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Small scale formations in the incompressible porous media equation

Alexander Kiselev  and  Yao Yao
Abstract.

We construct examples of solutions to the incompressible porous media (IPM) equation that must exhibit infinite in time growth of derivatives provided they remain smooth. As an application, this allows us to obtain nonlinear instability for a class of stratified steady states of IPM.

Key words and phrases:
IPM equation, two-dimensional incompressible flow, small scale creation, derivatives growth, nonlinear instability
2010 Mathematics Subject Classification:
35Q35,76B03
Department of Mathematics, Duke University, 120 Science Dr., Durham NC 27708, USA; email: [email protected]
School of Mathematics, Georgia Institute of Technology, Atlanta, GA 30332, USA; email: [email protected]

1. Introduction

In this paper, we consider the 2D incompressible porous media (IPM) equation. The equation describes evolution of density carried by the flow of incompressible fluid that is determined via Darcy’s law in the field of gravity:

tρ+(u)ρ=0,u=0,u+p=(0,ρ).\partial_{t}\rho+(u\cdot\nabla)\rho=0,\,\,\,\nabla\cdot u=0,\,\,\,u+\nabla p=-(0,\rho). (1.1)

Here ρ\rho is the transported density, uu is the vector field describing the fluid motion, and pp is the pressure. Throughout this paper, we consider the spatial domain Ω\Omega to be one of the following: the whole space 2\mathbb{R}^{2}, the torus 𝕋2=[π,π)2\mathbb{T}^{2}=[-\pi,\pi)^{2}, or the bounded strip S:=𝕋×[π,π]S:=\mathbb{T}\times[-\pi,\pi] that is periodic in x1x_{1}. In the last case, due to the presence of boundaries, uu also satisfies un=0u\cdot n=0 for x2=±πx_{2}=\pm\pi. In all the three cases, one can obtain a more explicit Biot-Savart law for uu:

u=(ΔΩ)1x1ρ.u=\nabla^{\perp}(-\Delta_{\Omega})^{-1}\partial_{x_{1}}\rho.

Here =(x2,x1)\nabla^{\perp}=(-\partial_{x_{2}},\partial_{x_{1}}), and the inverse Laplacian (ΔΩ)1(-\Delta_{\Omega})^{-1} for Ω=𝕋2\Omega=\mathbb{T}^{2} and Ω=𝕋×[π,π]\Omega=\mathbb{T}\times[-\pi,\pi] will be specified in Section 2.

There have been many recent papers analyzing the well-posedness questions for the IPM equation and its variants [1, 4, 5, 8, 19], lack of uniqueness of weak solutions [3, 18], and questions of long time dynamics [7, 1]. Viewed as an active scalar, the IPM equation is less regular than the 2D Euler equation in vorticity form, and has the same level of regularity as the SQG equation. Local well-posedness for sufficiently regular initial data has been proved in [5] for 2\mathbb{R}^{2}, and [1] for the strip SS. The argument can be adapted to the periodic setting 𝕋2\mathbb{T}^{2}; we will sketch a simple proof in Section 2.2. The question of global regularity vs finite-time blow up is open for the IPM equation, similarly to the SQG equation case. Moreover, to the best of our knowledge, there are not even examples of smooth solutions to the IPM equation that have infinite growth of derivatives. There are plenty of such examples for the 2D Euler equation, going back to work of Yudovich [12, 20] (see e.g. [6], [13] for more recent examples and further references). However, for the more singular SQG equation case, such examples have been established only recently [10]. The reason for such delay is that an example of infinite in time creation of small scales requires sufficiently strong control of the solution, which is not easily achieved when the drift is more singular. The example of [10] is based on the insight gained in the constructions for the 2D Euler case [13, 21], and is based on a hyperbolic point scenario controlled by odd-odd symmetry of the active scalar. It is tempting to use a similar idea for the IPM equation, but its structure is different - in particular, odd symmetry in x2x_{2} but even symmetry of ρ\rho in x1x_{1} is conserved instead of the odd-odd symmetry for the SQG equation. This, and the more detailed structure of the Biot-Savart law, appear to be significant obstacles in extending ideas of [10, 13, 21] to the IPM equation setting. In this paper, we construct examples of infinite growth of derivatives in smooth solutions of the IPM equation using a different idea, exploiting existence of monotone quantity which corresponds to the potential energy of the fluid. All our estimates below assume that the solutions remain smooth; more specifically, the arguments work if ρ\rho and uu are at least Lipschitz. If this regularity fails in finite time, we already have an even more dramatic effect than what we are trying to establish.

1.1. Small scale formation in IPM

In this paper, we consider the following three scenarios:

(S1) Let Ω=2\Omega=\mathbb{R}^{2}. Assume ρ0Cc(2)\rho_{0}\in C_{c}^{\infty}(\mathbb{R}^{2}) is odd in x2x_{2}, and ρ00\rho_{0}\geq 0 in ×+\mathbb{R}\times\mathbb{R}^{+}.

(S2) Let Ω=𝕋2=[π,π)2\Omega=\mathbb{T}^{2}=[-\pi,\pi)^{2} be the 2D torus. Assume ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) is odd in x2x_{2}.

(S3) Let Ω=S:=𝕋×[π,π]\Omega=S:=\mathbb{T}\times[-\pi,\pi] be a bounded strip that is periodic in x1x_{1}. Assume ρ0C(S)\rho_{0}\in C^{\infty}(S).

Our first result shows that in the scenario (S1), ρ(t)\rho(t) must have infinite-in-time growth in H˙s\dot{H}^{s} norm for any s>0s>0, if it remains regular for all times. Note that s>0s>0 is the sharp threshold, since for s=0s=0 we know ρ(t)L2=ρ0L2\|\rho(t)\|_{L^{2}}=\|\rho_{0}\|_{L^{2}} does not grow in time.

Theorem 1.1.

For Ω=2\Omega=\mathbb{R}^{2}, let ρ00\rho_{0}\not\equiv 0 satisfy the scenario (S1). Assuming that there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}, we have

0ρ(t)H˙s(2)4s𝑑tC(s,ρ0) for all s>0,\int_{0}^{\infty}\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}^{-\frac{4}{s}}dt\leq C(s,\rho_{0})\quad\text{ for all }s>0, (1.2)

which implies

lim suptts4ρ(t)H˙s(2)= for all s>0.\limsup_{t\to\infty}t^{-\frac{s}{4}}\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}=\infty\quad\text{ for all }s>0. (1.3)

The next result concerns the torus scenario (S2), where we prove infinite-in-time growth under some additional symmetry and positivity assumptions on ρ0\rho_{0}. As we will see in the remark afterwards, the same result also holds for the bounded strip scenario (S3).

Theorem 1.2.

For Ω=𝕋2\Omega=\mathbb{T}^{2}, let ρ00\rho_{0}\not\equiv 0 satisfy the scenario (S2). In addition, assume that ρ0\rho_{0} is even in x1x_{1}, ρ0=0\rho_{0}=0 for x1=0x_{1}=0, and ρ00\rho_{0}\geq 0 in D:=[0,π]2D:=[0,\pi]^{2}. Assuming that there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}, we have

0x1ρ(t)H˙s(𝕋2)22s+1𝑑tC(s,ρ0) for all s>12,\int_{0}^{\infty}\|\partial_{x_{1}}\rho(t)\|_{\dot{H}^{s}(\mathbb{T}^{2})}^{-\frac{2}{2s+1}}dt\leq C(s,\rho_{0})\quad\text{ for all }s>-\frac{1}{2}, (1.4)

which implies

lim suptt(s+12)ρ(t)H˙s+1(𝕋2)lim suptt(s+12)x1ρ(t)H˙s(𝕋2)= for all s>12.\limsup_{t\to\infty}t^{-(s+\frac{1}{2})}\|\rho(t)\|_{\dot{H}^{s+1}(\mathbb{T}^{2})}\geq\limsup_{t\to\infty}t^{-(s+\frac{1}{2})}\|\partial_{x_{1}}\rho(t)\|_{\dot{H}^{s}(\mathbb{T}^{2})}=\infty\quad\text{ for all }s>-\frac{1}{2}. (1.5)
Remark 1.3.

Observe that the solution ρ(,t)\rho(\cdot,t) in 𝕋2\mathbb{T}^{2} from Theorem 1.2 is automatically a solution in the bounded strip 𝕋×[π,π]\mathbb{T}\times[-\pi,\pi], with uu satisfying the no-flow condition on the top and bottom boundaries. (This is because ρ(,t)\rho(\cdot,t) is odd in x2x_{2} and has period 2π2\pi in x2x_{2} for all times. Thus ρ(,t)\rho(\cdot,t) is also odd about x2=±πx_{2}=\pm\pi, implying u(,t)e2=0u(\cdot,t)\cdot e_{2}=0 for all times on x2=±πx_{2}=\pm\pi.) Therefore, the growth results of Theorem 1.2 directly hold in scenario (S3). We note that the local well-posedness for the scenario (S3) has been established in [1], which in particular ensures the uniqueness of solution while it remains regular.

1.2. Nonlinear instability in IPM

One can easily check that any horizontal stratified state ρs=g(x2)\rho_{s}=g(x_{2}) is a stationary solution of (1.1) in 2\mathbb{R}^{2}, 𝕋2\mathbb{T}^{2} or SS, since u=(ΔΩ)1x1ρ0u=\nabla^{\perp}(-\Delta_{\Omega})^{-1}\partial_{x_{1}}\rho\equiv 0. (As we will see in Lemma 3.1, all smooth stationary solutions in SS are of the form ρs=g(x2)\rho_{s}=g(x_{2}). However, in 2\mathbb{R}^{2} and 𝕋2\mathbb{T}^{2} there are other smooth stationary solutions, e.g. any vertical stratified state is also stationary; see also [2, Section 5] for smooth stationary solutions in 2\mathbb{R}^{2} supported in an infinite slanted strip.)

Below we briefly summarize the previous stability results for the horizontal stratified state ρs=g(x2)\rho_{s}=g(x_{2}). Denoting η(x,t):=ρ(x,t)ρs(x)\eta(x,t):=\rho(x,t)-\rho_{s}(x) and plugging it into (1.1), η\eta satisfies

tη+uη=g(x2)u2,\partial_{t}\eta+u\cdot\nabla\eta=-g^{\prime}(x_{2})u_{2}, (1.6)

with u=(ΔΩ)1x1ηu=\nabla^{\perp}(-\Delta_{\Omega})^{-1}\partial_{x_{1}}\eta. For η\eta small, the linearized equation is tη=g(x2)u2\partial_{t}\eta=-g^{\prime}(x_{2})u_{2}, which can be written as

tη=g(x2)(ΔΩ)1x12η.\partial_{t}\eta=-g^{\prime}(x_{2})(-\Delta_{\Omega})^{-1}\partial^{2}_{x_{1}}\eta.

Since (ΔΩ)1x12(-\Delta_{\Omega})^{-1}\partial^{2}_{x_{1}} is a negative operator, one would expect the equation to be linearly stable if gg^{\prime} is uniformly negative (i.e. lighter density on top, heavier on the bottom).

For the stratified state ρs=x2\rho_{s}=-x_{2}, the asymptotic stability of the nonlinear equation (1.6) has been rigorously established by Elgindi [7] in 2\mathbb{R}^{2} and Castro–Córdoba–Lear [1] in SS, which also implies the global well-posedness of (1.1) for initial data close to ρs=x2\rho_{s}=-x_{2} in certain Sobolev spaces. More precisely, for ρs=x2\rho_{s}=-x_{2} in 2\mathbb{R}^{2}, if ηW4,1(2)+ηHs(2)<ϵ1\|\eta\|_{W^{4,1}(\mathbb{R}^{2})}+\|\eta\|_{H^{s}(\mathbb{R}^{2})}<\epsilon\ll 1 for s20s\geq 20, [7, Theorem 1.3] proved that η\eta remains regular for all time and satisfies η(t)H3ϵt1/4\|\eta(t)\|_{H^{3}}\lesssim\epsilon t^{-1/4} for all t>0t>0. [7] also obtained asymptotic stability results for periodic perturbation ηHs(𝕋2)\eta\in H^{s}(\mathbb{T}^{2}), where ρs\rho_{s} is still x2-x_{2} in the whole plane. In [1], the authors proved that for the stratified state ρs=x2\rho_{s}=-x_{2} in SS is asymptotically stable in Hs(S)H^{s}(S) for s10s\geq 10, although it may converge to a slightly different stratified state from ρs\rho_{s} as tt\to\infty.

In this paper, we aim to prove two nonlinear instability results for the horizontal stratified steady state ρs=g(x2)\rho_{s}=g(x_{2}) in 𝕋2\mathbb{T}^{2} and SS respectively. What sets our approach apart is that we are not following the common path of converting linear instability into a nonlinear one. Rather, we use the monotone quantity - potential energy - to prove infinite-in-time growth of Sobolev norms and then leverage these results to conclude the nonlinear instability. Our first instability result shows that in 𝕋2\mathbb{T}^{2}, any horizontal stratified steady state ρs\rho_{s} that is odd in x2x_{2} is nonlinearly unstable, and the instability can grow “infinitely in time”. Namely, for any arbitrarily large k>0k>0, one can construct an initial data ρ0\rho_{0} that is arbitrarily close to ρs\rho_{s} in HkH^{k}, such that lim suptρ(t)ρsH˙s(𝕋2)=\limsup_{t\to\infty}\|\rho(t)-\rho_{s}\|_{\dot{H}^{s}(\mathbb{T}^{2})}=\infty for all s>1s>1.

Theorem 1.4.

Let ρsC(𝕋2)\rho_{s}\in C^{\infty}(\mathbb{T}^{2}) be any horizontal stratified state (i.e. ρs(x)=g(x2)\rho_{s}(x)=g(x_{2})) that is odd in x2x_{2}. For any ϵ>0\epsilon>0 and any k>0k>0, there exists an initial data ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) satisfying

ρ0ρsHk(𝕋2)ϵ,\|\rho_{0}-\rho_{s}\|_{H^{k}(\mathbb{T}^{2})}\leq\epsilon,

such that the solution ρ(,t)\rho(\cdot,t) to (1.1) with initial data ρ0\rho_{0} (provided it remains smooth for all times) satisfies

lim suptts2ρ(t)ρsH˙s+1(𝕋2)= for all s>0.\limsup_{t\to\infty}t^{-\frac{s}{2}}\|\rho(t)-\rho_{s}\|_{\dot{H}^{s+1}(\mathbb{T}^{2})}=\infty\quad\text{ for all }s>0. (1.7)

Finally, we prove an instability result in the bounded strip S=𝕋×[π,π]S=\mathbb{T}\times[-\pi,\pi] for any stratified steady state ρsC(S)\rho_{s}\in C^{\infty}(S), including those monotone stratified states that are linearly stable such as ρs=x2\rho_{s}=-x_{2}. Namely, we can construct a smooth perturbation small in H2γH^{2-\gamma} norm for any γ>0\gamma>0, such that lim suptρ(t)ρsH˙s(S)=\limsup_{t\to\infty}\|\rho(t)-\rho_{s}\|_{\dot{H}^{s}(S)}=\infty for any s>1s>1.

Theorem 1.5.

Let ρsC(S)\rho_{s}\in C^{\infty}(S) be any stationary solution. For any ϵ,γ>0\epsilon,\gamma>0, there exists an initial data ρ0C(S)\rho_{0}\in C^{\infty}(S) satisfying

ρ0ρsH2γ(S)ϵ,\|\rho_{0}-\rho_{s}\|_{H^{2-\gamma}(S)}\leq\epsilon, (1.8)

such that the solution ρ(,t)\rho(\cdot,t) to (1.1) with initial data ρ0\rho_{0} (provided it remains smooth for all times) satisfies

lim suptts2ρ(t)ρsH˙s+1(S)= for all s>0.\limsup_{t\to\infty}t^{-\frac{s}{2}}\|\rho(t)-\rho_{s}\|_{\dot{H}^{s+1}(S)}=\infty\quad\text{ for all }s>0. (1.9)
Remark 1.6.

It is a natural question whether the perturbation can be made arbitrarily small in higher Sobolev spaces. While it is unclear to us whether H2H^{2} is the sharp threshold, we know that the exponent cannot exceed 10: for ρs=x2\rho_{s}=-x_{2}, if the initial perturbation is small in H10H^{10} or above, [1] showed ρ(t)ρsH3(S)\|\rho(t)-\rho_{s}\|_{H^{3}(S)} remains uniformly bounded in time.

1.3. Organization of the paper

In Section 2 we discuss some preliminaries and the local well-posedness results in the scenarios (S1)–(S3). In Section 3 we show the monotonicity of the potential energy in the three scenarios, and use it to prove the infinite-in-time growth results in Theorems 1.11.2. We take a brief detour in Section 4 to derive some infinite-in-time growth results for less restrictive initial data, which we call the “bubble” solution and the “layered” solution. This will enable us to obtain nonlinear instability results in Section 5 for initial data close to stratified steady states, where we prove Theorems 1.41.5.

2. Preliminaries on problem setting and local well-posedness

In this section, we discuss some preliminaries such as the Sobolev spaces for the spatial domains 2\mathbb{R}^{2}, 𝕋2\mathbb{T}^{2} and S=𝕋×[π,π]S=\mathbb{T}\times[-\pi,\pi] respectively, as well as the local-wellposedness results for the IPM equation (1.1). For the whole space and strip case, the local-wellposedness theory have already been established in [4] and [1] respectively. For the torus case we are unable to locate a local-wellposedness result, so we give a short proof in Section 2.2.

2.1. Sobolev norms and local well-posedness in 2\mathbb{R}^{2}

For any fL2(2)f\in L^{2}(\mathbb{R}^{2}), its Fourier transform is defined as usual as

f^(ξ):=12π2eiξxf(x)𝑑x for ξ2,\hat{f}(\xi):=\frac{1}{2\pi}\int_{\mathbb{R}^{2}}e^{-i\xi\cdot x}f(x)dx\quad\text{ for }\xi\in\mathbb{R}^{2},

and the Plancherel theorem yields f^L2(2)2=fL2(2)2.\|\hat{f}\|_{L^{2}(\mathbb{R}^{2})}^{2}=\|f\|_{L^{2}(\mathbb{R}^{2})}^{2}. As usual, we define

fH˙s(2)2:=2|ξ|2s|f^(ξ)|2𝑑ξ for any s0,\|f\|_{\dot{H}^{s}(\mathbb{R}^{2})}^{2}:=\int_{\mathbb{R}^{2}}|\xi|^{2s}|\hat{f}(\xi)|^{2}d\xi\quad\text{ for any }s\neq 0,

and

fHs(2)2:=2(1+|ξ|2)s|f^(ξ)|2𝑑ξ for any s.\|f\|_{{H}^{s}(\mathbb{R}^{2})}^{2}:=\int_{\mathbb{R}^{2}}(1+|\xi|^{2})^{s}|\hat{f}(\xi)|^{2}d\xi\quad\text{ for any }s\in\mathbb{R}.

For (1.1) in 2\mathbb{R}^{2}, Córdoba–Gancedo–Orive [5, Theorem 3.2] proved local-wellposedness for initial data ρ0Hs(2)\rho_{0}\in H^{s}(\mathbb{R}^{2}) with s>2s>2. They also established a regularity criteria, showing that ρ(t)\rho(t) remains regular as long as 0tρ(t)BMO𝑑s<\int_{0}^{t}\|\nabla\rho(t)\|_{BMO\,}ds<\infty. They also obtained another regularity criteria with a geometric flavor, and we refer the reader to [5, Theorem 3.4] for details.

2.2. Sobolev norms and local well-posedness in 𝕋2\mathbb{T}^{2}

For any fL1(𝕋2)f\in L^{1}(\mathbb{T}^{2}), let us denote its Fourier series as

f(x)=k2f^(k)eikx,f(x)=\sum_{k\in\mathbb{Z}^{2}}\hat{f}(k)e^{ik\cdot x}, (2.1)

where the Fourier coefficient f^(k)\hat{f}(k) for k=(k1,k2)2k=(k_{1},k_{2})\in\mathbb{Z}^{2} is given by

f^(k)=1(2π)2𝕋2eikxf(x)𝑑x.\hat{f}(k)=\frac{1}{(2\pi)^{2}}\int_{\mathbb{T}^{2}}e^{-ik\cdot x}f(x)dx. (2.2)

By Parseval’s theorem, for any f,gL2(𝕋2)f,g\in L^{2}(\mathbb{T}^{2}) we have 𝕋2f(x)g(x)¯𝑑x=(2π)2k2f^(k)g^(k)¯,\int_{\mathbb{T}^{2}}f(x)\overline{g(x)}dx=(2\pi)^{2}\sum_{k\in\mathbb{Z}^{2}}\hat{f}(k)\overline{\hat{g}(k)}, which in particular implies

fL2(𝕋2)2=(2π)2k2|f^(k)|2.\|f\|_{L^{2}(\mathbb{T}^{2})}^{2}=(2\pi)^{2}\sum_{k\in\mathbb{Z}^{2}}|\hat{f}(k)|^{2}. (2.3)

For s0s\neq 0, throughout this paper, fH˙s(𝕋2)\|f\|_{\dot{H}^{s}(\mathbb{T}^{2})} is defined by

fH˙s(𝕋2)2=(2π)2k2{(0,0)}|k|2s|f^(k)|2.\|f\|_{\dot{H}^{s}(\mathbb{T}^{2})}^{2}=(2\pi)^{2}\sum_{k\in\mathbb{Z}^{2}\setminus\{(0,0)\}}|k|^{2s}|\hat{f}(k)|^{2}. (2.4)

Finally, for mean-zero ff (in particular this is the case for x1ρ\partial_{x_{1}}\rho), its inverse Laplacian is given by (Δ)1f=k2{(0,0)}|k|2f^(k)eikx(-\Delta)^{-1}f=\sum_{k\in\mathbb{Z}^{2}\setminus\{(0,0)\}}|k|^{-2}\hat{f}(k)e^{ik\cdot x}.

Below we sketch a-priori estimates that can be used to establish local regularity as well as conditional criteria for global regularity. With these estimates, a fully rigorous argument can be given in a standard way, using either smooth mollifier approximations like in [14] or Galerkin approximations.

Suppose that ρ(x,t)\rho(x,t) is a smooth solution of tρ+(u)ρ=0,\partial_{t}\rho+(u\cdot\nabla)\rho=0, u=(Δ)1x1ρ,u=\nabla^{\perp}(-\Delta)^{-1}\partial_{x_{1}}\rho, where =(x2,x1).\nabla^{\perp}=(-\partial_{x_{2}},\partial_{x_{1}}). Observe that all the LpL^{p} norms of ρ\rho are conserved by evolution. Multiplying the equation by (Δ)sρ(-\Delta)^{s}\rho and integrating we obtain

12tρH˙s2+𝕋2(u)ρ(Δ)sρ𝑑x=0.\frac{1}{2}\partial_{t}\|\rho\|^{2}_{\dot{H}^{s}}+\int_{\mathbb{T}^{2}}(u\cdot\nabla)\rho(-\Delta)^{s}\rho\,dx=0.

Here s1s\geq 1 is an integer. In the integral above, we can expand the power of the Laplacian and integrate by parts, then use the periodicity to transfer exactly half of the derivatives on uρu\cdot\nabla\rho. What we get is a sum of terms of the form

𝕋2Ds((u)ρ)Dsρ𝑑x,\int_{\mathbb{T}^{2}}D^{s}((u\cdot\nabla)\rho)D^{s}\rho\,dx,

where DsD^{s} stands for some partial derivative of order s.s. Next we apply Leibniz rule to open up the derivative DsD^{s} falling on (u)ρ.(u\cdot\nabla)\rho. Note that when all derivatives fall on ρ,\rho, we get

𝕋2(u)DsρDsρ𝑑x=12𝕋2(u)(Dsρ)2𝑑x=0\int_{\mathbb{T}^{2}}(u\cdot\nabla)D^{s}\rho D^{s}\rho\,dx=\frac{1}{2}\int_{\mathbb{T}^{2}}(u\cdot\nabla)(D^{s}\rho)^{2}\,dx=0

due to incompressibility of u.u. Therefore we obtain a sum of the terms of the form

𝕋2DjuDsj+1ρDsρ𝑑x\int_{\mathbb{T}^{2}}D^{j}uD^{s-j+1}\rho D^{s}\rho\,dx

where 1js.1\leq j\leq s. Let us apply Hölder inequality to control such integral by

|𝕋2DjuDsj+1ρDsρ𝑑x|DjuLpjDsj+1ρLqjDsρL2,\left|\int_{\mathbb{T}^{2}}D^{j}uD^{s-j+1}\rho D^{s}\rho\,dx\right|\leq\|D^{j}u\|_{L^{p_{j}}}\|D^{s-j+1}\rho\|_{L^{q_{j}}}\|D^{s}\rho\|_{L^{2}},

where pj,p_{j}, qjq_{j} satisfy pj1+qj1=12.p_{j}^{-1}+q_{j}^{-1}=\frac{1}{2}. Let us recall a particular case of Gagliardo-Nirenberg inequality [9, 15]

DjfLqCfL1θfH˙sθ\|D^{j}f\|_{L^{q}}\leq C\|f\|_{L^{\infty}}^{1-\theta}\|f\|_{\dot{H}^{s}}^{\theta} (2.5)

for any fC0(2),f\in C_{0}^{\infty}(\mathbb{R}^{2}), where in the 2D case θ=j2qs1.\theta=\frac{j-\frac{2}{q}}{s-1}. The inequality is valid for s>j,s>j, 0<θ<1.0<\theta<1. While (2.5) is usually stated in 2,\mathbb{R}^{2}, an extension to 𝕋2\mathbb{T}^{2} is straightforward. Taking now pj=2(s+1)jp_{j}=\frac{2(s+1)}{j} and qj=2(s+1)s+1jq_{j}=\frac{2(s+1)}{s+1-j} and applying (2.5), we get

DjuLpjCDjρLpjCρL1jss21ρH˙sjss21,\|D^{j}u\|_{L^{p_{j}}}\leq C\|D^{j}\rho\|_{L^{p_{j}}}\leq C\|\rho\|_{L^{\infty}}^{1-\frac{js}{s^{2}-1}}\|\rho\|_{\dot{H}^{s}}^{\frac{js}{s^{2}-1}},

where in the first step we used LpLpL^{p}-L^{p} bound on singular integral operators for 1<p<.1<p<\infty. Similarly,

Ds+1jρLqjCρL1(s+1j)ss21ρH˙s(s+1j)ss21.\|D^{s+1-j}\rho\|_{L^{q_{j}}}\leq C\|\rho\|_{L^{\infty}}^{1-\frac{(s+1-j)s}{s^{2}-1}}\|\rho\|_{\dot{H}^{s}}^{\frac{(s+1-j)s}{s^{2}-1}}.

Therefore, for all 1js1\leq j\leq s we have

|𝕋2DjuDsj+1ρDsρ𝑑x|CρLs2s1ρH˙s2s1s1,\left|\int_{\mathbb{T}^{2}}D^{j}uD^{s-j+1}\rho D^{s}\rho\,dx\right|\leq C\|\rho\|_{L^{\infty}}^{\frac{s-2}{s-1}}\|\rho\|_{\dot{H}^{s}}^{\frac{2s-1}{s-1}},

and hence

tρH˙s2CρLs2s1ρH˙s2s1s1.\partial_{t}\|\rho\|^{2}_{\dot{H}^{s}}\leq C\|\rho\|_{L^{\infty}}^{\frac{s-2}{s-1}}\|\rho\|_{\dot{H}^{s}}^{\frac{2s-1}{s-1}}. (2.6)

Such inequality can be used to show local well-posedness in HsH^{s} provided that s>2.s>2.

To obtain a criteria for blow up, we can run a similar calculation but using ρL\|\nabla\rho\|_{L^{\infty}} and uL\|\nabla u\|_{L^{\infty}} instead of ρL\|\rho\|_{L^{\infty}} and with pj=2s/j,p_{j}=2s/j, qj=2s/(sj).q_{j}=2s/(s-j). This way instead of (2.6) we obtain the differential inequality

tρH˙s2C(ρL+uL)ρH˙s2.\partial_{t}\|\rho\|^{2}_{\dot{H}^{s}}\leq C\left(\|\nabla\rho\|_{L^{\infty}}+\|\nabla u\|_{L^{\infty}}\right)\|\rho\|_{\dot{H}^{s}}^{2}.

We can conclude control of ρH˙s\|\rho\|_{\dot{H}^{s}} up to any time TT provided that 0T(ρL+uL)𝑑t\int_{0}^{T}\left(\|\nabla\rho\|_{L^{\infty}}+\|\nabla u\|_{L^{\infty}}\right)\,dt remains finite. Let us state a proposition summarizing the observations of this section.

Proposition 2.1.

Consider the IPM equation (1.1) with the initial data ρ0Hs(𝕋2),\rho_{0}\in H^{s}(\mathbb{T}^{2}), s>2s>2 an integer. Then there exists a time T=T(ρ0Hs)T=T(\|\rho_{0}\|_{H^{s}}) such that for all 0tT0\leq t\leq T there exists a unique solution ρ(x,t),u(x,t)C([0,T],Hs(𝕋2)).\rho(x,t),u(x,t)\in C([0,T],H^{s}(\mathbb{T}^{2})). Moreover, the solution blows up at time TT if and only if

0t(ρ(,r)L(𝕋2)+u(,r)L(𝕋2))𝑑r\int_{0}^{t}\left(\|\nabla\rho(\cdot,r)\|_{L^{\infty}(\mathbb{T}^{2})}+\|\nabla u(\cdot,r)\|_{L^{\infty}(\mathbb{T}^{2})}\right)\,dr\rightarrow\infty

when tT.t\rightarrow T.

Remarks. 1. Uniqueness of the solution can be shown in a standard way; blow up is understood in the sense of leaving the class C([0,T],Hs(𝕋2)).C([0,T],H^{s}(\mathbb{T}^{2})).
2. The Proposition can certainly be improved in terms of the condition on ss and the regularity criterion, but we do not pursue it in this paper.

2.3. Sobolev norms and local well-posedness in a strip

When the domain is a bounded strip S:=𝕋×[π,π]S:=\mathbb{T}\times[-\pi,\pi], due to the presence of the top and bottom boundaries, the functional spaces and the local-wellposedness results are more involved than the periodic case. Below we briefly describe the results by Castro–Córdoba–Lear [1], and we refer the readers to the paper for more details.

Biot-Savart law and functional space. In the strip case, the velocity field uu is given by u=ψu=\nabla^{\perp}\psi, where the stream function ψ\psi solves the Poisson’s equation with zero boundary condition (see [1, Section 2.2] for a derivation):

{Δψ(,t)=x1ρ(,t) in S×[0,T),ψ(,t)=0 on S×[0,T),\begin{cases}-\Delta\psi(\cdot,t)=\partial_{x_{1}}\rho(\cdot,t)&\text{ in }S\times[0,T),\\ \psi(\cdot,t)=0&\text{ on }\partial S\times[0,T),\end{cases} (2.7)

so that u=(ΔS)1x1ρu=\nabla^{\perp}(-\Delta_{S})^{-1}\partial_{x_{1}}\rho. One can check that the operator ΔS-\Delta_{S} (with zero boundary condition) is a positive self-adjoint operator, and it has a family of eigenfunctions {ωp,q}p,q\{\omega_{p,q}\}_{p\in\mathbb{Z},q\in\mathbb{N}} that form an orthonormal basis for L2(S)L^{2}(S), given by

ωp,q(x):=ap(x1)bq(x2) for p,q,\omega_{p,q}(x):=a_{p}(x_{1})b_{q}(x_{2})\quad\text{ for }p\in\mathbb{Z},q\in\mathbb{N},

where

ap(x1):=eipx1 with x1𝕋 and p,a_{p}(x_{1}):=e^{ipx_{1}}\quad\text{ with }x_{1}\in\mathbb{T}\text{ and }p\in\mathbb{Z},

and

bq(x2):={cos(qx22)q odd,sin(qx22)q even, with x2[π,π] for q.b_{q}(x_{2}):=\begin{cases}\cos(\frac{qx_{2}}{2})&q\text{ odd,}\\ \sin(\frac{qx_{2}}{2})&q\text{ even,}\end{cases}\text{ with }x_{2}\in[-\pi,\pi]\text{ for }q\in\mathbb{N}.

The eigenfunction expansion allows us to define (ΔS)sf(-\Delta_{S})^{s}f for any ss\in\mathbb{R} and fL2(S)f\in L^{2}(S). We can then define the H˙s\dot{H}^{s} homogenous Sobolev norm as

fH˙s(S)2:=Sf(ΔS)sf𝑑x for s,\|f\|_{\dot{H}^{s}(S)}^{2}:=\int_{S}f(-\Delta_{S})^{s}fdx\quad\text{ for }s\in\mathbb{R}, (2.8)

and one can check that the spaces H˙s(S)\dot{H}^{s}(S) and H˙s(S)\dot{H}^{-s}(S) are dual with respect to the L2L^{2} norm (see e.g. [17] for the general construction of a scale of Sobolev spaces associated with a positive self-adjoint operator).

For s0s\geq 0, let us define fHs(S)2:=fH˙s(S)2+fL2(S)2\|f\|_{H^{s}(S)}^{2}:=\|f\|_{\dot{H}^{s}(S)}^{2}+\|f\|_{L^{2}(S)}^{2} as usual. For ss\in\mathbb{N}, the above definition of fHs(S)2\|f\|_{{H}^{s}(S)}^{2} is comparable to 0msDmfL2(S)2\sum_{0\leq m\leq s}\|D^{m}f\|_{L^{2}(S)}^{2} if x2nf|S=0\partial_{x_{2}}^{n}f|_{\partial S}=0 for all even nn with n<sn<s, where DmD^{m} is any partial derivative of order msm\leq s.

Local/global well-posedness results in the strip. Since the goal of [1] was to establish stability results near the steady state ρs(x)=x2\rho_{s}(x)=-x_{2}, (1.1) was written into an equivalent equation (1.6) (with g(x2)=x2g(x_{2})=-x_{2}) describing the evolution of η=ρρs\eta=\rho-\rho_{s}. Here uu can be expressed in terms of η\eta similarly to (2.7), except that the right hand side x1ρ\partial_{x_{1}}\rho is replaced by x1η\partial_{x_{1}}\eta (using that ρs\rho_{s} has zero contribution to uu since it is a steady state).

When the initial data η(0)\eta(0) belongs to the functional space Xk(S)X^{k}(S), given by

Xk(S):={fHk(𝕋2):x2nf|S=0 for all even n with n<k},X^{k}(S):=\{f\in H^{k}(\mathbb{T}^{2}):\partial_{x_{2}}^{n}f|_{\partial S}=0\text{ for all even $n$ with $n<k$}\},

(which in fact coincides with Hk(S)H^{k}(S) defined above), the authors proved local-wellposedness of (1.6) for η(0)Xk(S)\eta(0)\in X^{k}(S) for any k3k\geq 3 [1, Theorem 4.1], and gave a regularity criteria showing that η(t)\eta(t) remains in Xk(S)X^{k}(S) as long as 0t(η(s)L(S)+u(s)L(S))𝑑s<\int_{0}^{t}(\|\nabla\eta(s)\|_{L^{\infty}(S)}+\|\nabla u(s)\|_{L^{\infty}(S)})ds<\infty. As we discussed in the introduction, for k10k\geq 10, they proved the asymptotic stability of η(t)\eta(t) (which implies global regularity) for η(0)Xk(S)\eta(0)\in X^{k}(S) with η(0)Xk(S)1\|\eta(0)\|_{X^{k}(S)}\ll 1.

3. Infinite-in-time growth in the IPM

In this section we aim to prove Theorems 1.1 and 1.2. Throughout this paper, the evolution of the potential energy

E(t):=Ωx2ρ(x,t)𝑑x.E(t):=\int_{\Omega}x_{2}\rho(x,t)\,dx.

plays a key role. Let us first prove a simple lemma showing that in each of the scenarios (S1)–(S3), E(t)E(t) is monotone decreasing in time, and its time derivative is integrable in t(0,)t\in(0,\infty).

Lemma 3.1.

Assume that Ω\Omega and ρ0\rho_{0} satisfy one of the scenarios (S1)–(S3). Assuming that there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}, we have

ddtE(t)=x1ρH˙1(Ω)2=:δ(t).\frac{d}{dt}E(t)=-\underbrace{\|\partial_{x_{1}}\rho\|_{\dot{H}^{-1}(\Omega)}^{2}}_{=:\delta(t)}.

In addition, we have 0δ(t)𝑑tC(ρ0)<\int_{0}^{\infty}\delta(t)dt\leq C(\rho_{0})<\infty.

Proof.

A direct computation gives

E(t)=ddtΩx2ρ(x,t)𝑑x=Ωx2(u)ρ𝑑x=Ωu2ρ𝑑x.E^{\prime}(t)=\frac{d}{dt}\int_{\Omega}x_{2}\rho(x,t)\,dx=-\int_{\Omega}x_{2}(u\cdot\nabla)\rho\,dx=\int_{\Omega}u_{2}\rho\,dx. (3.1)

Here the last inequality is due to the divergence theorem, where the boundary integral vanishes in all the three scenarios (S1)–(S3): In (S1), the boundary integral (at infinity) vanishes since ρ(,t)Cc(2)\rho(\cdot,t)\in C_{c}^{\infty}(\mathbb{R}^{2}) for all time. In (S2), the boundary integral ππx2u1ρ𝑑x2|x1=πx1=π=0\int_{-\pi}^{\pi}x_{2}u_{1}\rho\,dx_{2}\big{|}_{x_{1}=-\pi}^{x_{1}=\pi}=0 due to periodicity, and ππx2u2ρ𝑑x1|x2=πx2=π=0\int_{-\pi}^{\pi}x_{2}u_{2}\rho\,dx_{1}\big{|}_{x_{2}=-\pi}^{x_{2}=\pi}=0 since ρ0\rho\equiv 0 on x2=±πx_{2}=\pm\pi (which follows from the facts that ρ(,t)\rho(\cdot,t) is odd in x2x_{2}, and periodic in 𝕋2\mathbb{T}^{2}). In (S3), again 11x2u1ρ𝑑x2|x1=πx1=π=0\int_{-1}^{1}x_{2}u_{1}\rho\,dx_{2}\big{|}_{x_{1}=-\pi}^{x_{1}=\pi}=0 due to periodicity in x1x_{1}, whereas ππx2u2ρ𝑑x1|x2=1x2=1=0\int_{-\pi}^{\pi}x_{2}u_{2}\rho\,dx_{1}\big{|}_{x_{2}=-1}^{x_{2}=1}=0 due to un=0u\cdot n=0 on x2=±πx_{2}=\pm\pi.

By (3.1) and the Biot-Savart law u=(ΔΩ)1x1ρu=\nabla^{\perp}(-\Delta_{\Omega})^{-1}\partial_{x_{1}}\rho, in (S1)–(S3), we get

E(t)=Ωu2ρ𝑑x=Ωρx1(ΔΩ)1x1ρdx=x1ρH˙1(Ω)2,E^{\prime}(t)=\int_{\Omega}u_{2}\rho\,dx=\int_{\Omega}\rho\partial_{x_{1}}(-\Delta_{\Omega})^{-1}\partial_{x_{1}}\rho\,dx=-\|\partial_{x_{1}}\rho\|_{\dot{H}^{-1}(\Omega)}^{2}, (3.2)

thus E(t)E(t) is monotone decreasing. Note that in the strip case Ω=S\Omega=S, the last identity follows from the definition of the H˙1\dot{H}^{-1} norm in SS as in (2.8).

Moreover, E(t)E(t) is uniformly bounded below for all times. In (S1), the assumptions that ρ0\rho_{0} is odd in x2x_{2} and ρ00\rho_{0}\geq 0 in ×+\mathbb{R}\times\mathbb{R}^{+} yield that ρ(t)0\rho(t)\geq 0 in ×+\mathbb{R}\times\mathbb{R}^{+}, thus E(t)0E(t)\geq 0 for all times. In (S2) and (S3), since a smooth solution ρ(x,t)\rho(x,t) of (1.1) has its LL^{\infty} norm invariant in time, we have that

E(t)ρ0L(Ω)4π0πx2𝑑x2=2π3ρ0L(Ω) for all t0.E(t)\geq-\|\rho_{0}\|_{L^{\infty}(\Omega)}4\pi\int_{0}^{\pi}x_{2}dx_{2}=-2\pi^{3}\|\rho_{0}\|_{L^{\infty}(\Omega)}\quad\text{ for all }t\geq 0.

Hence in all three cases (S1)–(S3), we have

0δ(t)𝑑t=0x1ρ(,t)H˙1(Ω)2𝑑t=E(0)limtE(t)C(ρ0) for all t0,\int_{0}^{\infty}\delta(t)\,dt=\int_{0}^{\infty}\|\partial_{x_{1}}\rho(\cdot,t)\|_{\dot{H}^{-1}(\Omega)}^{2}\,dt=E(0)-\lim_{t\to\infty}E(t)\leq C(\rho_{0})\quad\text{ for all }t\geq 0, (3.3)

finishing the proof. ∎

Remark 3.2.

When the equation is set in 2\mathbb{R}^{2} with ρ\rho decaying sufficiently fast, monotonicity of E(t)E(t) has been derived in [7, Corollary 1.2]. For the Muskat equation (which can be seen as a “patch” solution of IPM) with surface tension, [11] uses the gradient flow structure to construct weak solutions, where the energy functional is the potential energy plus the surface area of the free boundary.

Now we are ready to prove Theorems 1.1 and 1.2.

Proof of Theorem 1.1.

Due to Lemma 3.1, δ(t):=x1ρ(t)H˙1(2)2\delta(t):=\|\partial_{x_{1}}\rho(t)\|_{\dot{H}^{-1}(\mathbb{R}^{2})}^{2} satisfies 0δ(t)𝑑t<C0(ρ0)<\int_{0}^{\infty}\delta(t)dt<C_{0}(\rho_{0})<\infty. Denoting C2:=ρ0L2(2)2C_{2}:=\|\rho_{0}\|_{L^{2}(\mathbb{R}^{2})}^{2}, we have ρ(t)L2(2)2=C2\|\rho(t)\|_{L^{2}(\mathbb{R}^{2})}^{2}=C_{2} for all t0t\geq 0, since the LpL^{p} norm of ρ\rho is invariant in time for all 1p1\leq p\leq\infty. Let us define I:={t(0,):δ(t)<14C2}.I:=\left\{t\in(0,\infty):\delta(t)<\frac{1}{4}C_{2}\right\}. Note that 0δ(t)𝑑tC0(ρ0)\int_{0}^{\infty}\delta(t)dt\leq C_{0}(\rho_{0}) directly implies |+I|4C0(ρ0)/C2|\mathbb{R}^{+}\setminus I|\leq 4C_{0}(\rho_{0})/C_{2}. We claim that for any s>0s>0,

ρ(t)H˙s(2)C(s,ρ0L1(2),C2)δ(t)s4 for any tI.\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}\geq C(s,\|\rho_{0}\|_{L^{1}(\mathbb{R}^{2})},C_{2})\delta(t)^{-\frac{s}{4}}\quad\text{ for any }t\in I. (3.4)

Once we prove (3.4), plugging it into 0δ(t)𝑑tC0(ρ0)\int_{0}^{\infty}\delta(t)dt\leq C_{0}(\rho_{0}) and using the fact that |+I|4C0(ρ0)/C2|\mathbb{R}^{+}\setminus I|\leq 4C_{0}(\rho_{0})/C_{2}, we have

0ρ(t)H˙s(2)4s𝑑tC(s,ρ0L1,C2)4sIδ(t)𝑑t+4C0(ρ0)C2(inft0ρ(t)H˙s(2))4sC(s,ρ0).\int_{0}^{\infty}\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}^{-\frac{4}{s}}dt\leq C(s,\|\rho_{0}\|_{L^{1}},C_{2})^{-\frac{4}{s}}\int_{I}\delta(t)dt+\frac{4C_{0}(\rho_{0})}{C_{2}}\left(\inf_{t\geq 0}\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}\right)^{-\frac{4}{s}}\leq C(s,\rho_{0}).

Here in the last inequality we used that for any s>0s>0, ρ(t)H˙s(2)\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})} is bounded below by a positive constant c(s,ρ0)c(s,\rho_{0}), which follows from the elementary interpolation inequality ρ(t)L2(2)ρ(t)H˙s(2)11+sρL1(2)s1+s\|\rho(t)\|_{L^{2}(\mathbb{R}^{2})}\leq\|\rho(t)\|_{\dot{H}^{s}(\mathbb{R}^{2})}^{\frac{1}{1+s}}\|\rho\|_{L^{1}(\mathbb{R}^{2})}^{\frac{s}{1+s}}, as well as the fact that ρ(t)L2(2)\|\rho(t)\|_{L^{2}(\mathbb{R}^{2})} and ρ(t)L1(2)\|\rho(t)\|_{L^{1}(\mathbb{R}^{2})} are invariant in time. This finishes the proof of (1.2). Combining (1.2) with the fact that 1t1𝑑t=\int_{1}^{\infty}t^{-1}dt=\infty gives (1.3) as a direct consequence.

In the rest we aim to prove (3.4) for any fixed tIt\in I, and we will drop the tt dependence in ρ\rho and δ\delta below for notational simplicity. Defining

Dδ:={(ξ1,ξ2):|ξ1||ξ|2δC2}.D_{\delta}:=\left\{(\xi_{1},\xi_{2}):\frac{|\xi_{1}|}{|\xi|}\geq\sqrt{\frac{2\delta}{C_{2}}}\right\}.

we observe that

δ=x1ρH˙1(2)2=2ξ12|ξ|2|ρ^(ξ)|2𝑑ξDδξ12|ξ|2|ρ^(ξ)|2𝑑ξ2δC2Dδ|ρ^|2𝑑ξ.\delta=\|\partial_{x_{1}}\rho\|_{\dot{H}^{-1}(\mathbb{R}^{2})}^{2}=\int_{\mathbb{R}^{2}}\frac{\xi_{1}^{2}}{|\xi|^{2}}|\hat{\rho}(\xi)|^{2}d\xi\geq\int_{D_{\delta}}\frac{\xi_{1}^{2}}{|\xi|^{2}}|\hat{\rho}(\xi)|^{2}d\xi\geq\frac{2\delta}{C_{2}}\int_{D_{\delta}}|\hat{\rho}|^{2}d\xi.

This gives Dδ|ρ^|2𝑑ξ12C2\int_{D_{\delta}}|\hat{\rho}|^{2}d\xi\leq\frac{1}{2}C_{2}, and combining it with ρ^L2(2)2=ρL2(2)2=C2\|\hat{\rho}\|_{L^{2}(\mathbb{R}^{2})}^{2}=\|\rho\|_{L^{2}(\mathbb{R}^{2})}^{2}=C_{2} yields Dδc|ρ^|2𝑑ξ12C2\int_{D_{\delta}^{c}}|\hat{\rho}|^{2}d\xi\geq\frac{1}{2}C_{2}. Note that DδcD_{\delta}^{c} consists of two symmetric cones containing the ξ2\xi_{2} axis, and it can be expressed in polar coordinates as Dδc={(rcosθ,rsinθ):r0,|cosθ|<2δ/C2D_{\delta}^{c}=\{(r\cos\theta,r\sin\theta):r\geq 0,|\cos\theta|<\sqrt{2\delta/C_{2}}}.

Clearly, ρ^L(2)(2π)1ρ0L1(2)=:C1\|\hat{\rho}\|_{L^{\infty}(\mathbb{R}^{2})}\leq(2\pi)^{-1}\|\rho_{0}\|_{L^{1}(\mathbb{R}^{2})}=:C_{1}. Let hδ>0h_{\delta}>0 be such that |Dδc{|ξ2|<hδ}|=(4C12)1C2|D_{\delta}^{c}\cap\{|\xi_{2}|<h_{\delta}\}|=(4C_{1}^{2})^{-1}C_{2}, which will be estimated momentarily. Such definition gives

Dδc{|ξ2|hδ}|ρ^|2𝑑ξ=Dδc|ρ^|2𝑑ξDδc{|ξ2|<hδ}|ρ^|2𝑑ξ12C2(4C12)1C2C12=14C2,\int_{D_{\delta}^{c}\cap\{|\xi_{2}|\geq h_{\delta}\}}|\hat{\rho}|^{2}d\xi=\int_{D_{\delta}^{c}}|\hat{\rho}|^{2}d\xi-\int_{D_{\delta}^{c}\cap\{|\xi_{2}|<h_{\delta}\}}|\hat{\rho}|^{2}d\xi\geq\frac{1}{2}C_{2}-(4C_{1}^{2})^{-1}C_{2}C_{1}^{2}=\frac{1}{4}C_{2},

immediately leading to

ρH˙s(2)22|ξ2|2s|ρ^|2𝑑ξhδ2sDδc{|ξ2|hδ}|ρ^|2𝑑ξC24hδ2s.\|\rho\|_{\dot{H}^{s}(\mathbb{R}^{2})}^{2}\geq\int_{\mathbb{R}^{2}}|\xi_{2}|^{2s}|\hat{\rho}|^{2}d\xi\geq h_{\delta}^{2s}\int_{D_{\delta}^{c}\cap\{|\xi_{2}|\geq h_{\delta}\}}|\hat{\rho}|^{2}d\xi\geq\frac{C_{2}}{4}h_{\delta}^{2s}. (3.5)

It remains to estimate hδh_{\delta}. Denoting θ0:=cos1(2δC2)\theta_{0}:=\cos^{-1}(\sqrt{\frac{2\delta}{C_{2}}}), we know Dδc{|ξ2|<hδ}D_{\delta}^{c}\cap\{|\xi_{2}|<h_{\delta}\} consists of two identical triangles with height hδh_{\delta} and base 2hδcotθ02h_{\delta}\cot\theta_{0}. Thus

(4C12)1C2=|Dδc{|ξ2|<hδ}|=2hδ2cotθ04δC21/2hδ2,(4C_{1}^{2})^{-1}C_{2}=|D_{\delta}^{c}\cap\{|\xi_{2}|<h_{\delta}\}|=2h_{\delta}^{2}\cot\theta_{0}\leq 4\sqrt{\delta}C_{2}^{-1/2}h_{\delta}^{2},

where in the last inequality we used cosθ0=2δC2\cos\theta_{0}=\sqrt{\frac{2\delta}{C_{2}}} and sinθ0=12δC21/2\sin\theta_{0}=\sqrt{1-\frac{2\delta}{C_{2}}}\geq 1/\sqrt{2}, due to tIt\in I. Therefore hδ(4C1)1C23/4δ1/4h_{\delta}\geq(4C_{1})^{-1}C_{2}^{3/4}\delta^{-1/4}. Plugging it into (3.5) yields (3.4), finishing the proof. ∎

Proof of Theorem 1.2.

Since ρ0\rho_{0} is even in x1x_{1} and odd in x2x_{2}, due to the Biot-Savart law u=(Δ)1x1ρu=\nabla^{\perp}(-\Delta)^{-1}\partial_{x_{1}}\rho, the even-odd symmetry of ρ\rho remains true for all times. In particular, it implies that on the boundary of the smaller square D:=[0,π]2D:=[0,\pi]^{2}, we have u(,t)n|D=0u(\cdot,t)\cdot n|_{\partial D}=0, and combining it with ρ00\rho_{0}\geq 0 on DD gives ρ(t)0\rho(t)\geq 0 on DD for all times. In addition, note that ρ0=0\rho_{0}=0 on x1=0x_{1}=0 and the fact that u(,t)n|D=0u(\cdot,t)\cdot n|_{\partial D}=0 imply ρ(0,x2,t)0\rho(0,x_{2},t)\equiv 0 for all x2x_{2} and tt.

For any t0t\geq 0, ρ(,t):𝕋2\rho(\cdot,t):\mathbb{T}^{2}\to\mathbb{R} has Fourier series (2.1)–(2.2) (with ff replaced by ρ(,t)\rho(\cdot,t)), and the Fourier coefficient ρ^(k,t)\hat{\rho}(k,t) for k=(k1,k2)2k=(k_{1},k_{2})\in\mathbb{Z}^{2} can be written as

ρ^(k,t)=1(2π)2𝕋eik1x1𝕋eik2x2ρ(x1,x2,t)𝑑x2𝑑x1=1(2π)2𝕋eik1x1(2i)0πsin(k2x2)ρ(x1,x2,t)𝑑x2=:g(x1,k2,t)𝑑x1,\begin{split}\hat{\rho}(k,t)&=\frac{1}{(2\pi)^{2}}\int_{\mathbb{T}}e^{-ik_{1}x_{1}}\int_{\mathbb{T}}e^{-ik_{2}x_{2}}\rho(x_{1},x_{2},t)dx_{2}dx_{1}\\ &=\frac{1}{(2\pi)^{2}}\int_{\mathbb{T}}e^{-ik_{1}x_{1}}(-2i)\underbrace{\int_{0}^{\pi}\sin(k_{2}x_{2})\rho(x_{1},x_{2},t)dx_{2}}_{=:g(x_{1},k_{2},t)}dx_{1},\end{split} (3.6)

where the last identity follows from the oddness of ρ(,t)\rho(\cdot,t) in x2x_{2}.

Let us take a closer look at the function g(x1,1,t)g(x_{1},1,t) in the last line of (3.6) (where we set k2=1k_{2}=1). It satisfies the following properties for all t0t\geq 0:

  1. (a)

    g(x1,1,t)0g(x_{1},1,t)\geq 0 for all x1𝕋x_{1}\in\mathbb{T} and t0t\geq 0, and is even in x1x_{1}.

  2. (b)

    g(0,1,t)=0g(0,1,t)=0 for all t0t\geq 0.

  3. (c)

    𝕋g(x1,1,t)𝑑x1c(ρ0)\int_{\mathbb{T}}g(x_{1},1,t)dx_{1}\geq c(\rho_{0}) for all t0t\geq 0, where c(ρ0)>0c(\rho_{0})>0 only depends on ρ0\rho_{0}.

Here properties (a, b) follow from the facts that ρ(t)\rho(t) is even in x1x_{1}, nonnegative on D=[0,π]2D=[0,\pi]^{2}, and ρ(0,x2,t)0\rho(0,x_{2},t)\equiv 0 for all times. For property (c), note that 𝕋g(x1,1,t)𝑑x1=20πg(x1,1,t)𝑑x1=2Dsin(x2)ρ(x,t)𝑑x.\int_{\mathbb{T}}g(x_{1},1,t)dx_{1}=2\int_{0}^{\pi}g(x_{1},1,t)dx_{1}=2\int_{D}\sin(x_{2})\rho(x,t)dx. Hölder’s inequality and the fact that sin(x2)ρ(x,t)0\sin(x_{2})\rho(x,t)\geq 0 in DD yield that

Dsin(x2)ρ(x,t)dx(Dsin(x2)1/2dx)2(Dρ(x,t)1/3dx)3c(Dρ(x,t)1/3dx)3,\int_{D}\sin(x_{2})\rho(x,t)dx\geq\left(\int_{D}\sin(x_{2})^{-1/2}dx\right)^{-2}\left(\int_{D}\rho(x,t)^{1/3}dx\right)^{3}\geq c\left(\int_{D}\rho(x,t)^{1/3}dx\right)^{3},

where c>0c>0 is a universal constant. Since ρ\rho is advected by a divergence-free flow uu with un|D=0u\cdot n|_{\partial D}=0, one can easily check that Dρ(x,t)1/3𝑑x=Dρ01/3𝑑x>c1\int_{D}\rho(x,t)^{1/3}dx=\int_{D}\rho_{0}^{1/3}dx>c_{1} for some c1(ρ0)>0c_{1}(\rho_{0})>0, finishing the proof of property (c).

Let us define g^(k1,t)\hat{g}(k_{1},t) as the Fourier coefficient of g(,1,t)g(\cdot,1,t), given by

g^(k1,t):=12π𝕋eik1x1g(x1,1,t)𝑑x for any k1.\hat{g}(k_{1},t):=\frac{1}{2\pi}\int_{\mathbb{T}}e^{-ik_{1}x_{1}}g(x_{1},1,t)dx\quad\text{ for any }k_{1}\in\mathbb{Z}. (3.7)

Comparing (3.7) with (3.6) directly yields

ρ^(k1,1,t)=2i2πg^(k1,t) for any k1.\hat{\rho}(k_{1},1,t)=\frac{-2i}{2\pi}\hat{g}(k_{1},t)\quad\text{ for any }k_{1}\in\mathbb{Z}. (3.8)

Using the functions gg and g^\hat{g}, we can estimate δ(t)=ρ(t)H˙1(𝕋2)2\delta(t)=\|\rho(t)\|_{\dot{H}^{-1}(\mathbb{T}^{2})}^{2} from below as

δ(t)=(2π)2k2{(0,0)}k12|k|2|ρ^(k1,k2,t)|2(2π)2k1{0}k12k12+1|ρ^(k1,1,t)|22k1{0}|g^(k1,t)|2=1π𝕋|g(x1,1,t)g¯(t)|2𝑑x1\begin{split}\delta(t)&=(2\pi)^{2}\sum_{k\in\mathbb{Z}^{2}\setminus\{(0,0)\}}\frac{k_{1}^{2}}{|k|^{2}}|\hat{\rho}(k_{1},k_{2},t)|^{2}\geq(2\pi)^{2}\sum_{k_{1}\in\mathbb{Z}\setminus\{0\}}\frac{k_{1}^{2}}{k_{1}^{2}+1}|\hat{\rho}(k_{1},1,t)|^{2}\\ &\geq 2\sum_{k_{1}\in\mathbb{Z}\setminus\{0\}}|\hat{g}(k_{1},t)|^{2}=\frac{1}{\pi}\int_{\mathbb{T}}|g(x_{1},1,t)-\bar{g}(t)|^{2}dx_{1}\end{split} (3.9)

where g¯(t):=12π𝕋g(x1,1,t)𝑑x1\bar{g}(t):=\frac{1}{2\pi}\int_{\mathbb{T}}g(x_{1},1,t)dx_{1} is the average of g(,1,t)g(\cdot,1,t) in 𝕋\mathbb{T}. By property (c), we have g¯(t)c(ρ0)2π>0\bar{g}(t)\geq\frac{c(\rho_{0})}{2\pi}>0 for all t0t\geq 0. Intuitively, if δ(t)\delta(t) is small, g(,1,t)g(\cdot,1,t) must be very close to g¯(t)\bar{g}(t) in L2L^{2}. With g(0,1,t)g(0,1,t) pinned down at zero (by property (b)), and g¯\bar{g} being uniformly positive, g(,1,t)g(\cdot,1,t) must have order 1 oscillations in a small neighborhood near 0, suggesting it should have a large H˙α\dot{H}^{\alpha} norm for α>12\alpha>\frac{1}{2}. This estimate will be made rigorous in Lemma 3.3 right after the proof. Applying Lemma 3.3 to g(x1,1,t)g(x_{1},1,t), we have

g(,1,t)H˙α(𝕋)c(α,ρ0)δ(t)α+12 for all α>12.\|g(\cdot,1,t)\|_{\dot{H}^{\alpha}(\mathbb{T})}\geq c(\alpha,\rho_{0})\delta(t)^{-\alpha+\frac{1}{2}}\quad\text{ for all }\alpha>\frac{1}{2}. (3.10)

Note that

g(,1,t)H˙α(𝕋)2=2πk10|k1|2α|g^(k1,t)|2=2π3k10|k1|2α|ρ^(k1,1,t)|2π2x1ρH˙α1(𝕋2)2,\|g(\cdot,1,t)\|_{\dot{H}^{\alpha}(\mathbb{T})}^{2}=2\pi\sum_{k_{1}\neq 0}|k_{1}|^{2\alpha}|\hat{g}(k_{1},t)|^{2}=2\pi^{3}\sum_{k_{1}\neq 0}|k_{1}|^{2\alpha}|\hat{\rho}(k_{1},1,t)|^{2}\leq\frac{\pi}{\sqrt{2}}\|\partial_{x_{1}}\rho\|_{\dot{H}^{\alpha-1}(\mathbb{T}^{2})}^{2},

where the last inequality follows by just looking at the k2=1k_{2}=1 part of the sum for the last norm taken on Fourier side and using α>1/2.\alpha>1/2. Setting s:=α1s:=\alpha-1 and applying (3.10), we have

x1ρH˙s(2π)1/2g(,1,t)H˙s+1(𝕋)c(s,ρ0)δs12 for s>12.\|\partial_{x_{1}}\rho\|_{\dot{H}^{s}}\geq\Big{(}\frac{\sqrt{2}}{\pi}\Big{)}^{1/2}\|g(\cdot,1,t)\|_{\dot{H}^{s+1}(\mathbb{T})}\geq c(s,\rho_{0})\delta^{-s-\frac{1}{2}}\quad\text{ for }s>-\frac{1}{2}.

Plugging this inequality into 0δ(t)𝑑tC0(ρ0)<\int_{0}^{\infty}\delta(t)dt\leq C_{0}(\rho_{0})<\infty implies (1.4), and combining (1.4) with the fact that 1t1𝑑t=\int_{1}^{\infty}t^{-1}dt=\infty gives (1.5) as a direct consequence. ∎

Now we state and prove the lemma used in the proof of Theorem 1.2.

Lemma 3.3.

If f:𝕋f:\mathbb{T}\to\mathbb{R} satisfies f(0)=0f(0)=0, 𝕋f(x)𝑑xc0>0\int_{\mathbb{T}}f(x)dx\geq c_{0}>0 and 𝕋|ff¯|2𝑑x<δ\int_{\mathbb{T}}|f-\bar{f}|^{2}dx<\delta (where f¯:=12π𝕋f(x)𝑑x\bar{f}:=\frac{1}{2\pi}\int_{\mathbb{T}}f(x)dx), then

fH˙α(𝕋)c(α,c0)δα+12 for all α>12.\|f\|_{\dot{H}^{\alpha}(\mathbb{T})}\geq c(\alpha,c_{0})\delta^{-\alpha+\frac{1}{2}}\quad\text{ for all }\alpha>\frac{1}{2}. (3.11)
Proof.

Note that h(x):=f(x)f¯h(x):=f(x)-\bar{f} has mean zero in 𝕋\mathbb{T}, and h(0)=f¯c0h(0)=-\bar{f}\leq-c_{0}. By the assumption 𝕋h2𝑑x<δ\int_{\mathbb{T}}h^{2}dx<\delta, there exists some x0(0,4δc02)x_{0}\in(0,\frac{4\delta}{c_{0}^{2}}) such that h(x0)>c02h(x_{0})>-\frac{c_{0}}{2}. This implies

hCγ(𝕋)|h(x0)h(0)||x00|γ(c0/2)1+2γδγ for all 0<γ1.\|h\|_{C^{\gamma}(\mathbb{T})}\geq\frac{|h(x_{0})-h(0)|}{|x_{0}-0|^{\gamma}}\geq(c_{0}/2)^{1+2\gamma}\delta^{-\gamma}\quad\text{ for all }0<\gamma\leq 1.

Applying the Sobolev embedding theorem, we have

hH˙γ+12(𝕋)c(γ)hCγ(𝕋)c(γ,c0)δγ for all 0<γ1,\|h\|_{\dot{H}^{\gamma+\frac{1}{2}}(\mathbb{T})}\geq c(\gamma)\|h\|_{C^{\gamma}(\mathbb{T})}\geq c(\gamma,c_{0})\delta^{-\gamma}\quad\text{ for all }0<\gamma\leq 1,

and setting α=γ+12\alpha=\gamma+\frac{1}{2} gives (3.11) for α(12,32]\alpha\in(\frac{1}{2},\frac{3}{2}], where we also use that hH˙α(𝕋)=fH˙α(𝕋)\|h\|_{\dot{H}^{\alpha}(\mathbb{T})}=\|f\|_{\dot{H}^{\alpha}(\mathbb{T})}. For α>32\alpha>\frac{3}{2}, we can apply the interpolation inequality hH˙1(𝕋)hH˙α(𝕋)1αhL2(𝕋)α1α\|h\|_{\dot{H}^{1}(\mathbb{T})}\leq\|h\|_{\dot{H}^{\alpha}(\mathbb{T})}^{\frac{1}{\alpha}}\|h\|_{L^{2}(\mathbb{T})}^{\frac{\alpha-1}{\alpha}} to obtain

hH˙α(𝕋)hH˙1(𝕋)αhL2(𝕋)(α1)c(α,c0)δα+12,\|h\|_{\dot{H}^{\alpha}(\mathbb{T})}\geq\|h\|_{\dot{H}^{1}(\mathbb{T})}^{\alpha}\|h\|_{L^{2}(\mathbb{T})}^{-(\alpha-1)}\geq c(\alpha,c_{0})\delta^{-\alpha+\frac{1}{2}},

thus we can conclude. ∎

4. Bubble and layer solutions

Previously, we have proved infinite time growth results in Theorem 1.2 and Remark 1.3 for scenarios (S2) and (S3), under some additional assumption on ρ0\rho_{0}. In this section we aim to work with less restrictive initial data – in particular, the assumption that ρ0=0\rho_{0}=0 for x1=0x_{1}=0 can now be dropped. This will enable us to obtain instability results in Section 5 for initial data close to stratified steady states. However, as the proof is done by a different approach, the set of Sobolev exponents with norm growth (as well as the growth rate in time) is not as good as Theorem 1.2 and Remark 1.3.

We first consider the initial data ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) of “bubble” type, that is, its level sets have a connected component Γ0\Gamma_{0} enclosing a simply-connected region, and |ρ0||\nabla\rho_{0}| does not vanish on Γ0\Gamma_{0} (see Figure 1 for an illustration). Intuitively, since the topological structure of all level sets is preserved under the evolution, the presence of the “bubble” prevents the solution ρ(x,t)\rho(x,t) from aligning into a perfectly stratified form where x1ρ\partial_{x_{1}}\rho may increasingly vanish. In the next result we rigorously justify this by showing that x1ρ(t)L1(𝕋2)>c>0\|\partial_{x_{1}}\rho(t)\|_{L^{1}(\mathbb{T}^{2})}>c>0 for all times, and as we will see, this leads to infinite-in-time growth in certain Sobolev norms.

Proposition 4.1.

Let Ω=𝕋2\Omega=\mathbb{T}^{2}, and assume ρ0\rho_{0} satisfies the scenario (S2). Suppose there exists a simple closed curve Γ0𝕋2\Gamma_{0}\subset\mathbb{T}^{2} enclosing a simply-connected domain D0𝕋2D_{0}\subset\mathbb{T}^{2}, and ρ0\rho_{0} satisfies ρ0|Γ0=const\rho_{0}|_{\Gamma_{0}}=\text{const} and infΓ0|ρ0|>0\inf_{\Gamma_{0}}|\nabla\rho_{0}|>0111Observe that by Sard’s theorem [16], since ρ0C2(𝕋2)\rho_{0}\in C^{2}(\mathbb{T}^{2}), the set of hh such that {ρ0(x)=h}\{\rho_{0}(x)=h\} contains a critical point has Lebesgue measure zero. . Assuming that there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}, we have

0x1ρ(,t)H˙s(𝕋2)2s𝑑tC(s,ρ0) for all s>0.\int_{0}^{\infty}\|\partial_{x_{1}}\rho(\cdot,t)\|_{\dot{H}^{s}(\mathbb{T}^{2})}^{-\frac{2}{s}}dt\leq C(s,\rho_{0})\quad\text{ for all }s>0. (4.1)

which implies

lim suptts2x1ρ(t)H˙s(𝕋2)= for all s>0.\limsup_{t\to\infty}t^{-\frac{s}{2}}\|\partial_{x_{1}}\rho(t)\|_{\dot{H}^{s}(\mathbb{T}^{2})}=\infty\quad\text{ for all }s>0. (4.2)
Proof.

Since ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) with infΓ0|ρ0|>0\inf_{\Gamma_{0}}|\nabla\rho_{0}|>0, |ρ0||\nabla\rho_{0}| is uniformly positive in some open neighborhood of Γ0\Gamma_{0}. Combining this with ρ0|Γ0=const=:c0\rho_{0}|_{\Gamma_{0}}=\text{const}=:c_{0}, for any cc\in\mathbb{R} sufficiently close to c0c_{0}, the level set {ρ0=c}\{\rho_{0}=c\} has a connected component that is a simple closed curve near Γ0\Gamma_{0}. Since Γ0\Gamma_{0} encloses a simply-connected region D0D_{0}, there exists a simple closed curve Γ1D0\Gamma_{1}\subset D_{0} such that ρ0|Γ1=c1c0\rho_{0}|_{\Gamma_{1}}=c_{1}\neq c_{0}. Denote by D1D_{1} the region enclosed by Γ1\Gamma_{1}, which is also simply-connected. See Figure 1 for an illustration of the curves Γ0,Γ1\Gamma_{0},\Gamma_{1} and the domains D0,D1D_{0},D_{1}.

Refer to caption
Figure 1. An illustration of the curves Γ0\Gamma_{0}, Γ1\Gamma_{1} and the domains D0D_{0}, D1D_{1} in the “bubble solution”.

Let us as usual define the trajectories of the flow by

dΦt(x)dt=u(Φt(x),t),Φ0(x)=x.\frac{d\Phi_{t}(x)}{dt}=u(\Phi_{t}(x),t),\,\,\,\Phi_{0}(x)=x. (4.3)

While the solution remains smooth, the flow map Φt:𝕋2𝕋2\Phi_{t}:\mathbb{T}^{2}\to\mathbb{T}^{2} is a measure-preserving smooth mapping. Thus Φt(D0)\Phi_{t}(D_{0}) and Φt(D1)\Phi_{t}(D_{1}) remain simply-connected in 𝕋2\mathbb{T}^{2}, and they satisfy Φt(D1)Φt(D0)\Phi_{t}(D_{1})\subset\Phi_{t}(D_{0}) for all t0t\geq 0. Denoting by m()m(\cdot) the Lebesgue measure of a set (which is preserved by Φt\Phi_{t}), we have m(Φt(D1))=m(D1)m(\Phi_{t}(D_{1}))=m(D_{1}) for all t0t\geq 0. In addition, since ρ\rho is advected by uu (1.1), we have as usual that ρ(Φt(x),t)=ρ0(x)\rho(\Phi_{t}(x),t)=\rho_{0}(x) for all xx and tt, thus ρ(x,t)|xΦt(Γ0)=c0\rho(x,t)|_{x\in\Phi_{t}(\Gamma_{0})}=c_{0} and ρ(x,t)|xΦt(Γ1)=c1\rho(x,t)|_{x\in\Phi_{t}(\Gamma_{1})}=c_{1} for all t0t\geq 0.

Let us denote Π2:𝕋2𝕋\Pi_{2}:\mathbb{T}^{2}\to\mathbb{T} the projection map onto the x2x_{2} variable, i.e. for any S𝕋2S\subset\mathbb{T}^{2}, Π2(S):={x2𝕋:(x1,x2)S for some x1𝕋}\Pi_{2}(S):=\{x_{2}\in\mathbb{T}:(x_{1},x_{2})\in S\text{ for some }x_{1}\in\mathbb{T}\}. Using Φt(D1)Φt(D0)\Phi_{t}(D_{1})\subset\Phi_{t}(D_{0}), we have

Π2(Φt(D1))Π2(Φt(D0)) for all t0.\Pi_{2}(\Phi_{t}(D_{1}))\subset\Pi_{2}(\Phi_{t}(D_{0}))\quad\text{ for all }t\geq 0.

Since Φt(D0)\Phi_{t}(D_{0}) and Φt(D1)\Phi_{t}(D_{1}) are simply-connected domains enclosed by boundaries Φt(Γ0)\Phi_{t}(\Gamma_{0}) and Φt(Γ1)\Phi_{t}(\Gamma_{1}) respectively, the above becomes

Π2(Φt(Γ1))=Π2(Φt(D1))Π2(Φt(D0))=Π2(Φt(Γ0)) for all t0.\Pi_{2}(\Phi_{t}(\Gamma_{1}))=\Pi_{2}(\Phi_{t}(D_{1}))\subset\Pi_{2}(\Phi_{t}(D_{0}))=\Pi_{2}(\Phi_{t}(\Gamma_{0}))\quad\text{ for all }t\geq 0. (4.4)

Using m(Φt(D1))=m(D1)m(\Phi_{t}(D_{1}))=m(D_{1}), we have Π2(Φt(D1))m(D1)2π\Pi_{2}(\Phi_{t}(D_{1}))\geq\frac{m(D_{1})}{2\pi} for all t0t\geq 0. Finally, defining I(t):=Π2(Φt(Γ1))I(t):=\Pi_{2}(\Phi_{t}(\Gamma_{1})), which is a subset in 𝕋\mathbb{T}, we have shown that |I(t)|m(D1)2π|I(t)|\geq\frac{m(D_{1})}{2\pi} and I(t)Π2(Φt(Γ0))I(t)\subset\Pi_{2}(\Phi_{t}(\Gamma_{0})) for all t0t\geq 0.

By definition of I(t)I(t) and (4.4), for any t0t\geq 0 and x2I(t)x_{2}\in I(t), 𝕋×x2\mathbb{T}\times x_{2} has a non-empty intersection with both Φt(Γ1)\Phi_{t}(\Gamma_{1}) and Φt(Γ0)\Phi_{t}(\Gamma_{0}). Since ρ(,t)|Φt(Γ0)=c0\rho(\cdot,t)|_{\Phi_{t}(\Gamma_{0})}=c_{0} and ρ(,t)|Φt(Γ1)=c1\rho(\cdot,t)|_{\Phi_{t}(\Gamma_{1})}=c_{1}, it implies

𝕋|x1ρ(x1,x2,t)|𝑑x1|c1c0| for any x2I(t),t0.\int_{\mathbb{T}}|\partial_{x_{1}}\rho(x_{1},x_{2},t)|dx_{1}\geq|c_{1}-c_{0}|\quad\text{ for any }x_{2}\in I(t),t\geq 0. (4.5)

Integrating this in x2x_{2} and using |I(t)|m(D1)2π|I(t)|\geq\frac{m(D_{1})}{2\pi}, we have 𝕋2|x1ρ(x,t)|𝑑xm(D1)|c1c0|2π\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho(x,t)|\,dx\geq\frac{m(D_{1})|c_{1}-c_{0}|}{2\pi} for all t0,t\geq 0, thus Cauchy-Schwartz yields

𝕋2|x1ρ|2𝑑x14π2(𝕋2|x1ρ|𝑑x)2=m(D1)2|c1c0|216π4>0 for all t0.\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho|^{2}\,dx\geq\frac{1}{4\pi^{2}}\left(\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho|\,dx\right)^{2}=\frac{m(D_{1})^{2}|c_{1}-c_{0}|^{2}}{16\pi^{4}}>0\quad\text{ for all }t\geq 0. (4.6)

Applying the interpolation inequalityfL2(𝕋2)fH˙1(𝕋2)ss+1fH˙s(𝕋2)1s+1\|f\|_{L^{2}(\mathbb{T}^{2})}\leq\|f\|_{\dot{H}^{-1}(\mathbb{T}^{2})}^{\frac{s}{s+1}}\|f\|_{\dot{H}^{s}(\mathbb{T}^{2})}^{\frac{1}{s+1}} for s>0s>0 with f=x1ρf=\partial_{x_{1}}\rho, we have

δ(t)=x1ρH˙1(𝕋2)2x1ρL2(𝕋2)2+2sx1ρH˙s(𝕋2)2s for all s>0,t0.\delta(t)=\|\partial_{x_{1}}\rho\|_{\dot{H}^{-1}(\mathbb{T}^{2})}^{2}\geq\|\partial_{x_{1}}\rho\|_{L^{2}(\mathbb{T}^{2})}^{2+\frac{2}{s}}\|\partial_{x_{1}}\rho\|_{\dot{H}^{s}(\mathbb{T}^{2})}^{-\frac{2}{s}}\quad\text{ for all }s>0,t\geq 0. (4.7)

Plugging (4.7), (4.6) into (3.3) we obtain (4.1). Finally, combining (4.1) with the fact that 1t1𝑑t=\int_{1}^{\infty}t^{-1}dt=\infty gives (4.2) as a direct consequence. ∎

The growth for “bubble” solutions can be easily adapted to the bounded strip case as follows.

Corollary 4.2.

Let Ω=S=:𝕋×[π,π]\Omega=S=:\mathbb{T}\times[-\pi,\pi], and assume ρ0\rho_{0} satisfies scenario (S3). Suppose there exists a simple closed curve Γ0S\Gamma_{0}\subset S^{\circ} enclosing a simply-connected domain D0SD_{0}\subset S, and ρ0\rho_{0} satisfies ρ0|Γ0=const\rho_{0}|_{\Gamma_{0}}=\text{const} and infΓ0|ρ0|>0\inf_{\Gamma_{0}}|\nabla\rho_{0}|>0. Assuming that there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}, we have

0x1ρ(,t)H˙s(S)2s𝑑tC(s,ρ0) for all s>0.\int_{0}^{\infty}\|\partial_{x_{1}}\rho(\cdot,t)\|_{\dot{H}^{s}(S)}^{-\frac{2}{s}}dt\leq C(s,\rho_{0})\quad\text{ for all }s>0. (4.8)

which implies

lim suptts2x1ρ(t)H˙s(S)= for all s>0.\limsup_{t\to\infty}t^{-\frac{s}{2}}\|\partial_{x_{1}}\rho(t)\|_{\dot{H}^{s}(S)}=\infty\quad\text{ for all }s>0. (4.9)
Proof.

The proof is almost identical to the proof of Proposition 4.1. Again, there exists Γ1\Gamma_{1} enclosing a simply-connected domain D1D0D_{1}\subset D_{0}, such that ρ0|Γ1=c1\rho_{0}|_{\Gamma_{1}}=c_{1}, and c1c0:=ρ0|Γ0c_{1}\neq c_{0}:=\rho_{0}|_{\Gamma_{0}}. Defining I(t):=Π2(Φt(Γ1))I(t):=\Pi_{2}(\Phi_{t}(\Gamma_{1})) (which is now a subset in [π,π][-\pi,\pi]), the same argument gives that |I(t)|m(D1)2π|I(t)|\geq\frac{m(D_{1})}{2\pi} and (4.5). Thus (4.6) still holds (except that the integral now takes place in SS instead of 𝕋2\mathbb{T}^{2}), and the rest of the proof remains unchanged. Note that the interpolation inequality fL2(S)fH˙1(S)ss+1fH˙s(S)1s+1\|f\|_{L^{2}(S)}\leq\|f\|_{\dot{H}^{-1}(S)}^{\frac{s}{s+1}}\|f\|_{\dot{H}^{s}(S)}^{\frac{1}{s+1}} holds in SS as well by a straightforward argument using the eigenfunction expansion similar to the standard Fourier argument in 𝕋2.\mathbb{T}^{2}.

Our next result concerns “layered” initial data, which we define below.

Definition 4.3.

For ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}), we say it has a layered structure if there exists a measure-preserving smooth diffeomorphism ϕ:𝕋2𝕋2\phi:\mathbb{T}^{2}\to\mathbb{T}^{2} that satisfies ϕ(𝕋×{π})=𝕋×{π}\phi(\mathbb{T}\times\{\pi\})=\mathbb{T}\times\{\pi\}, such that ρs=ρ0(ϕ1(x))\rho_{s}=\rho_{0}(\phi^{-1}(x)) is a stratified solution, i.e. ρs(x)\rho_{s}(x) only depends on x2x_{2}. In this case, we call ρs\rho_{s} the stratified state corresponding to ρ0\rho_{0}.

Note that any layered initial data ρ0\rho_{0} has a unique corresponding stratified state ρs\rho_{s}. (Even though the mapping ϕ\phi is not unique, e.g. one can shift ϕ\phi by any (a,0)(a,0)). To see this, take any curve Γ\Gamma such that ρ0|Γ=c\rho_{0}|_{\Gamma}=c with infΓ|ρ0|>0\inf_{\Gamma}|\nabla\rho_{0}|>0, and denote by DD the region bounded between Γ\Gamma and 𝕋×{π}\mathbb{T}\times\{\pi\}. Since ϕ\phi is measure-preserving and ϕ(𝕋×{π})=𝕋×{π}\phi(\mathbb{T}\times\{\pi\})=\mathbb{T}\times\{\pi\}, we know ϕ(D)=𝕋×[x2,π]\phi(D)=\mathbb{T}\times[x_{2},\pi] must have the same area as DD, leading to ρs(π|D|2π)=c\rho_{s}(\pi-\frac{|D|}{2\pi})=c. Since ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) (thus ρs\rho_{s} is also smooth), Sard’s theorem allows us to run this argument for a.e. cc, which defines ρs\rho_{s} uniquely for all xx. See Figure 2 for an illustration of a layered initial data ρ0\rho_{0} and its corresponding stratified state ρs\rho_{s}.

Refer to caption
Figure 2. An illustration of a “layered” initial data ρ0\rho_{0} and its corresponding stratified state ρs\rho_{s}.

Clearly, Theorem 1.2 cannot be applied to any layered ρ0\rho_{0} since ρ0(0,x2)0\rho_{0}(0,x_{2})\not\equiv 0, and Proposition 4.1 fails too since there is no level set Γ\Gamma enclosing a simply-connected region. Despite these difficulties, we will show that small scale formation can still happen to ρ0\rho_{0}, as long as its potential energy is strictly lower than that of ρs\rho_{s}.

Proposition 4.4.

Let Ω=𝕋2\Omega=\mathbb{T}^{2}. Assume ρ0\rho_{0} satisfies scenario (S2), and it has a layered structure in the sense of Definition 4.3, with corresponding stratified state denoted by ρs\rho_{s}. In addition, suppose

E(0)=𝕋2ρ0(x)x2dx<𝕋2ρs(x)x2dx=:Es.E(0)=\int_{\mathbb{T}^{2}}\rho_{0}(x)x_{2}dx<\int_{\mathbb{T}^{2}}\rho_{s}(x)x_{2}dx=:E_{s}. (4.10)

Then the estimates (4.1) and (4.2) hold, given there is a global-in-time smooth solution ρ(x,t)\rho(x,t) to (1.1) with initial data ρ0\rho_{0}.

Remark 4.5.

As a side note, it is not hard to construct layered initial data ρ0\rho_{0} satisfying (4.10) – see Figure 3 for an illustration.

Refer to caption
Figure 3. An example of a “layered” ρ0\rho_{0} satisfying the inequality (4.10). Let ρ0\rho_{0} be odd in x2x_{2}, and set ρ0=1D\rho_{0}=1_{D} in the upper half of 𝕋2\mathbb{T}^{2}, where DD is bounded between x2=45πx_{2}=\frac{4}{5}\pi and x2=π2π4cos(x1)x_{2}=\frac{\pi}{2}-\frac{\pi}{4}\cos(x_{1}). The right figure shows its corresponding stratified state ρs\rho_{s}. Such (discontinuous) ρ0\rho_{0} has a potential energy strictly less than that of ρs\rho_{s}, since the center of mass of DD is lower than ϕ(D)\phi(D). One can then slightly mollify ρ0\rho_{0} to obtain a smooth layered initial data satisfying (4.10).
Proof.

To begin with, we will show that for any t0t\geq 0, ρ(,t)\rho(\cdot,t) also has a layered structure with corresponding stratified state being ρs\rho_{s}. The assumption on ρ0\rho_{0} gives ρsϕ=ρ0\rho_{s}\circ\phi=\rho_{0} for some measure-preserving diffeomorphism ϕ\phi. Combining this with ρ(Φt(x),t)=ρ0(x)\rho(\Phi_{t}(x),t)=\rho_{0}(x) (where Φt(x)\Phi_{t}(x) is the flow trajectory given by (4.3)), we have ρs=ρ((Φtϕ1)(x),t)\rho_{s}=\rho((\Phi_{t}\circ\phi^{-1})(x),t) for all times. Here Φtϕ1:𝕋2𝕋2\Phi_{t}\circ\phi^{-1}:\mathbb{T}^{2}\to\mathbb{T}^{2} is a measure-preserving diffeomorphism, and it keeps the set 𝕋×{π}\mathbb{T}\times\{\pi\} invariant, since both ϕ\phi and Φt\Phi_{t} have this property: ϕ\phi has this property due to Definition 4.3, whereas Φt\Phi_{t} has this property since u2=0u_{2}=0 on x2=πx_{2}=\pi for all times.

Let us denote b:=EsE(0)>0,b:=E_{s}-E(0)>0, where the strict positivity is due to (4.10). By Lemma 3.1, E(t)E(t) is non-increasing in time, thus

EsE(t)EsE(0)=b>0 for all t0.E_{s}-E(t)\geq E_{s}-E(0)=b>0\quad\text{ for all }t\geq 0. (4.11)

Since ρs\rho_{s} is the only stratified state that is topologically reachable from ρ(,t)\rho(\cdot,t) (among all measure-preserving diffeomorphisms that keeps 𝕋×{π}\mathbb{T}\times\{\pi\} invariant), the fact that ρ(,t)\rho(\cdot,t) has a potential energy strictly less than ρs\rho_{s} (with the gap being at least bb) intuitively suggests that ρ(,t)\rho(\cdot,t) cannot have all level sets very close to horizontal. Below we will show that this is indeed true, in the sense that 𝕋2|x1ρ(x,t)|𝑑x\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho(x,t)|dx is bounded below by a positive constant for all times.

By (4.11) and the definition of potential energy E(t)E(t), we have

bEsE(t)=𝕋2x2(ρs(x)ρ(x,t))𝑑xπ𝕋2|ρs(x)ρ(x,t)|𝑑x,b\leq E_{s}-E(t)=\int_{\mathbb{T}^{2}}x_{2}(\rho_{s}(x)-\rho(x,t))dx\leq\pi\int_{\mathbb{T}^{2}}|\rho_{s}(x)-\rho(x,t)|dx, (4.12)

and let us take a closer look at the integrand. In the first paragraph of the proof we showed ρs(x)=ρ(Ψt(x),t)\rho_{s}(x)=\rho(\Psi_{t}(x),t), where Ψt:=Φtϕ1\Psi_{t}:=\Phi_{t}\circ\phi^{-1} is a measure-preserving diffeomorphism that keeps 𝕋×{π}\mathbb{T}\times\{\pi\} invariant. As a result, for any t0t\geq 0 and x2𝕋x_{2}\in\mathbb{T}, Ψt(𝕋×{x2})\Psi_{t}(\mathbb{T}\times\{x_{2}\}) must have a non-empty intersection with 𝕋×{x2}\mathbb{T}\times\{x_{2}\}, i.e. there exists x~1\tilde{x}_{1} and x¯1\bar{x}_{1} depending on x2x_{2} and tt, such that Ψt(x~1,x2)=(x¯1,x2)\Psi_{t}(\tilde{x}_{1},x_{2})=(\bar{x}_{1},x_{2}). Combining this with the fact that ρs\rho_{s} is a function of x2x_{2} only, we have

|ρs(x)ρ(x,t)|=|ρs(x~1,x2)ρ(x,t)|=|ρ(x¯1,x2,t)ρ(x1,x2,t)|𝕋|x1ρ(s1,x2,t)|𝑑s1|\rho_{s}(x)-\rho(x,t)|=|\rho_{s}(\tilde{x}_{1},x_{2})-\rho(x,t)|=|\rho(\bar{x}_{1},x_{2},t)-\rho(x_{1},x_{2},t)|\leq\int_{\mathbb{T}}|\partial_{x_{1}}\rho(s_{1},x_{2},t)|ds_{1}

for any x=(x1,x2)𝕋2,t0x=(x_{1},x_{2})\in\mathbb{T}^{2},t\geq 0. Plugging this into (4.12) gives

b2π2𝕋2|x1ρ(x,t)|𝑑x,b\leq 2\pi^{2}\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho(x,t)|dx,

leading to 𝕋2|x1ρ(x,t)|𝑑xb2π2>0\int_{\mathbb{T}^{2}}|\partial_{x_{1}}\rho(x,t)|dx\geq\frac{b}{2\pi^{2}}>0 for all t0t\geq 0. Now that we have a positive lower bound on x1ρ(t)L1(𝕋2)\|\partial_{x_{1}}\rho(t)\|_{L^{1}(\mathbb{T}^{2})}, the rest of the argument can proceed the same way as in (4.6) and (4.7) in the proof of Proposition 4.1, allowing us to obtain the same estimates (4.1)–(4.2). ∎

5. Instability of horizontally stratified steady states

In this section we aim to prove the two nonlinear instability results Theorems 1.4 and 1.5 in 𝕋2\mathbb{T}^{2} and SS respectively. We start with Theorem 1.4, which shows that any stratified steady state ρs\rho_{s} in 𝕋2\mathbb{T}^{2} that is odd in x2x_{2} is nonlinearly unstable in an arbitrarily high Sobolev space. The idea is to locate a point x0𝕋2x_{0}\in\mathbb{T}^{2} where locally ρs\rho_{s} has heavier density on top of lighter one, then use a circular flow to slightly perturb ρs\rho_{s} near x0x_{0} to construct a “layered” initial data that satisfies the assumption of Proposition 4.4.

Proof of Theorem 1.4.

We claim that for any ϵ>0\epsilon>0 and k>0k>0, we can construct a ρ0C(𝕋2)\rho_{0}\in C^{\infty}(\mathbb{T}^{2}) satisfying all the following:

  1. (a)

    ρ0\rho_{0} is odd in x2x_{2}, and has a layered structure in the sense of Definition 4.3 with corresponding stratified state ρs\rho_{s}.

  2. (b)

    ρ0ρsHk(𝕋2)<ϵ\|\rho_{0}-\rho_{s}\|_{H^{k}(\mathbb{T}^{2})}<\epsilon.

  3. (c)

    E(0)<𝕋2x2ρsdx=:EsE(0)<\int_{\mathbb{T}^{2}}x_{2}\rho_{s}dx=:E_{s}.

Once these are shown to be true, a direct application of Proposition 4.4 immediately yields the infinite-in-time growth results (4.1) and (4.2). Since x1ρ(,t)=x1(ρ(,t)ρs)\partial_{x_{1}}\rho(\cdot,t)=\partial_{x_{1}}(\rho(\cdot,t)-\rho_{s}), (4.2) directly implies (1.7), finishing the proof.

In the rest of the proof we aim to construct ρ0\rho_{0} and prove the claim. We will focus on the construction of ρ0\rho_{0} in the upper half of torus 𝕋+2:=𝕋×[0,π]\mathbb{T}^{2}_{+}:=\mathbb{T}\times[0,\pi], and at the end we will extend it to the lower part 𝕋2\mathbb{T}^{2}_{-} by an odd extension.

Recall that ρs(x)=g(x2)\rho_{s}(x)=g(x_{2}) is a smooth stratified state that is odd in x2x_{2}. Thus gg is odd and smooth in 𝕋\mathbb{T}. Such gg cannot be monotone, so there exists some h0(0,π)h_{0}\in(0,\pi) such that g(h0)>0g^{\prime}(h_{0})>0. For 0<ϵ010<\epsilon_{0}\ll 1 to be fixed later, let φϵ0Cc()\varphi_{\epsilon_{0}}\in C^{\infty}_{c}(\mathbb{R}) be non-negative and supported on [ϵ0,2ϵ0][\epsilon_{0},2\epsilon_{0}]. Let v:𝕋+22v:\mathbb{T}^{2}_{+}\to\mathbb{R}^{2} be the velocity field of an incompressible circular flow around x0:=(0,h0)x_{0}:=(0,h_{0}), given by

v(x)=(xx0)φϵ0(|xx0|) for x𝕋+2.v(x)=(x-x_{0})^{\perp}\varphi_{\epsilon_{0}}(|x-x_{0}|)\quad\text{ for }x\in\mathbb{T}^{2}_{+}. (5.1)

For any τ0\tau\geq 0, let ρ~(,τ)\tilde{\rho}(\cdot,\tau) be the solution to

τρ~+vρ~=0 in 𝕋+2×(0,)\partial_{\tau}\tilde{\rho}+v\cdot\nabla\tilde{\rho}=0\quad\text{ in }\mathbb{T}^{2}_{+}\times(0,\infty) (5.2)

with initial data ρ~(,0)=ρs\tilde{\rho}(\cdot,0)=\rho_{s}. Since vv is supported in a small annulus B(x0,2ϵ0)B(x0,ϵ0)B(x_{0},2\epsilon_{0})\setminus B(x_{0},\epsilon_{0}), clearly ρ~(,τ)=ρs\tilde{\rho}(\cdot,\tau)=\rho_{s} outside the annulus. Intuitively, since ρs\rho_{s} has heavier density on top of lighter density locally near x0x_{0}, we formally expect that ρ~(τ)\tilde{\rho}(\tau) should have lower potential energy than ρs\rho_{s} for a short time. (Here the “time” τ\tau is the perturbation parameter, and has nothing to do with the actual time in (1.1)). Below we will rigorously show

F(τ):=𝕋+2(ρ~(x,τ)ρs)x2𝑑x<0 for all 0<ϵ01 and 0<τ1.F(\tau):=\int_{\mathbb{T}^{2}_{+}}(\tilde{\rho}(x,\tau)-\rho_{s})x_{2}dx<0\quad\text{ for all }0<\epsilon_{0}\ll 1\text{ and }0<\tau\ll 1. (5.3)

Since the integral can be reduced to the set B(x0,2ϵ0)B(x0,ϵ0)B(x_{0},2\epsilon_{0})\setminus B(x_{0},\epsilon_{0}), it is convenient to write it in polar coordinates centered at the point x0x_{0}. Using the change of variables x1=rcosθ,x2=h0+rsinθx_{1}=r\cos\theta,x_{2}=h_{0}+r\sin\theta, we have

F(τ)\displaystyle F(\tau) =\displaystyle= ϵ02ϵ002πρ~(rcosθ,h0+rsinθ,τ)(h0+rsinθ)r𝑑θ𝑑rB(x0,2ϵ)B(x0,ϵ)ρsx2𝑑x=:Cs\displaystyle\displaystyle\int_{\epsilon_{0}}^{2\epsilon_{0}}\int_{0}^{2\pi}\tilde{\rho}(r\cos\theta,h_{0}+r\sin\theta,\tau)(h_{0}+r\sin\theta)rd\theta dr-\underbrace{\int_{B(x_{0},2\epsilon)\setminus B(x_{0},\epsilon)}\rho_{s}x_{2}dx}_{=:C_{s}} (5.4)
=\displaystyle= ϵ02ϵ002πρs(rcos(θφϵ0(r)τ),h0+rsin(θφϵ0(r)τ))(h0+rsinθ)r𝑑θ𝑑rCs\displaystyle\displaystyle\int_{\epsilon_{0}}^{2\epsilon_{0}}\int_{0}^{2\pi}\rho_{s}(r\cos(\theta-\varphi_{\epsilon_{0}}(r)\tau),h_{0}+r\sin(\theta-\varphi_{\epsilon_{0}}(r)\tau))(h_{0}+r\sin\theta)rd\theta dr-C_{s}
=\displaystyle= ϵ02ϵ002πg(h0+rsin(θφϵ0(r)τ))(h0+rsinθ)r𝑑θ𝑑rCs\displaystyle\displaystyle\int_{\epsilon_{0}}^{2\epsilon_{0}}\int_{0}^{2\pi}g(h_{0}+r\sin(\theta-\varphi_{\epsilon_{0}}(r)\tau))(h_{0}+r\sin\theta)rd\theta dr-C_{s}
=:\displaystyle=: ϵ02ϵ0f(r,τ)𝑑rCs,\displaystyle\displaystyle\int_{\epsilon_{0}}^{2\epsilon_{0}}f(r,\tau)dr-C_{s},

where the second identity follows from the facts that ρ~(,τ)\tilde{\rho}(\cdot,\tau) is transported by vv with initial data ρs\rho_{s}, and vv is a circular flow with angular velocity φϵ0(r)\varphi_{\epsilon_{0}}(r) along B(x0,r)\partial B(x_{0},r). We can rewrite f(r,τ)f(r,\tau) as

f(r,τ)=r202πg(h0+rsin(θφϵ0(r)τ))sinθdθ+h0r02πg(h0+rsin(θφϵ0(r)τ))𝑑θ,\begin{split}f(r,\tau)=&r^{2}\int_{0}^{2\pi}g(h_{0}+r\sin(\theta-\varphi_{\epsilon_{0}}(r)\tau))\sin\theta d\theta+h_{0}r\int_{0}^{2\pi}g(h_{0}+r\sin(\theta-\varphi_{\epsilon_{0}}(r)\tau))d\theta,\end{split}

where the second integral is constant in τ\tau using the substitution ϑ=θφϵ0(r)τ\vartheta=\theta-\varphi_{\epsilon_{0}}(r)\tau. Thus taking the τ\tau derivative gives

ddτf(r,τ)=r3φϵ0(r)02πg(h0+rsin(θφϵ0(r)τ))cos(θφϵ0(r)τ)sinθdθ,\frac{d}{d\tau}f(r,\tau)=-r^{3}\varphi_{\epsilon_{0}}(r)\int_{0}^{2\pi}g^{\prime}(h_{0}+r\sin(\theta-\varphi_{\epsilon_{0}}(r)\tau))\cos(\theta-\varphi_{\epsilon_{0}}(r)\tau)\sin\theta\,d\theta,

leading to

ddτf(r,τ)|τ=0=r3φϵ0(r)02πg(h0+rsinθ)cosθsinθdθ=0,\frac{d}{d\tau}f(r,\tau)\Big{|}_{\tau=0}=-r^{3}\varphi_{\epsilon_{0}}(r)\int_{0}^{2\pi}g^{\prime}(h_{0}+r\sin\theta)\cos\theta\sin\theta\,d\theta=0, (5.5)

since the integrand is odd about θ=π2\theta=\frac{\pi}{2}. Taking one more derivative and setting τ=0\tau=0, we have

d2dτ2f(r,τ)|τ=0=r4φϵ02(r)02πg′′(h0+rsinθ)(cosθ)2sinθdθr3φϵ02(r)02πg(h0+rsinθ)(sinθ)2𝑑θ=φϵ02(r)(πr3g(h0)+O(r4)).\begin{split}\frac{d^{2}}{d\tau^{2}}f(r,\tau)\Big{|}_{\tau=0}&=r^{4}\varphi_{\epsilon_{0}}^{2}(r)\int_{0}^{2\pi}g^{\prime\prime}(h_{0}+r\sin\theta)(\cos\theta)^{2}\sin\theta\,d\theta\\ &\quad-r^{3}\varphi_{\epsilon_{0}}^{2}(r)\int_{0}^{2\pi}g^{\prime}(h_{0}+r\sin\theta)(\sin\theta)^{2}d\theta\\ &=\varphi_{\epsilon_{0}}^{2}(r)\left(-\pi r^{3}g^{\prime}(h_{0})+O(r^{4})\right).\end{split}

Since h0h_{0} is chosen such that g(h0)>0g^{\prime}(h_{0})>0, for all sufficiently small 0<ϵ010<\epsilon_{0}\ll 1 we have

d2dτ2f(r,τ)|τ=012πr3φϵ02(r)g(h0)<0 for all r(ϵ0,2ϵ0).\frac{d^{2}}{d\tau^{2}}f(r,\tau)\Big{|}_{\tau=0}\leq-\frac{1}{2}\pi r^{3}\varphi_{\epsilon_{0}}^{2}(r)g^{\prime}(h_{0})<0\quad\text{ for all }r\in(\epsilon_{0},2\epsilon_{0}).

Plugging (5.5) and the above into (5.4) gives that ddτF(τ)|τ=0=0\frac{d}{d\tau}F(\tau)\big{|}_{\tau=0}=0 and d2dτ2F(τ)|τ=0c(ϵ0)g(h0)<0\frac{d^{2}}{d\tau^{2}}F(\tau)\big{|}_{\tau=0}\leq-c(\epsilon_{0})g^{\prime}(h_{0})<0. Combining these with F(0)=0F(0)=0 gives (5.3).

Finally, we use odd reflection to extend ρ~(,τ)\tilde{\rho}(\cdot,\tau) to 𝕋2\mathbb{T}^{2}_{-}, which is equivalent with simutaneously applying a circular flow to ρs\rho_{s} near (0,h0)(0,-h_{0}) in the opposite direction as v|𝕋+2v|_{\mathbb{T}^{2}_{+}}. We then set ρ0:=ρ~(τ)\rho_{0}:=\tilde{\rho}(\tau) with 0<τ10<\tau\ll 1 sufficiently small, and let us check that it satisfies the claim (a,b,c): (a) is a direct consequence from the definition, since ρ0\rho_{0} can be reached from ρs\rho_{s} by an explicit measure-preserving smooth flow that is only non-zero near (0,±h0)(0,\pm h_{0}). Also, since ρ~(,τ)\tilde{\rho}(\cdot,\tau) is transported from ρs\rho_{s} with a smooth velocity field vv, for any k>0k>0, we have ρ~(τ)ρsHk0\|\tilde{\rho}(\tau)-\rho_{s}\|_{H^{k}}\to 0 as τ0+\tau\to 0^{+}, thus property (b) is satisfied. As for the potential energy, note that (5.3) gives that E(0)Es=2F(τ)<0E(0)-E_{s}=2F(\tau)<0 when 0<τ10<\tau\ll 1 is sufficiently small, finishing the proof of (c). ∎

Finally, we are ready to prove Theorem 1.5 which deals with the instability on the strip. The idea is to perturb the steady state to make a small “bubble” localized near one point, then apply Corollary 4.2.

Proof of Theorem 1.5.

First note that any stationary solution ρsC(S)\rho_{s}\in C^{\infty}(S) must be stratified of the form ρs=g(x2)\rho_{s}=g(x_{2}), since only in this case it satisfies x1ρsH˙1(Ω)=0\|\partial_{x_{1}}\rho_{s}\|_{\dot{H}^{-1}(\Omega)}=0 by Lemma 3.1.

Let φCc(2)\varphi\in C_{c}^{\infty}(\mathbb{R}^{2}) be a nonnegative function supported in B(0,1)B(0,1) with φ(0)=1\varphi(0)=1. For 0<λ<10<\lambda<1, let

ρ0λ(x):=ρs(x)+2Aλφ(λ1x) for xS,\rho_{0\lambda}(x):=\rho_{s}(x)+2A\lambda\varphi(\lambda^{-1}x)\quad\text{ for }x\in S,

where A:=ρsL(S)A:=\|\nabla\rho_{s}\|_{L^{\infty}(S)}. Clearly, ρ0λC(S)\rho_{0\lambda}\in C^{\infty}(S), and ρ0λ=ρs\rho_{0\lambda}=\rho_{s} in SB(0,λ)S\setminus B(0,\lambda).

Let us first check that (1.8) is satisfied for ρ0:=ρ0λ\rho_{0}:=\rho_{0\lambda} with 0<λ10<\lambda\ll 1. A simple scaling argument yields that D2(ρ0λρs)L2(S)=2AD2φL2(2)\|D^{2}(\rho_{0\lambda}-\rho_{s})\|_{L^{2}(S)}=2A\|D^{2}\varphi\|_{L^{2}(\mathbb{R}^{2})} is invariant in λ\lambda (where D2D^{2} is any partial derivative of order 2), thus ρ0λρsH2(S)\|\rho_{0\lambda}-\rho_{s}\|_{H^{2}(S)} is uniformly bounded for all 0<λ<10<\lambda<1. Combining this with ρ0λρsL2(S)CAλ2\|\rho_{0\lambda}-\rho_{s}\|_{L^{2}(S)}\leq CA\lambda^{2}, we have ρ0λρsH2γ(S)CAλγ\|\rho_{0\lambda}-\rho_{s}\|_{H^{2-\gamma}(S)}\leq CA\lambda^{\gamma} for all γ>0\gamma>0 (where CC only depends on φ\varphi), where the right hand side can be made arbitrarily small for 0<λ10<\lambda\ll 1.

We claim that for any 0<λ<10<\lambda<1, ρ0λ\rho_{0\lambda} satisfies the assumption of a “bubble solution” in Corollary 4.2. To see this, note that the definitions of AA and ρ0λ\rho_{0\lambda} yields

ρ0λ(x)=ρs(x)ρs(0)+Aλ for any xB(0,λ),\rho_{0\lambda}(x)=\rho_{s}(x)\leq\rho_{s}(0)+A\lambda\quad\text{ for any }x\in\partial B(0,\lambda),

whereas

ρ0λ(0)=ρs(0)+2Aλ.\rho_{0\lambda}(0)=\rho_{s}(0)+2A\lambda.

Applying Sard’s theorem [16] to ρ0λ\rho_{0\lambda}, for almost every h(ρs(0)+Aλ,ρs(0)+2Aλ)h\in(\rho_{s}(0)+A\lambda,\rho_{s}(0)+2A\lambda), we know {ρ0λ=h}\{\rho_{0\lambda}=h\} has a connected component in B(0,λ)B(0,\lambda) on which |ρ0λ||\nabla\rho_{0\lambda}| never vanishes. Naming any such connected component Γ0\Gamma_{0}, we then have that ρ0λ\rho_{0\lambda} satisfies the assumption in Corollary 4.2. As a result we have the estimate (4.9). Using that x1ρ(,t)=x1(ρ(,t)ρs)\partial_{x_{1}}\rho(\cdot,t)=\partial_{x_{1}}(\rho(\cdot,t)-\rho_{s}), (4.9) directly implies (1.9), thus finishes the proof. ∎

Remark 5.1.

For a stratified solution ρs=g(x2)\rho_{s}=g(x_{2}) that does not satisfy g0g^{\prime}\leq 0, the perturbation can be made small in higher Sobolev spaces. Namely, if there exists x0Sx_{0}\in S such that x2ρs(x0)>0\partial_{x_{2}}\rho_{s}(x_{0})>0, one can proceed as in the proof of Proposition 4.4 to construct a “layered” initial data close to ρs\rho_{s} in HkH^{k} norm for arbitrarily large k>0k>0.

Acknowledgement. The authors acknowledge partial support of the NSF-DMS grants 1715418, 1846745 and 2006372. AK has been partially supported by Simons Foundation. YY has been partially supported by the Sloan Research Fellowship. This paper has been initiated at the AIM Square, and the authors thank AIM for support and collaborative opportunity.

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