Abstract
Kuramoto–Velarde equation describes the spatiotemporal evolution of the morphology of steps on crystal surfaces, or the evolution of the spinoidal decomposition of phase separating systems in an external field. We prove the well-posedness of the classical solutions for the Cauchy problem, associated with this equation for each choice of the terminal time T.
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1 Introduction
In this paper, we investigate the well-posedness of the following Cauchy problem:
with
On the flux f), we assume
for some positive constant \(C_0\).
On the initial datum, we assume
Taking
Equation (1.1) reads
It is known as the Kuramoto–Velarde equation and it describes slow space-time variations of disturbances at interfaces, diffusion–reaction fronts and plasma instability fronts [26, 30, 31]. It also describes Benard–Marangoni cells that occur when there is large surface tension on the interface [38, 67, 71] in a microgravity environment. This situation arises in crystal growth experiments aboard an orbiting space station, although the free interface is metastable with respect to small perturbations. The nonlinearities \(\kappa u\partial _{x}^2u\) and \(\delta (\partial _x u)^2\) model pressure destabilization effects striving to rupture the interface. (1.6) is deduced in [66] to describe the long waves on a viscous fluid owing down an inclined plane, and in [25] to model the drift waves in a plasma.
From a mathematical point of view, in [40], the exact solutions for (1.6) are studied, while, in [60], the initial boundary problem is analyzed. In [7, 8], the authors prove the existence of the solitons for (1.6). Instead, in [56], the existence of traveling wave solutions for (1.6) is studied. In [41], the author analyzes the existence of the periodic solution for (1.6), under appropriate assumptions on \(b_1,\,\gamma ,\,\alpha ,\,\kappa ,\,\delta \) and \(\beta \). The well-posedness of the Cauchy problem for (1.6) is proven in [59], using the energy space technique and taking \(b_1=0\). In [15], under assumption
and \(\delta =2\kappa \), through a priori estimates together with an application of the Cauchy–Kovalevskaya Theorem, the well-posedness of the classical solutions of (1.6) is proven. In [11], under Assumption (1.7) and \(\delta \ne 2\kappa \), the well-posedness of classical solutions is proven, under appropriate assumptions on \(\beta \), T and \(H^1\)-norm of the initial datum. Finally, in [16], the well-posedness of classical solutions is proven, under Assumption (1.7) and under appropriate assumptions on \(\beta \), T and \(L^2\)-norm of the initial datum.
Taking \(\kappa =\delta =0\) in (1.6), we have
It was also independently deduced by Kuramoto [45,46,47] to describe the phase turbulence in reaction–diffusion systems, and by Sivashinsky [64], to describe plane flame propagation, taking into account the combined influence of diffusion and thermal conduction of the gas on the stability of a plane flame front.
Equation (1.8) can be used to study incipient instabilities in several physical and chemical systems [5, 37, 48]. Moreover, (1.8), which is also known as the Benney–Lin equation [3, 52], was derived by Kuramoto in the study of phase turbulence in Belousov–Zhabotinsky reactions [51].
From a mathematical point of view, the dynamical properties and the existence of exact solutions for (1.8) have been investigated in [29, 42, 44, 57, 58, 69]. The control problem for (1.8) are studied in [1, 4, 32]. In [6], the problem of global exponential stabilization of (1.8) with periodic boundary conditions is analyzed. In [39], it is proposed a generalization of optimal control theory for (1.8), while, in [55], the problem of global boundary control of (1.8) is considered. In [61], the existence of solitonic solutions for (1.8) is proven. In [2, 15, 17, 18, 65], the well-posedness of the Cauchy problem for (1.8) is proven, using the energy space technique, the fixed point method, a priori estimates together with an application of the Cauchy–Kovalevskaya Theorem and a priori estimates together with an application of the Aubin–Lions Lemma, respectively. Instead, in [19, 53, 54], the initial-boundary value problem for (1.8) is studied, using a priori estimates together with an application of the Cauchy–Kovalevskaya Theorem, and the energy space technique, respectively. Finally, following [20, 49, 62], in [21], the convergence of the solution of (1.8) to to the unique entropy one of the Burgers equation is proven.
Taking
(1.1) reads
It models the spinodal decomposition of phase separating systems in an external field [28, 50, 70], the spatiotemporal evolution of the morphology of steps on crystal surfaces [33, 43, 61] and the growth of thermodynamically unstable crystal surfaces with strongly anisotropic surface tension [34,35,36]. In the case of a growing crystal surface with strongly anisotropic surface tension, the function u represents the surface slope, while the constants \(b_1\) and \(b_1\) are the growth driving forces proportional to the difference between the bulk chemical potentials of the solid and fluid phases. Equation (1.10) is also deduced by Watson [68] as a small-slope approximation of the crystal growth model obtained in [27].
Here we complete the results of [11, 16]. Here we assume (1.4) on the initial condition and our arguments are based on the Aubin-Lions Lemma [13, 14, 23, 24, 63].
The main result of this paper is the following theorem.
Theorem 1.1
Assume (1.2), (1.3) and (1.4). Fixed \(\gamma ,\,\alpha ,\,\kappa ,\,\delta ,\,T\), there exists a unique solution u of (1.1), such that
Moreover, if \(u_1\) and \(u_2\) are two solutions of (1.1) corresponding to the initial data \(u_{1,0}\) and \(u_{2,0}\), we have that
for some suitable \(C(T)>0\), and every, \(0\le t\le T\).
The paper is organized as follows. In Sect. 2, we prove several a priori estimates on a vanishing viscosity approximation of (1.1). Those play a key role in the proof of our main result, that is given in Sect. 3.
2 Vanishing Viscosity Approximation
Our existence argument is based on passing to the limit in a vanishing viscosity approximation of (1.1).
Fix a small number \(0<\varepsilon <1\) and let \(u_\varepsilon =u_\varepsilon (t,x)\) be the unique classical solution of the following problem [9,10,11]:
where \(u_{\varepsilon ,0}\) is a \(C^{\infty }\) approximation of \(u_0\), such that
where \(C_0\) is a positive constant, independent on \(\varepsilon \).
Let us prove some a priori estimates on \(u_\varepsilon \). We denote by \(C_0\) the constants which depend only on the initial data, and by C(T), the constants which depend also on T.
Following [11, Lemma 2.1] and [22, Lemma 2.2] , we prove the following result.
Lemma 2.1
Fix \(\gamma ,\,\alpha ,\,\kappa ,\,\delta ,\,T\). There exists a constant \(C(T)>0\), independent of \(\varepsilon \), such that
for every \(0\le t\le T\).
Proof
We begin by proving that
for every \(0\le t\le T\), where A is a arbitrary positive constant, and
Consider A a positive constant. Multiplying (2.1) by \(2u_\varepsilon -2A\partial _{x}^2u_\varepsilon \), an integration on \(\mathbb {R}\) gives
Consequently, we have that
Observe that
Moreover,
It follows from (2.10), (2.11) and (2.12) that
Due to (1.3) and the Young inequality,
where \(D_1\) is a positive constant, which will be specified later. Therefore, by (2.13),
Taking \(D_1=\frac{1}{5}\), we have that
Observe that
Thanks to the Young inequality,
It follows from (2.14) that
We define
It follows from (2.15) that
Thanks to the Hölder inequality,
Hence,
It follows from (2.17) and (2.18) that
Due to the Young inequality,
Consequently, by (2.19),
Defined
it follows from (2.20) that
that is,
Since
by (2.22), we have that
which gives
Multiplying (2.23) by \(e^{2\ell _4t}\), we get
Therefore,
Integrating on (0, t), we have that
that is,
Using (2.16) and (2.21) in (2.24), thanks to (2.9), we have (2.8).
We prove (2.3). We begin by observing that, by (2.2),
where
Consequently, we have that
which gives,
Moreover,
It follows from (2.8), (2.27) and (2.28) that
that is
We search A such that
that is,
Therefore,
which gives
Taking \(\beta \) as in
(2.31) reads
Thanks to (2.32), we have that
Therefore, thanks to (2.33), (2.30), which is equivalent to (2.31), holds, taking A very big, and up to rescaling, we can have \(\vert \beta \vert =A^n\), with n defined in (2.32).
Consequently, by (2.32), (2.29), (2.30), or (2.31), and (2.33), there exists a constant \(C(T)>0\), independent of \(\varepsilon \), such that
Hence,
which gives (2.3).
We prove (2.4). Thanks to (2.3), (2.16) with \(A=1\), and (2.18) with \(A=1\), we have that
which gives (2.4).
Finally, we prove (2.5), (2.6), (2.7). We begin by observing that, thanks to (2.3), (2.4) and (2.15) with \(A=1\), we have that
Integrating on (0, t), by (2.2), we get
which gives (2.5), (2.6), (2.7). \(\square \)
Lemma 2.2
Fix \(\gamma ,\,\alpha ,\,\kappa ,\,\delta ,\,T\). There exists a constant \(C(T)>0\), independent of \(\varepsilon \), such that
for every \(0\le t\le T\).
Proof
Let \(0\le t\le T\). We begin by proving (2.34). [12, Lemma 2.3] says that
Thanks to (2.4), we have that
Integrating on (0, t), we have (2.34).
Finally, we prove (2.35). We begin by observing that
Due to the (2.4) and the Hölder and Young inequalities,
It follows from (2.36) that
Due to the Young inequality,
Consequently, by (2.37), we have that
Thanks to the Hölder inequality,
Hence,
Observe that
Thanks to the Hölder inequality,
It follows from (2.39) that
which gives
It follows from (2.3), (2.39) and (2.40) that
Consequently, by (2.38) and (2.41), we get
Integrating on (0, t), we have (2.35). \(\square \)
Lemma 2.3
Fix \(\gamma ,\,\alpha ,\,\kappa ,\,\delta ,\,T\). There exists a constant \(C(T)>0\), independent of \(\varepsilon \), such that
for every \(0\le t\le T\).
Proof
Let \(0\le t\le T\). Multiplying (2.1) by \(2\varepsilon \partial _{x}^4u_\varepsilon \), an integration on \(\mathbb {R}\) gives
Therefore, we have that
Since \(0<\varepsilon <1\), thanks to (2.3), (2.4) and the Young inequality,
It follows from (2.43) that
Integrating on (0, t), by (2.2) and (2.34), we get
which gives (2.42). \(\square \)
3 Proof of Theorem 1.1
This section is devoted to the proof of Theorem 1.1.
We begin by proving the following lemma.
Lemma 3.1
Fix \(\gamma ,\,\alpha ,\,\kappa ,\,\delta ,\,T\). Then,
Consequently, there exists a subsequence \(\{u_{\varepsilon _k}\}_{k\in \mathbb {N}}\) of \(\{u_\varepsilon \}_{\varepsilon >0}\) and \(u\in L^2_\mathrm{{loc}} ((0,\infty )\times \mathbb {R})\) such that, for each compact subset K of \((0,\infty )\times \mathbb {R})\),
Moreover, u is a solution of (1.1), satisfying (1.11).
Proof
We begin by proving (3.1). To prove (3.1), we rely on the Aubin–Lions Lemma (see [13, 14, 23, 24, 63]). We recall that
where the first inclusion is compact and the second is continuous. Owing to the Aubin–Lions Lemma [63], to prove (3.1), it suffices to show that
We prove (3.3). Thanks to Lemma 2.1,
Therefore,
which gives (3.3).
We prove (3.4). We begin by observing that
Therefore, by (2.1) and (3.5), we have that
where
We claim that
Moreover, thanks to (2.3) and (2.42),
Therefore, by (3.6), (3.7) and (3.8), we have that
We have that
Moreover, thanks to (2.34),
Consequently, (3.4) follows from (3.9), (3.10) and (3.11).
Thanks to the Aubin–Lions Lemma, (3.1) and (3.2) hold.
Therefore, arguing as in [14, Theorem 1.1], u is solution of (1.1) and, thanks to Lemmas 2.1 and 2.2, (1.11) holds. \(\square \)
Now, we prove Theorem 1.1.
Proof of Theorem 1.1
We begin by observing that, by (3.5), (1.1) reads:
Lemma 3.1 gives the existence of a solution (3.12) satisfying (1.11). We prove (1.12). Let \(u_1\) and \(u_2\) two solutions of (3.12), which verify (1.11), that is
Then, the function
is the solution of the following Cauchy problem:
Fixed \(T>0\), since \(u_1,\, u_2\in H^1(\mathbb {R})\), for every \(0\le t\le T\), we have that
Since \(f\in C^1(\mathbb {R})\), thanks to (3.13), there exists \(\xi \) between \( u_1\) and \(u_2\), such that
Moreover, by (2.38), we have that
Observe that, thanks to (3.13)
Thanks to (3.16) and (3.18), (3.14) reads
Multiplying (3.19) by \(2\omega \), an integration on \(\mathbb {R}\) gives
Consequently, we have that
Due to (3.15), (3.17) and the Young inequality,
It follows from (3.20) that
Thanks to the Hölder inequality,
Hence,
Due to the Young inequality,
Therefore, by (3.21), we have that
Observe that
Hence, by the Young inequality,
Consequently, by (3.22),
The Gronwall Lemma and (3.14) give
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The authors are members of the Gruppo Nazionale per l’Analisi Matematica, la Probabilità e le loro Applicazioni (GNAMPA) of the Istituto Nazionale di Alta Matematica (INdAM). GMC has been partially supported by the Research Project of National Relevance “Multiscale Innovative Materials and Structures” granted by the Italian Ministry of Education, University and Research (MIUR Prin 2017, project code 2017J4EAYB and the Italian Ministry of Education, University and Research under the Programme Department of Excellence Legge 232/2016 (Grant No. CUP-D94I18000260001).
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Coclite, G.M., di Ruvo, L. \(H^1\) Solutions for a Kuramoto–Velarde Type Equation. Mediterr. J. Math. 20, 110 (2023). https://doi.org/10.1007/s00009-023-02295-4
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DOI: https://doi.org/10.1007/s00009-023-02295-4