t 1.. Main result Let θ be a small fixed constant, and λ max be the dominant eigenvalue which is the maximal growth rate. We also denote the gap between the largest growth rate λ max and the rest by ν > 0. Then for δ>0 arbitrary small, we define the escape time T δ by θ = δ exp ( λ max T δ), (.1) or equivalently Our main theorem is T δ = 1 λ max ln θ δ. Theorem 1. Assume that the set of q = d i=1 q i satisfying instability criterion (1.10) is not empty for given parameters μ, D, k, χ, fandū.let w 0 (x) = q Ω w q r (q) + w + q r +(q) } e q (x) H such that w 0 =1. Then there exist constants δ 0 > 0,C> 0,andθ>0, depending on k, Ū, D, μ, f, χ, such that for all 0 <δ δ 0, if the initial perturbation of the steady state [Ū, V ] in (1.3) is w δ (x, 0) = δw 0, then its nonlinear evolution w δ (t, x) satisfies
6 154 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) wδ (t, x) δe λ maxt w + q r +(q)e q (x) q Ω max C e νt + δ w 0 + H δe λ } maxt δe λ maxt for 0 t T δ,andν > 0 is the gap between λ max and the rest of λ q in (1.9). We notice that for 0 t T δ, δe λ maxt θ, is sufficiently small. As long as w + q 0 0 for at least one q 0 Ω max, which is generic for perturbations, the corresponding fastest growing modes δeλ maxt w + q r +(q)e q δeλ maxt w + r+ q0 (q 0 ), q Ω max have the dominant leading order of δe λ maxt. Our theorem implies that the dynamics of a general perturbation is characterized by such linear dynamics over a long time period of εt δ t T δ,for any ε > 0. In particular, choose a fixed q 0 Ω max and let w 0 (x) = r +(q 0 ) r + (q 0 ) e q 0 (x) then if t = T δ, wδ (t, ) δe λ maxt δ r +(q 0 ) r + (q 0 ) e q 0 ( ) C δ ν/λ max + θ }, hence w δ (t, ) θ C δ ν/λ max + θ } θ/ > 0, which implies nonlinear instability as δ 0. The instability occurs before the possible blow-up time. In the early work of Keller and Segel [14] in 1970, they formulated the advection diffusion system (1.1) which consists of two parabolic equations and viewed the initiation of Slime mold aggregation as instability. Linearized system was used to analyze early stage of pattern formation and its instability around homogeneous steady states. This Keller Segel model has since received much attention and there have been many contributions on this subject such as aggregations, dynamics of blow-ups, travelling waves. See [1 3,9 11,8,13,15 19] for related results. Linear stability and instability of stationary solutions with more general nonlinearity was studied in [0] using bifurcation analysis. However, nonlinear evolution of the pattern formation has yet been fully understood for the Keller Segel model, to the authors knowledge. We rigorously prove that linear fastest growing modes determine unstable patterns for the full Keller Segel system (1.4) and (1.5), over a time period of the order ln 1 δ. Each initial perturbation certainly can behaves drastically differently from another, which gives rise to the richness of patterns. On the other hand, the dominating linear dynamics over a fixed finite-dimensional space of maximal growing modes ensures that there is a common characteristic pattern for a general class initial data. Therefore, we believe that our result indeed provide a mathematical description for the pattern formation in the Keller Segel model. Our paper stems from a program to study various nonlinear instabilities for non-dissipative systems arising in mathematical physics [5 7,1], where severe higher-order perturbations (unbounded in the L norms, for instance) occur. Indeed, for many such systems without dissipation, the passage from linear instability to nonlinear instability is very delicate. If there is a dominant eigenvalue, then
7 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) a bootstrap argument was developed by Strauss and the first author to prove nonlinear instability, for the perturbation initially along the dominant eigenfunction. The key is to try to control the nonlinear growth of higher-order energy norm for the perturbation by the linear growth rate, up to the time T δ. Very recently in [4], based upon a precise linear analysis, dynamics of general perturbation can be characterized by the linear dynamics of fastest growing modes for unstable Kirchhoff ellipses. This marks a beginning of a quantitative description of instability. Our research is inspired by the work [4]. In the presence of dissipation, continuum spectra are absent in bounded domain, which leads to finite number of dominant growing modes. Moreover, natural higher-order energy estimate now can be easily combined with the bootstrap idea to control the nonlinear term χ (u v) in the L space. Since our method is general, we believe that such kind of pattern formation should exist for a wide class of systems with dissipation. 3. Bootstrap lemma We state existence of local-in-time solutions for (1.4) (1.5). Lemma (Local existence). For s 1 (d = 1) and s (d =, 3), thereexistat> 0 and a constant C depending on k, Ū, V, D, μ, f, χ such that w(t) H s C w(0) H s. We now derive the following energy estimates for d-dimensional chemotaxis model with d = 1,, 3. Lemma 3. Suppose that [u(x, t), v(x, t)] is a solution to the full system (1.4) (1.5). Then 1 d dt = + = } u + (Ūχ) v dx Dμ } μ 4 u + (Ūχ) v dx + Ak μ C 0 w H 3 w + C u, where C 0 is the universal constant while C = Ū 6 χ 6 f 6 D 3 μ 5 k 3. α = v Proof. We first notice that the Keller Segel equation preserves the evenness of the solution w(x, t), i.e., if w(x, t) is a solution, then w( x i, t) is also a solution. We can regard the Neumann problem as a special case with evenness of the periodic problem by standard way of even extension w(x, t) with respect to one of the x i. For this reason we may assume periodicity at the boundary of the extended T 3 ( π, π) d. Since now there is no contributions from the boundaries, we can take second-order -derivative of (1.4) and add A of (1.5) to get 1 d u + A v } + μ u + AD v χ Ū } v u + Ak v dt T d = χ u v} u + Af u v I 1 + I,
8 156 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) where the constant A is given in (1.15). As in (1.14), the second integrand is bounded below by μ u + (Ūχ) μ v. The nonlinear term I 1 is bounded by I 1 = (u v) u dx u L v u + u L v u + u v L u. We apply the following the Sobolev imbedding to control u L g L ( ) C 0 g H ( ), (3.1) for d 3. Moreover, from the periodic boundary conditions, u = v = 0, we also use the Poincaré inequality g g L4 ( ) C 0 g if d 3, (3.) to further get } u L + v L C 0 u H + v H C0 = w, where C 0 is a universal constant. Hence I 1 C 0 w H 3 w as desired. Finally, I is simply bounded by I = Af u v Af k u + Ak v. By the interpolation between u and u, the first term above is bounded by Af k a u + 1 } 4a u for any a > 0. We can choose a such that Af k a = 1 μ. Collecting terms, we conclude the proof. 4 We are now ready to establish the bootstrap lemma, which controls the H growth of w(x, t) in term of its L growth.
9 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) Lemma 4. Suppose that w(x, t) is a solution to the full system (1.4) (1.5) such that for 0 t T, and w(, t) H 1 } μ min C 0 4, (Ūχ) μ w(, t) C1 e λ maxt w(, 0), (3.3) then we have for 0 t T, where C 3 = C (Ūχ) 1 max Dμ, w(t) H C 3 w(0) H + e λ maxt w(, 0) } Dμ (Ūχ) } max 4C λ max, 1} 1. Proof. It suffices to only consider the second-order derivatives of w(x, t). From the previous lemma and our assumption for w H,wededucethatfor0 t T 1 d dt = So that by (3.3) and an integration from 0 to t, wehave = = u(t) + (Ūχ) v(t) } Dμ } u + (Ūχ) v dx C u. Dμ u(0) (Ūχ) } + v(0) + 4C C 1 e λ maxt w(, 0), Dμ λ max for 0 t T. Now our lemma follows directly by separating the cases of (Ūχ) Dμ 4. Nonlinear instability and pattern formation We now prove our main Theorem 1: (Ūχ) 1 and Dμ < 1. Proof of Theorem 1. Let w δ (x, t) be the family of solutions to the Keller Segel system (1.4) (1.5) with initial data w δ (x, 0) = δw 0.DefineT by Note that T is well defined. We also define T = sup t } w δ (t) δe Lt w 0 C 1 δ exp(λ maxt). T = sup t w δ (t) H 1 }} μ min C 0 4, (Ūχ). μ
10 158 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) We recall T δ in (.1) where θ is chosen such that C 0 C 3 θ<min λmax 4, μ 8, (Ūχ) 4μ }. (4.1) We now derive estimates for H norm of w δ (x, t) for 0 t mint, T δ, T }. First of all, by the definition of T,fort T and Lemma 1 w δ (t) 3C 1 δ exp(λ maxt). Moreover, using Lemma 4 and applying a bootstrap argument yields w δ (t) H C 3 δ w0 H + δe λ maxt }. (4.) We now establish a sharper L estimate for w δ (x, t), for0 t mint, T δ, T }. We first apply Duhamel s principle to obtain t w δ (t) = δe Lt w 0 0 e L(t τ )[ (u δ (τ ) v δ (τ ) ), 0 ] dτ. Using Lemma 1, (3.1), (3.), and Lemma 4 yields, for 0 t mint δ, T, T } w δ (t) δe Lt w 0 C 1 C 1 t 0 t 0 + C 1 C 1 C 0 e λ max(t τ ) (u δ (τ ) v δ (τ ) ) dτ e λ max(t τ ) u δ (τ ) L v δ (τ ) dτ t 0 t 0 e λ max(t τ ) u δ (τ ) L 4 v δ (τ ) L 4 dτ e λ max(t τ ) w δ (τ ) H dτ. By our choice of t mint, T, T δ }, it is further bounded by w δ (t) δe Lt w 0 C 1 C 0 C 3 We now prove by contradiction that for δ sufficiently small, t 0 e λ max(t τ ) δ w 0 H + δ e λ maxτ } dτ w0 δ H C 1 C 0 C } δe λ maxt δe λmaxt. (4.3) λ max λ max
11 Y. Guo, H.J. Hwang / J. Differential Equations 49 (010) T δ = min T δ, T, T }, and therefore our theorem follows by further separating q Ω max and move q / Ω max in (1.13) to the right-hand side. If T is the smallest, we can let t = T T δ in (4.) w δ ( T ) H C 3 δ w0 H + δe λ maxt δ } = C 3 δ w0 H + θ } < 1 } μ min C 0 4, (Ūχ), μ for C 3 δ w 0 H 1 C 0 min μ 4, (Ūχ) μ }, by our choice of θ in (4.1) with C 3 1. This is a contradiction to the definition of T. On the other hand, if T is the smallest, we let t = T in (4.3) to get w δ ( T ) δe LT w0 δ w 0 H C 1 C 0 C } δe λ δ maxt δe λ maxt λ max λ max w0 δ H C 1 C 0 C 3 + θ } δe λ maxt λ max λ max < C 1 δeλ maxt, w 0 H for C 0 C δ 3 λ max < 1/4 forδ small, by our choice of θ in (4.1). This again contradicts the definition of T and our theorem follows. Acknowledgments Hyung Ju Hwang is supported by Basic Science Research Program through the National Research Foundation of Korea funded by the Ministry of Education, Science and Technology ( ). References [1] W. Alt, Biased random walk models for chemotaxis and related diffusion approximations, J. Math. Biol. 9 (1980) [] P. Biler, Global solutions to some parabolic elliptic systems of chemotaxis, Adv. Math. Sci. Appl. 9 (1999) [3] M.P. Brenner, P. Constantin, L.P. Kadanoff, A. Schenkel, S.C. Venkataramani, Attraction, diffusion and collapse, Nonlinearity 1 (1999) [4] Y. Guo, C. Hallstrom, D. Spirn, Dynamics near an unstable Kirchhoff ellipse, Comm. Math. Phys. 45 (004) [5] Y. Guo, W. Strauss, Instability of periodic BGK equilibria, Comm. Pure Appl. Math. 48 (3) (1995) [6] Y. Guo, Instability of symmetric vortices with large charge and coupling constant, Comm. Pure Appl. Math. 49 (8) (1996) [7] C. Bardos, Y. Guo, W. Strauss, Stable and unstable ideal plane flows. Dedicated to the memory of Jacques-Lious Lions, Chin. Ann. Math. Ser. B 3 () (00) [8] K. Hadeler, T. Hillen, F. Lutscher, The Langevin or Kramers approach to biological modeling, Math. Models Methods Appl. Sci. 14 (10) (004) [9] M.A. Herrero, J.J.L. Velázquez, A blow-up mechanism for a chemotaxis model, Ann. Sc. Norm. Super. Pisa Cl. Sci. (4) 4 (4) (1997) [10] T. Hillen, K.J. Painter, Global existence for a parabolic chemotaxis model with prevention of overcrowding, Adv. in Appl. Math. 6 (001) [11] D. Horstmann, A. Stevens, A constructive approach to travelling waves in chemotaxis, J. Nonlinear Sci. 14 (1) (004) 1 5. [1] H.-J. Hwang, Y. Guo, On the dynamical Rayleigh Taylor instability, Arch. Ration. Mech. Anal. 167 (3) (003) [13] W. Jäger, S. Luckhaus, On explosions of solutions to a system of partial differential equations modelling chemotaxis, Trans. Amer. Math. Soc. 39 () (199)
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