This paper was converted on www.awesomepapers.org from LaTeX by an anonymous user.
Want to know more? Visit the Converter page.

A Crank-Nicolson type minimization scheme
for a hyperbolic free boundary problem

Abstract

We consider a hyperbolic free boundary problem by means of minimizing time discretized functionals of Crank-Nicolson type. The feature of this functional is that it enjoys energy conservation in the absence of free boundaries, which is an essential property for numerical calculations. The existence and regularity of minimizers is shown and an energy estimate is derived. These results are then used to show the existence of a weak solution to the free boundary problem in the 1-dimensional setting.

Yoshiho Akagawa

National Institute of Technology, Gifu College

Motosu, Gifu, 501-0495 Japan

[email protected]

Elliott Ginder

Meiji Institute for Advanced Study of Mathematical Sciences, Meiji University

Nakanoku, Tokyo, 164-8525 Japan

[email protected]

Syota Koide

Graduate School of Natural Science and Technology, Kanazawa University

Kanazawa, Ishikawa, 920-1192 Japan

[email protected]

Seiro Omata

Institute of Science and Engineering, Kanazawa University

Kanazawa, Ishikawa, 920-1192 Japan

[email protected]

Karel Svadlenka(corresponding author)

Graduate School of Science, Kyoto University

Sakyoku, Kyoto, 606-8502 Japan

[email protected]


1 Introduction

In this paper we treat a variational problem related to the following hyperbolic free boundary problem:

Problem (1). Find u:Ω×[0,T)u:\Omega\times[0,T)\to\mathbb{R} such that

{χ{u>0}¯utt=ΔuinΩ×(0,T),u(x,0)=u0(x)inΩ,ut(x,0)=v0(x)inΩ,\begin{cases}\chi_{\overline{\{u>0\}}}\,u_{tt}&=\Delta u\quad\hbox{in}\,\,\Omega\times(0,T),\\ u(x,0)&=u_{0}(x)\quad\hbox{in}\,\,\Omega,\\ u_{t}(x,0)&=v_{0}(x)\quad\hbox{in}\,\,\Omega,\\ \end{cases} (1)

under suitable boundary conditions, where ΩN\Omega\subset\mathbb{R}^{N} is a bounded Lipschitz domain, T>0T>0 is the final time, u0u_{0} denotes the initial condition, v0v_{0} is the initial velocity, and {u>0}\{u>0\} is the set {(x,t)Ω×(0,T):u(x,t)>0}\{(x,t)\in\Omega\times(0,T):u(x,t)>0\}.

We observe that uu satisfies the wave equation where u>0u>0, and that uu is harmonic when u<0.u<0. It can be formally shown that, in the energy-preserving regime, solutions fulfill the following free boundary condition:

|u|2ut2=0onΩ×(0,T){u>0}.|\nabla u|^{2}-u^{2}_{t}=0\quad\hbox{on}\,\,\Omega\times(0,T)\cap\partial\{u>0\}. (2)

This kind of problem is a natural prototype for explaining phenomena involving oscillations in the presence of an obstacle, e.g., an elastic string hitting a desk or soap bubbles moving atop water. However, due to the lack of rigorous mathematical results for hyperbolic free boundary problems, numerical studies of this problem are very limited. On the other hand, interesting results have been already obtained for first-order hyperbolic free boundary problems, see, e.g., [3] for the analysis of a model of tumor growth, or [6] for the analysis of wave-structure interactions.

In this paper, we propose a numerical scheme with good energy conservation properties and provide its theoretical background at least in the case of space dimension 1. We remark that similar types of problems have been treated in [8], [13], [7] [5], and that the recent paper [11] has established a precise mathematical formulation. These papers revealed that the discrete Morse flow (also known as minimizing movements), a variational method based on time-discretized functionals, is an effective tool not only for problems of elliptic and parabolic type but also in the hyperbolic setting.

We now briefly review those previous results. Kikuchi and Omata [8] studied the problem in the one-dimensional domain Ω=(0,)\Omega=(0,\infty). They showed the existence and uniqueness of a strong solution uC2(Ω×(0,){u>0})u\in C^{2}(\Omega\times(0,\infty)\cap\{u>0\}), the regularity of its free boundary {u>0}\partial\{u>0\} and the well-posedness of the problem under suitable compatibility conditions. Yoshiuchi et al. [13] addressed a similar problem to Problem 1 including a damping term αut\alpha u_{t}. Using the discrete Morse flow, they derived an energy estimate for approximate solutions, and provided numerical results. The following problem, stated here without initial and boundary conditions, has been treated by Kikuchi in [7]:

{uttuxx0in(0,1)×(0,){u>0},spt(uttuxx){u=0},u(x,t)0L2-a.e..\begin{cases}&u_{tt}-u_{xx}\geq 0\quad\hbox{in}\,\,(0,1)\times(0,\infty)\cap\{u>0\},\\ &\hbox{spt}\,(u_{tt}-u_{xx})\subset\{u=0\},\\ &u(x,t)\geq 0\quad\hbox{$L^{2}$-a.e.}.\end{cases}

He constructed a weak solution to this problem using a minimizing method in the spirit of the discrete Morse flow. Moreover, two of the present authors, Ginder and Svadlenka, dealt with a hyperbolic free boundary problem under a volume constraint in [5]. They constructed a weak solution in the one dimensional setting, again using the discrete Morse flow. The analysis of hyperbolic obstacle problems based on this variational framework of discrete Morse flow was significantly extended to nonlocal problems (with fractional Laplacian) and to semilinear problems in a vector-valued setting by the group of Bonafini, Novaga and Orlandi in the papers [1, 2].

The technique used in this paper is similar to the discrete Morse flow used in the above papers, but it has some distinct differences. We now explain our approach, together with the organization of the paper. The first step is to consider the minimization, within the set

𝒦:={uH1(Ω);u=u0onΩ},\mathcal{K}:=\{u\in H^{1}(\Omega)\,;\,u=u_{0}\,\hbox{on}\,\partial\Omega\},

of the following time-discretized, Crank-Nicolson type functional:

Jm(u):=Ω𝒮m(u)|u2um1+um2|22h2𝑑x+14Ω|u+um2|2𝑑xJ_{m}(u):=\int_{\Omega\cap\mathcal{S}_{m}(u)}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx (3)

where 𝒮m(u)\mathcal{S}_{m}(u) denotes the set {u>0}{um1>0}{um2>0}\{u>0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\}. In the above, umu_{m} represents an approximation of the solution to the original problem at a fixed time tm=mht_{m}=mh, where mm\in{\mathbb{N}}, and h>0h>0 denotes the time step, obtained by dividing the time interval (0,T)(0,T) into MM equal parts. The difference with the previous approaches (e.g., [13], [5]) appears in the gradient term. As will be shown, our gradient term yields the energy conservation property even in the time discretized setting when there is no free boundary (i.e., when the restriction to the set 𝒮m(u)\mathcal{S}_{m}(u) is omitted). This is a significant improvement to the previous approaches, where energy conservation does not hold and leads to inaccurate numerical solutions. We believe that combination of the new energy-preserving scheme with the more advanced analytical techniques developed in [1, 2] will lead to a powerful framework. The details of the new variational scheme are presented in Section 2.

The sequence {um}\{u_{m}\} is constructed using the initial conditions u0𝒦u_{0}\in\mathcal{K} and v0H01(Ω)v_{0}\in H^{1}_{0}(\Omega). In particular, a forward differencing is used to define u1:=u0+hv0𝒦u_{1}:=u_{0}+hv_{0}\in{\mathcal{K}}. Then, for any integer m2m\geq 2, a minimizer u~m\widetilde{u}_{m} of JmJ_{m} exists and has the subsolution property (Theorem 3.1, Proposition 3.2 in Section 3), which can be shown by a standard argument, such as in [13]. We then define the cut-off minimizer um:=max{u~m,0}u_{m}:=\max\{\widetilde{u}_{m},0\} and find that the minimizers umu_{m} satisfy an energy estimate (Theorem 3.3). In particular, for any integer k1k\geq 1, we have

ukuk1hL2(Ω)2+12ukL2(Ω)2C(u0,v0,Ω),\Bigl{\|}\frac{u_{k}-u_{k-1}}{h}\Bigr{\|}_{L^{2}(\Omega)}^{2}+\frac{1}{2}\|\nabla u_{k}\|_{L^{2}(\Omega)}^{2}\leq C(u_{0},v_{0},\Omega),

where CC is independent of kk and hh. The regularity of umu_{m} can then be obtained and this leads to the first variation formula (Proposition 3.7). The next step is to define approximate weak solutions of the free boundary problem, as well as a weak solution of Problem 1. This is done in Section 4. In the case of a 1-dimensional domain, the energy estimate and the embedding theorem allow us to pass the time step size hh to zero in the equation of approximate weak solutions to obtain a weak solution of Problem 1.

In Section 4, we also formally discuss the role of free boundary condition on a more general setting for this problem, namely a hyperbolic free boundary problem with an adhesion term. When energy is not conserved, we cannot calculate the first variation in the usual way. In this case, we adopt a formal approach and derive the equation from a measure theoretic point of view. We conclude by presenting numerical results and their analysis in Section 5, emphasizing the wide applicability of the proposed numerical method.

2 Energy conservation

In this section, we derive the energy preserving property of the functional JmJ_{m} in (3), which has not been achieved in previous research. To this end, let us consider the following modified functional:

Im(u):=Ω|u2um1+um2|22h2𝑑x+14Ω|u+um2|2𝑑x,I_{m}(u):=\int_{\Omega}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx, (4)

on the set 𝒦:={uH1(Ω);u=u0onΩ}\mathcal{K}:=\{u\in H^{1}(\Omega)\,;\,u=u_{0}\,\hbox{on}\,\partial\Omega\}. This functional can be regarded as the no-free boundary version of JmJ_{m}. We note that a unique minimizer exists for each ImI_{m} whenever Im(u0)<I_{m}(u_{0})<\infty since the functional is convex and lower semicontinuous.

Theorem 2.1 (Energy conservation)

Minimizers uku_{k} of IkI_{k} conserve the energy

Ek:=ukuk1hL2(Ω)2+12(ukL2(Ω)2+uk1L2(Ω)2),E_{k}:=\Bigl{\|}\frac{u_{k}-u_{k-1}}{h}\Bigr{\|}^{2}_{L^{2}(\Omega)}+\frac{1}{2}\Bigl{(}\|\nabla u_{k}\|^{2}_{L^{2}(\Omega)}+\|\nabla u_{k-1}\|^{2}_{L^{2}(\Omega)}\Bigr{)}, (5)

in the sense that EkE_{k} is independent of k1k\geq 1.

Proof. For m2m\geq 2, the function (1λ)um+λum2=um+λ(um2um)(1-\lambda)u_{m}+\lambda u_{m-2}=u_{m}+\lambda(u_{m-2}-u_{m}) is admissible for every λ[0,1]\lambda\in[0,1], which justifies

ddλIm(um+λ(um2um))|λ=0=0.\left.\frac{d}{d\lambda}I_{m}(u_{m}+\lambda(u_{m-2}-u_{m}))\right|_{\lambda=0}=0.

Computing this derivative, we have

0\displaystyle 0 =ddλΩ[|um+λ(um2um)2um1+um2|22h2\displaystyle=\frac{d}{d\lambda}\int_{\Omega}\Bigl{[}\frac{|u_{m}+\lambda(u_{m-2}-u_{m})-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}
+14|(um+λ(um2um))+um2|2]|λ=0dx\displaystyle\left.\qquad\qquad+\frac{1}{4}|\nabla(u_{m}+\lambda(u_{m-2}-u_{m}))+\nabla u_{m-2}|^{2}\Bigr{]}\right|_{\lambda=0}\,dx
=Ω[(um2um)(um2um1+um2)h2\displaystyle=\int_{\Omega}\Bigl{[}\frac{(u_{m-2}-u_{m})(u_{m}-2u_{m-1}+u_{m-2})}{h^{2}}
+12(um2um)(um+um2)]dx\displaystyle\qquad\qquad+\frac{1}{2}\nabla(u_{m-2}-u_{m})\cdot\nabla(u_{m}+u_{m-2})\Bigr{]}\,dx
=Ω[(um1um2)2(umum1)2h2+12|um2|212|um|2]𝑑x.\displaystyle=\int_{\Omega}\Bigl{[}\frac{(u_{m-1}-u_{m-2})^{2}-(u_{m}-u_{m-1})^{2}}{h^{2}}+\frac{1}{2}|\nabla u_{m-2}|^{2}-\frac{1}{2}|\nabla u_{m}|^{2}\Bigr{]}\,dx.

Summing over m=2,,km=2,...,k, we arrive at

Ω[1h2(u1u0)21h2(ukuk1)2+12|u0|2+12|u1|212|uk1|212|uk|2]dx=0,\int_{\Omega}\Bigl{[}\frac{1}{h^{2}}(u_{1}-u_{0})^{2}-\frac{1}{h^{2}}(u_{k}-u_{k-1})^{2}\\ +\frac{1}{2}|\nabla u_{0}|^{2}+\frac{1}{2}|\nabla u_{1}|^{2}-\frac{1}{2}|\nabla u_{k-1}|^{2}-\frac{1}{2}|\nabla u_{k}|^{2}\Bigr{]}\,dx=0,

which means

E1\displaystyle E_{1} =\displaystyle= Ω[1h2(u1u0)2+12|u0|2+12|u1|2]𝑑x\displaystyle\int_{\Omega}\Bigl{[}\frac{1}{h^{2}}(u_{1}-u_{0})^{2}+\frac{1}{2}|\nabla u_{0}|^{2}+\frac{1}{2}|\nabla u_{1}|^{2}\Bigr{]}\,dx
=\displaystyle= Ω[1h2(ukuk1)2+12|uk1|2+12|uk|2]𝑑x\displaystyle\int_{\Omega}\Bigl{[}\frac{1}{h^{2}}(u_{k}-u_{k-1})^{2}+\frac{1}{2}|\nabla u_{k-1}|^{2}+\frac{1}{2}|\nabla u_{k}|^{2}\Bigr{]}\,dx
=\displaystyle= Ek,\displaystyle E_{k},

and the proof is complete.

3 The minimizing method

For any integer m2m\geq 2, we introduce the following functional:

Jm(u)=Ω𝒮m(u)|u2um1+um2|22h2𝑑x+14Ω|u+um2|2𝑑x,J_{m}(u)=\int_{\Omega\cap\mathcal{S}_{m}(u)}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx, (6)

where 𝒮m(u):={u>0}{um1>0}{um2>0}\mathcal{S}_{m}(u):=\{u>0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\}.

We determine a sequence of functions {um}\{u_{m}\} iteratively by taking u0𝒦u_{0}\in{\mathcal{K}} and u1=u0+hv0𝒦u_{1}=u_{0}+hv_{0}\in{\mathcal{K}}, defining u~m\widetilde{u}_{m} as a minimizer of JmJ_{m} in 𝒦\mathcal{K}, and setting um:=max{u~m,0}u_{m}:=\max\{\widetilde{u}_{m},0\}.

We now study the existence and regularity of minimizers which guarantees the possibility of applying the first variation formula to JmJ_{m}.

Theorem 3.1 (Existence)

If Jm(u0)<J_{m}(u_{0})<\infty, then there exists a minimizer u~m𝒦\widetilde{u}_{m}\in{\mathcal{K}} of the functional JmJ_{m}.

Proof. Given um1,um2u_{m-1},u_{m-2}, we show the existence of u~m\widetilde{u}_{m}. Since the infimum of JmJ_{m} is non-negative, we have only to show the lower semi-continuity of JmJ_{m}. Take any minimizing sequence {uj}𝒦\{u^{j}\}\subset\mathcal{K} such that Jm(uj)infu𝒦Jm(u)J_{m}(u^{j})\to\inf_{u\in\mathcal{K}}J_{m}(u) as jj\to\infty. Since the sequence {uju0}H01(Ω)\{u^{j}-u_{0}\}\subset H^{1}_{0}(\Omega) is bounded in H1(Ω)H^{1}(\Omega), there exist u~H01(Ω)\widetilde{u}\in H^{1}_{0}(\Omega) and γLp(Ω)\gamma\in L^{p}(\Omega), p[1,)p\in[1,\infty) such that, up to extracting a subsequence,

uju0\displaystyle u^{j}-u_{0} u~strongly inL2(Ω),\displaystyle\to\,\widetilde{u}\quad\hbox{strongly in}\,\,L^{2}(\Omega),
(uju0)\displaystyle\nabla(u^{j}-u_{0}) u~weakly inL2(Ω),\displaystyle\rightharpoonup\,\nabla\widetilde{u}\quad\hbox{weakly in}\,\,L^{2}(\Omega), (7)
χ𝒮m(uj)\displaystyle\chi_{\mathcal{S}_{m}(u^{j})} γweakly inLp(Ω).\displaystyle\rightharpoonup\,\gamma\quad\hbox{weakly in}\,\,L^{p}(\Omega).

Since 0γ10\leq\gamma\leq 1 a.e. on Ω\Omega, and γ=1\gamma=1 a.e. on {u>0}\{u>0\}, where u:=u~+u0𝒦u:=\widetilde{u}+u_{0}\in\mathcal{K},

Jm(u)\displaystyle J_{m}(u) =Ω|u2um1+um2|22h2χ𝒮m(u)𝑑x+14Ω|u+um2|2𝑑x\displaystyle=\int_{\Omega}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\chi_{\mathcal{S}_{m}(u)}\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx
Ω|u2um1+um2|22h2γ𝑑x+14Ω|u+um2|2𝑑x\displaystyle\leq\int_{\Omega}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\gamma\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx
lim infjJm(uj),\displaystyle\leq\liminf_{j\to\infty}J_{m}(u^{j}),

where the second inequality follows from (3).

The minimizers of JmJ_{m} have the following subsolution property.

Proposition 3.2 (Subsolution)

Any minimizer uu of JmJ_{m} satisfies the following inequality for arbitrary nonnegative ζH01(Ω)\zeta\in H_{0}^{1}(\Omega):

Ω𝒮m(u)u2um1+um2h2ζ𝑑x+Ωu+um22ζdx0.\int_{\Omega\cap\mathcal{S}_{m}(u)}\frac{u-2u_{m-1}+u_{m-2}}{h^{2}}\zeta\,dx+\int_{\Omega}\nabla\frac{u+u_{m-2}}{2}\cdot\nabla\zeta\,dx\leq 0. (8)

Proof. Fixing ζC0(Ω)\zeta\in C_{0}^{\infty}(\Omega) with ζ0\zeta\geq 0, and ε>0\varepsilon>0, we have

0\displaystyle 0 Jm(uεζ)Jm(u)(by the minimality of u)\displaystyle\leq J_{m}(u-\varepsilon\zeta)-J_{m}(u)\quad(\hbox{by the minimality of $u$})
=Ω|(uεζ)2um1+um2|22h2χ𝒮m(uεζ)𝑑x+14Ω|(uεζ)+um2|2𝑑x\displaystyle=\int_{\Omega}\frac{|(u-\varepsilon\zeta)-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\chi_{\mathcal{S}_{m}(u-\varepsilon\zeta)}\,dx+\frac{1}{4}\int_{\Omega}|\nabla(u-\varepsilon\zeta)+\nabla u_{m-2}|^{2}\,dx
(Ω|u2um1+um2|22h2χ𝒮m(u)𝑑x+14Ω|u+um2|2𝑑x).\displaystyle\qquad-\Bigl{(}\int_{\Omega}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\chi_{\mathcal{S}_{m}(u)}\,dx+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx\Bigr{)}. (9)

Noting that,

χ𝒮m(uεζ)χ𝒮m(u)0,\displaystyle\chi_{\mathcal{S}_{m}(u-\varepsilon\zeta)}-\chi_{\mathcal{S}_{m}(u)}\leq 0,
|(uεζ)2um1+um2|2|u2um1+um2|2\displaystyle|(u-\varepsilon\zeta)-2u_{m-1}+u_{m-2}|^{2}-|u-2u_{m-1}+u_{m-2}|^{2}
=2εζ(u2um1+um2)+ε2ζ2,\displaystyle\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad\qquad=-2\varepsilon\zeta(u-2u_{m-1}+u_{m-2})+\varepsilon^{2}\zeta^{2},
|(uεζ)+um2|2|u+um2|2=2ε(u+um2)ζ+ε2|ζ|2,\displaystyle|\nabla(u-\varepsilon\zeta)+\nabla u_{m-2}|^{2}-|\nabla u+\nabla u_{m-2}|^{2}=-2\varepsilon(\nabla u+\nabla u_{m-2})\cdot\nabla\zeta+\varepsilon^{2}|\nabla\zeta|^{2},

we continue the estimate as

(3)\displaystyle(\ref{subpro_proof1}) Ω{2εζ(u2um1+um2)+ε2ζ2}×12h2χ𝒮m(u)𝑑x\displaystyle\leq\int_{\Omega}\{-2\varepsilon\zeta(u-2u_{m-1}+u_{m-2})+\varepsilon^{2}\zeta^{2}\}\times\frac{1}{2h^{2}}\chi_{\mathcal{S}_{m}(u)}\,dx
+14Ω{2ε(u+um2)ζ+ε2|ζ|2}𝑑x.\displaystyle\qquad+\frac{1}{4}\int_{\Omega}\{-2\varepsilon(\nabla u+\nabla u_{m-2})\cdot\nabla\zeta+\varepsilon^{2}|\nabla\zeta|^{2}\}\,dx.

Dividing by ε\varepsilon, letting ε\varepsilon decrease to zero from above, and applying a density argument concludes the proof.

We now derive an energy estimate satisfied by the minimizers of JmJ_{m}.

Theorem 3.3 (Energy estimate)

For any integer k1k\geq 1, we have

ukuk1hL2(Ω)2+12ukL2(Ω)2v0L2(Ω)2+12u0L2(Ω)2+12u1L2(Ω)2.\Bigl{\|}\frac{u_{k}-u_{k-1}}{h}\Bigr{\|}_{L^{2}(\Omega)}^{2}+\frac{1}{2}\|\nabla u_{k}\|_{L^{2}(\Omega)}^{2}\leq\|v_{0}\|_{L^{2}(\Omega)}^{2}+\frac{1}{2}\|\nabla u_{0}\|_{L^{2}(\Omega)}^{2}+\frac{1}{2}\|\nabla u_{1}\|_{L^{2}(\Omega)}^{2}. (10)

Proof. Since the function (1λ)u~m+λum2=u~m+λ(um2u~m)(1-\lambda)\widetilde{u}_{m}+\lambda u_{m-2}=\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m}) belongs to 𝒦\mathcal{K} for any λ[0,1]\lambda\in[0,1], by the minimality property, we have Jm(u~m)Jm(u~m+λ(um2u~m))J_{m}(\widetilde{u}_{m})\leq J_{m}(\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})), and thus,

limλ0+1λ(Jm(u~m+λ(um2u~m))Jm(u~m))0.\lim_{\lambda\rightarrow 0+}{\frac{1}{\lambda}}\Bigl{(}J_{m}(\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m}))-J_{m}(\widetilde{u}_{m})\Bigr{)}\geq 0. (11)

Let AmA_{m} denote the set

Am:=Ω({u~m>0}{um1>0}{um2>0}).A_{m}:=\Omega\cap(\{\widetilde{u}_{m}>0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\}).

We investigate the behavior of the individual terms in (11)(\ref{EE1}). For the gradient term we get

limλ0+14λ(|(u~m+λ(um2u~m)+um2)|2|(u~m+um2)|2)\displaystyle\lim_{\lambda\rightarrow 0+}\frac{1}{4\lambda}\left(|\nabla(\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})+u_{m-2})|^{2}-|\nabla(\widetilde{u}_{m}+u_{m-2})|^{2}\right)
=12(u~m+um2)(um2u~m)dx\displaystyle\qquad\qquad=\frac{1}{2}\nabla(\widetilde{u}_{m}+u_{m-2})\cdot\nabla(u_{m-2}-\widetilde{u}_{m})\,dx
=12|um2|212|u~m|2\displaystyle\qquad\qquad=\frac{1}{2}|\nabla u_{m-2}|^{2}-\frac{1}{2}|\nabla\widetilde{u}_{m}|^{2}
12|um2|212|um|2.\displaystyle\qquad\qquad\leq\frac{1}{2}|\nabla u_{m-2}|^{2}-\frac{1}{2}|\nabla u_{m}|^{2}. (12)

For the time-discretized term, taking into account that the set

Bm(λ):={u~m+λ(um2u~m)>0}{um1>0}{um2>0}B_{m}(\lambda):=\{\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})>0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\}

is contained in the set AmA_{m}, we find that

12h2Ω(|u~m+λ(um2u~m)2um1+um2|2χBm(λ)\displaystyle\frac{1}{2h^{2}}\int_{\Omega}\Bigl{(}|\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})-2u_{m-1}+u_{m-2}|^{2}\chi_{B_{m}(\lambda)}
|u~m2um1+um2|2χAm)dx\displaystyle\qquad-|\widetilde{u}_{m}-2u_{m-1}+u_{m-2}|^{2}\chi_{A_{m}}\Bigr{)}\,dx
12h2Ω(|u~m+λ(um2u~m)2um1+um2|2\displaystyle\leq\frac{1}{2h^{2}}\int_{\Omega}\Bigl{(}|\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})-2u_{m-1}+u_{m-2}|^{2}
|u~m2um1+um2|2)χAmdx.\displaystyle\qquad-|\widetilde{u}_{m}-2u_{m-1}+u_{m-2}|^{2}\Bigr{)}\chi_{A_{m}}\,dx.

Then we have

limλ0+12h2λΩ(|u~m+λ(um2u~m)2um1+um2|2\displaystyle\lim_{\lambda\to 0+}\frac{1}{2h^{2}\lambda}\int_{\Omega}\Bigl{(}|\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})-2u_{m-1}+u_{m-2}|^{2}
|u~m2um1+um2|2)χAmdx\displaystyle\qquad-|\widetilde{u}_{m}-2u_{m-1}+u_{m-2}|^{2}\Bigr{)}\chi_{A_{m}}\,dx
=limλ0+12h2Am(um2u~m)(2u~m+λ(um2u~m)4um1+2um2)𝑑x\displaystyle=\lim_{\lambda\to 0+}\frac{1}{2h^{2}}\int_{A_{m}}(u_{m-2}-\widetilde{u}_{m})(2\widetilde{u}_{m}+\lambda(u_{m-2}-\widetilde{u}_{m})-4u_{m-1}+2u_{m-2})\,dx (13)
=1h2Am(um2u~m)(u~m2um1+um2)𝑑x\displaystyle=\frac{1}{h^{2}}\int_{A_{m}}(u_{m-2}-\widetilde{u}_{m})(\widetilde{u}_{m}-2u_{m-1}+u_{m-2})\,dx
=1h2Am[(um1um2)2(um1u~m)2]𝑑x.\displaystyle=\frac{1}{h^{2}}\int_{A_{m}}[(u_{m-1}-u_{m-2})^{2}-(u_{m-1}-\widetilde{u}_{m})^{2}]\,dx.

Now, Am(um1um2)2𝑑xΩ(um1um2)2𝑑x\int_{A_{m}}(u_{m-1}-u_{m-2})^{2}\,dx\leq\int_{\Omega}(u_{m-1}-u_{m-2})^{2}\,dx since the integrand is non-negative. Moreover, um=max{u~m,0}u_{m}=\max\{\widetilde{u}_{m},0\} and um10u_{m-1}\geq 0 imply (um1u~m)2(um1um)2(u_{m-1}-\widetilde{u}_{m})^{2}\geq(u_{m-1}-u_{m})^{2}, therefore

Am(um1u~m)2𝑑xAm(um1um)2𝑑x.-\int_{A_{m}}(u_{m-1}-\widetilde{u}_{m})^{2}\,dx\leq-\int_{A_{m}}(u_{m-1}-u_{m})^{2}\,dx.

Noting that, outside of AmA_{m}, both umu_{m} and um1u_{m-1} vanish, we get

Am(um1um)2𝑑x=Ω(um1um)2𝑑x.-\int_{A_{m}}(u_{m-1}-u_{m})^{2}\,dx=-\int_{\Omega}(u_{m-1}-u_{m})^{2}\,dx.

Returning to (3), we get the estimate for the time discretized term:

the right hand side of(3)1h2Ω[(um1um2)2(um1um)2]𝑑x.\hbox{the right hand side of}\,\,(\ref{time_dis_estimate})\leq\frac{1}{h^{2}}\int_{\Omega}[(u_{m-1}-u_{m-2})^{2}-(u_{m-1}-u_{m})^{2}]dx.

Combining this result and the gradient term estimate (3), we obtain

Ω[1h2(um1um2)21h2(um1um)2+12|um2|212|um|2]𝑑x0.\int_{\Omega}\Bigl{[}\frac{1}{h^{2}}(u_{m-1}-u_{m-2})^{2}-\frac{1}{h^{2}}(u_{m-1}-u_{m})^{2}+\frac{1}{2}|\nabla u_{m-2}|^{2}-\frac{1}{2}|\nabla u_{m}|^{2}\Bigr{]}\,dx\geq 0.

Summing over m=2,,km=2,...,k, we arrive at

Ω[1h2(u1u0)21h2(ukuk1)2+12|u0|2+12|u1|212|uk1|212|uk|2]dx0,\int_{\Omega}\Bigl{[}\frac{1}{h^{2}}(u_{1}-u_{0})^{2}-\frac{1}{h^{2}}(u_{k}-u_{k-1})^{2}\\ +\frac{1}{2}|\nabla u_{0}|^{2}+\frac{1}{2}|\nabla u_{1}|^{2}-\frac{1}{2}|\nabla u_{k-1}|^{2}-\frac{1}{2}|\nabla u_{k}|^{2}\Bigr{]}\,dx\geq 0,

which, after omitting the term |uk1|20,|\nabla u_{k-1}|^{2}\geq 0, yields the desired estimate.

The following theorem is obtained by a standard argument from elliptic regularity theory. For the sake of completeness, we shall briefly demonstrate it.

Theorem 3.4 (Regularity)

Assume, in addition, that u0,u1u_{0},u_{1} belong to L(Ω)Cloc0,α0(Ω)L^{\infty}(\Omega)\cap C^{0,\alpha_{0}}_{\mathrm{loc}}(\Omega) for some α0(0,1)\alpha_{0}\in(0,1), where u1:=u0+hv0u_{1}:=u_{0}+hv_{0}, and u0u_{0} are non-negative. For every Ω~Ω\widetilde{\Omega}\subset\subset\Omega, there exists a positive constant α(0,1)\alpha\in(0,1) independent of mm, such that the minimizers u~m\widetilde{u}_{m} belong to C0,α(Ω~)C^{0,\alpha}(\tilde{\Omega}).

To prove this, we prepare two lemmas.

Lemma 3.5

u~mL(Ω)\widetilde{u}_{m}\in L^{\infty}(\Omega) for every m2m\geq 2.

Proof. We use mathematical induction for m2m\geq 2. For m=2m=2, setting ψδ(u):=uδ(u+u0k)+𝒦\psi_{\delta}(u):=u-\delta(u+u_{0}-k)^{+}\in\mathcal{K}, where u:=u~2u:=\widetilde{u}_{2}, (u+u0k)+:=max{u+u0k,0}(u+u_{0}-k)^{+}:=\max\{u+u_{0}-k,0\}, δ>0\delta>0, kmax{2maxΩu0,1}k\geq\max\{2\max_{\partial\Omega}u_{0},1\}, we calculate the quantity J2(ψδ(u))J2(u)J_{2}(\psi_{\delta}(u))-J_{2}(u), which is non-negative by the minimality of uu. Noting that Sm(ψδ(u))Sm(u)S_{m}(\psi_{\delta}(u))\subset S_{m}(u), we have

0\displaystyle 0 J2(ψδ(u))J2(u)\displaystyle\leq J_{2}(\psi_{\delta}(u))-J_{2}(u)
Ω(|ψδ(u)2u1+u0|22h2|u2u1+u0|22h2)χ𝒮2(u)𝑑x\displaystyle\leq\int_{\Omega}\Bigl{(}\frac{|\psi_{\delta}(u)-2u_{1}+u_{0}|^{2}}{2h^{2}}-\frac{|u-2u_{1}+u_{0}|^{2}}{2h^{2}}\Bigr{)}\chi_{\mathcal{S}_{2}(u)}\,dx
+14Ω(|ψδ(u)+u0|2|u+u0|2)𝑑x.\displaystyle\qquad+\frac{1}{4}\int_{\Omega}\Bigl{(}|\nabla\psi_{\delta}(u)+\nabla u_{0}|^{2}-|\nabla u+\nabla u_{0}|^{2}\Bigr{)}\,dx.

Dividing by δ\delta, letting δ0+\delta\to 0+, and setting Ak:={u+u0>k}A_{k}:=\{u+u_{0}>k\}, we get

0\displaystyle 0 Ak𝒮2(u)u2u1+u0h2(u+u0k)𝑑x12Ak|u+u0|2𝑑x\displaystyle\leq-\int_{A_{k}\cap\mathcal{S}_{2}(u)}\frac{u-2u_{1}+u_{0}}{h^{2}}(u+u_{0}-k)\,dx-\frac{1}{2}\int_{A_{k}}|\nabla u+\nabla u_{0}|^{2}\,dx
Ak𝒮2(u)2u1h2(u+u0k)𝑑x12Ak|u+u0|2𝑑x\displaystyle\leq\int_{A_{k}\cap\mathcal{S}_{2}(u)}\frac{2u_{1}}{h^{2}}(u+u_{0}-k)\,dx-\frac{1}{2}\int_{A_{k}}|\nabla u+\nabla u_{0}|^{2}\,dx
Ch2(12Ak(u+u0k)2𝑑x+12|Ak|)12Ak|u+u0|2𝑑x,\displaystyle\leq\frac{C}{h^{2}}\Bigl{(}\frac{1}{2}\int_{A_{k}}(u+u_{0}-k)^{2}\,dx+\frac{1}{2}|A_{k}|\Bigr{)}-\frac{1}{2}\int_{A_{k}}|\nabla u+\nabla u_{0}|^{2}\,dx,

where we have used Young’s inequality at the last line. Since k1k\geq 1, we get

Ak|u+u0|2𝑑xC(Ak(u+u0k)2𝑑x+k2|Ak|).\int_{A_{k}}|\nabla u+\nabla u_{0}|^{2}\,dx\leq C\Bigl{(}\int_{A_{k}}(u+u_{0}-k)^{2}\,dx+k^{2}|A_{k}|\Bigr{)}.

Therefore, by [9, Theorem 2.5.1], we find that u+u0L(Ω)u+u_{0}\in L^{\infty}(\Omega), and hence u=u~2L(Ω)u=\widetilde{u}_{2}\in L^{\infty}(\Omega).

Next, we assume that u~kL(Ω)\widetilde{u}_{k}\in L^{\infty}(\Omega) for all k=2,,m1k=2,...,m-1. Since uk=max{u~k,0}u_{k}=\max\{\widetilde{u}_{k},0\} belongs to L(Ω)L^{\infty}(\Omega) for all k=2,,m1k=2,...,m-1, by repeating the above argument with u~2,u1,u0\widetilde{u}_{2},u_{1},u_{0} replaced by u~m,um1,um2\widetilde{u}_{m},u_{m-1},u_{m-2}, respectively, we get u~m+um2L(Ω)\widetilde{u}_{m}+u_{m-2}\in L^{\infty}(\Omega). Therefore, u~mL(Ω)\widetilde{u}_{m}\in L^{\infty}(\Omega).

The previous result implies that there exists μ>0\mu>0, which depends only on Ω,u0,u1,h\Omega,u_{0},u_{1},h but not on mm, such that supΩ|u~m|μ\sup_{\Omega}|\widetilde{u}_{m}|\leq\mu.

Lemma 3.6

Fix d>0d>0. There exists γ=γ(Ω,μ,d,h)>0\gamma=\gamma(\Omega,\mu,d,h)>0 such that for U=±(u~m+um2)U=\pm(\widetilde{u}_{m}+u_{m-2}),

Ak,rσr|U|2𝑑xγ[1(σr)2supBr(Uk)2+1]|Ak,r|\int_{A_{k,r-\sigma r}}|\nabla U|^{2}\,dx\leq\gamma\Bigl{[}\frac{1}{(\sigma r)^{2}}\sup_{B_{r}}(U-k)^{2}+1\Bigr{]}|A_{k,r}|

for all σ(0,1)\sigma\in(0,1), BrΩB_{r}\subset\Omega, and kk with kmaxBrUdk\geq\max_{B_{r}}U-d, where Ak,r:={xBr;U(x)>k}A_{k,r}:=\{x\in B_{r};U(x)>k\}, and BrB_{r} is a ball of radius rr.

Proof. For fixed m2m\geq 2, first we show the statement for U=u~m+um2U=\widetilde{u}_{m}+u_{m-2}. We set ζ=η2max{u+um2k,0}\zeta=\eta^{2}\max\{u+u_{m-2}-k,0\} in Proposition 3.2, where u:=u~mu:=\widetilde{u}_{m}, kk is a real number with kmaxBr(u+um2)dk\geq\max_{B_{r}}(u+u_{m-2})-d, η\eta is smooth function with sptηBr\hbox{spt}\,\eta\subset B_{r}, 0η10\leq\eta\leq 1, η1\eta\equiv 1 on BsB_{s}, |η|2/(rs)|\nabla\eta|\leq 2/(r-s) in BrBsB_{r}\setminus B_{s}, and s=rσr(0,r)s=r-\sigma r\in(0,r), σ(0,1)\sigma\in(0,1). Then, using the boundedness of u,um1,um2u,u_{m-1},u_{m-2}, we get

0\displaystyle 0 Ak,r𝒮m(u)u2um1+um2h2η2(u+um2k)𝑑x\displaystyle\leq-\int_{A_{k,r}\cap\mathcal{S}_{m}(u)}\frac{u-2u_{m-1}+u_{m-2}}{h^{2}}\eta^{2}(u+u_{m-2}-k)\,dx
12Ak,r(u+um2)(2η)η(u+um2k)𝑑x\displaystyle\quad-\frac{1}{2}\int_{A_{k,r}}(\nabla u+\nabla u_{m-2})\cdot(2\eta)\nabla\eta(u+u_{m-2}-k)\,dx
12Ak,r|u+um2|2η2𝑑x\displaystyle\qquad-\frac{1}{2}\int_{A_{k,r}}|\nabla u+\nabla u_{m-2}|^{2}\eta^{2}\,dx
C|Ak,r|+12(12Ak,r|(u+um2)|2η2𝑑x+2Ak,r|η|2(u+um2k)2𝑑x)\displaystyle\leq C|A_{k,r}|+\frac{1}{2}\Bigl{(}\frac{1}{2}\int_{A_{k,r}}|\nabla(u+u_{m-2})|^{2}\eta^{2}\,dx+2\int_{A_{k,r}}|\nabla\eta|^{2}(u+u_{m-2}-k)^{2}\,dx\Bigr{)}
12Ak,r|u+um2|2η2𝑑x\displaystyle\quad-\frac{1}{2}\int_{A_{k,r}}|\nabla u+\nabla u_{m-2}|^{2}\eta^{2}\,dx
C[1+1(σr)2supBr(u+um2k)2]|Ak,r|14Ak,s|(u+um2)|2dx,\displaystyle\leq C\Bigr{[}1+\frac{1}{(\sigma r)^{2}}\sup_{B_{r}}(u+u_{m-2}-k)^{2}\Bigr{]}|A_{k,r}|-\frac{1}{4}\int_{A_{k,s}}|\nabla(u+u_{m-2})|^{2}\,dx,

where the constant CC depends only on h,μ,d,Ωh,\mu,d,\Omega.

Next, we prove the same inequality for U=(u~m+um2)U=-(\widetilde{u}_{m}+u_{m-2}). Note that u~m-\widetilde{u}_{m} is a minimizer of the following functional:

Jm(w):=Ω𝒮m(w)|w+2um1um2|22h2𝑑x+14Ω|wum2|2𝑑x.\displaystyle J_{m}^{-}(w):=\int_{\Omega\cap\mathcal{S}_{m}^{-}(w)}\frac{|w+2u_{m-1}-u_{m-2}|^{2}}{2h^{2}}\,dx+\frac{1}{4}\int_{\Omega}|\nabla w-\nabla u_{m-2}|^{2}\,dx.
in the set𝒦:={wH1(Ω);w=u0onΩ},\displaystyle\qquad\text{in the set}\quad{\mathcal{K}}^{-}:=\left\{w\in H^{1}(\Omega);\,w=-u_{0}\,\,\hbox{on}\,\,\partial\Omega\right\},

where 𝒮m(w)\mathcal{S}_{m}^{-}(w) is defined to be the set {w<0}{um1>0}{um2>0}\{w<0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\}.

Now, for w:=u~mw:=-\widetilde{u}_{m}, we set φ:=wζ𝒦\varphi:=w-\zeta\in{\mathcal{K}}^{-} where ζ:=ηmax{wum2k,0}\zeta:=\eta\max\{w-u_{m-2}-k,0\}, kk is a real number with kmaxBr(wum2)dk\geq\max_{B_{r}}(w-u_{m-2})-d, and η\eta is a smooth function chosen in the same way as above. Then, by the minimality of ww,

0\displaystyle 0 Jm(φ)Jm(w)\displaystyle\leq J_{m}^{-}(\varphi)-J_{m}^{-}(w)
Ω𝒮m(φ)(2(w+2um1um2)2h2ζ+|ζ|22h2)𝑑x\displaystyle\leq\int_{\Omega\cap\mathcal{S}_{m}^{-}(\varphi)}\Bigl{(}\frac{-2(w+2u_{m-1}-u_{m-2})}{2h^{2}}\zeta+\frac{|\zeta|^{2}}{2h^{2}}\Bigr{)}\,dx
+Ω|w+2um1um2|22h2(χ𝒮m(φ)χ𝒮m(w))𝑑x\displaystyle\qquad+\int_{\Omega}\frac{|w+2u_{m-1}-u_{m-2}|^{2}}{2h^{2}}\Bigl{(}\chi_{\mathcal{S}_{m}^{-}(\varphi)}-\chi_{\mathcal{S}_{m}^{-}(w)}\Bigr{)}\,dx
+14Ω|φum2|2𝑑x14Ω|wum2|2𝑑x.\displaystyle\qquad\qquad+\frac{1}{4}\int_{\Omega}|\nabla\varphi-\nabla u_{m-2}|^{2}\,dx-\frac{1}{4}\int_{\Omega}|\nabla w-\nabla u_{m-2}|^{2}\,dx. (14)

Note that the term in the third line is less than or equal to 12h2sptζ|w+2um1um2|2𝑑x\frac{1}{2h^{2}}\int_{\hbox{spt}\,\zeta}|w+2u_{m-1}-u_{m-2}|^{2}\,dx, since χ𝒮m(φ)χ𝒮m(w)\chi_{\mathcal{S}_{m}^{-}(\varphi)}-\chi_{\mathcal{S}_{m}^{-}(w)} is positive only for xx satisfying 0w(x)<ζ(x)0\leq w(x)<\zeta(x). Therefore, recalling that sptζAk,r\hbox{spt}\,\zeta\subset A_{k,r}, the first two terms on the right-hand side of (3) are less than or equal to C|Ak,r|C|A_{k,r}|, where CC is a constant depending only Ω,μ,d,h\Omega,\mu,d,h. Then, we continue the estimate (3) as follows:

0\displaystyle 0 C|Ak,r|+12Ak,r(1η)2|wum2|2𝑑x\displaystyle\leq C|A_{k,r}|+\frac{1}{2}\int_{A_{k,r}}(1-\eta)^{2}|\nabla w-\nabla u_{m-2}|^{2}\,dx
+12Ak,r(wum2k)2|η|2𝑑x14Ak,r|wum2|2𝑑x\displaystyle\quad+\frac{1}{2}\int_{A_{k,r}}(w-u_{m-2}-k)^{2}|\nabla\eta|^{2}\,dx-\frac{1}{4}\int_{A_{k,r}}|\nabla w-\nabla u_{m-2}|^{2}\,dx
C|Ak,r|+12Ak,r|(wum2)|2𝑑x+2(σr)2Ak,r(wum2k)2𝑑x\displaystyle\leq C|A_{k,r}|+\frac{1}{2}\int_{A_{k,r}}|\nabla(w-u_{m-2})|^{2}\,dx+\frac{2}{(\sigma r)^{2}}\int_{A_{k,r}}(w-u_{m-2}-k)^{2}\,dx
34Ak,s|(wum2)|2𝑑x.\displaystyle\quad-\frac{3}{4}\int_{A_{k,s}}|\nabla(w-u_{m-2})|^{2}\,dx.

Therefore, we get

Ak,s|(wum2)|2𝑑xC|Ak,r|+θAk,r|(wum2)|2𝑑x\displaystyle\int_{A_{k,s}}|\nabla(w-u_{m-2})|^{2}\,dx\leq C|A_{k,r}|+\theta\int_{A_{k,r}}|\nabla(w-u_{m-2})|^{2}\,dx
+831(σr)2Ak,r(wum2k)2𝑑x,\displaystyle\qquad+\frac{8}{3}\frac{1}{(\sigma r)^{2}}\int_{A_{k,r}}(w-u_{m-2}-k)^{2}\,dx,

where θ=23<1\theta=\frac{2}{3}<1. By Lemma V. 3.1 in [4], we obtain

Ak,s|(wum2)|2𝑑xC|Ak,r|+831(σr)2Ak,r(wum2k)2𝑑x,\int_{A_{k,s}}|\nabla(w-u_{m-2})|^{2}\,dx\leq C|A_{k,r}|+\frac{8}{3}\frac{1}{(\sigma r)^{2}}\int_{A_{k,r}}(w-u_{m-2}-k)^{2}\,dx,

which is the desired estimate for (u~m+um2)-(\widetilde{u}_{m}+u_{m-2}).

Proof of Theorem 3.4. Lemmas 3.5 and 3.6 imply that u~:=u~m+um2\widetilde{u}:=\widetilde{u}_{m}+u_{m-2} (m2m\geq 2) belongs to the De Giorgi class 2(Ω,μ,γ,d)\mathcal{B}_{2}(\Omega,\mu,\gamma,d). Thus, by De Giorgi’s embedding theorem ([9, Section 2.6]), u~m+um2C0,α~(Ω~)\widetilde{u}_{m}+u_{m-2}\in C^{0,\widetilde{\alpha}}(\widetilde{\Omega}) for some α~(0,1)\widetilde{\alpha}\in(0,1) which is independent of mm. We can now prove that u~mC0,α(Ω~)\widetilde{u}_{m}\in C^{0,\alpha}(\widetilde{\Omega}) for some α(0,1)\alpha\in(0,1). To this end, set α:=min{α0,α~}\alpha:=\min\{\alpha_{0},\widetilde{\alpha}\}. For m=2m=2, by the fact that u~2+u0C0,α~(Ω~)C0,α(Ω~)\widetilde{u}_{2}+u_{0}\in C^{0,\widetilde{\alpha}}(\widetilde{\Omega})\subset C^{0,\alpha}(\widetilde{\Omega}), and the assumption u0C0,α0(Ω~)C0,α(Ω~)u_{0}\in C^{0,\alpha_{0}}(\widetilde{\Omega})\subset C^{0,\alpha}(\widetilde{\Omega}), we see that u~2C0,α(Ω~)\widetilde{u}_{2}\in C^{0,\alpha}(\widetilde{\Omega}). Hence, u2:=max{u~,0}u_{2}:=\max\{\widetilde{u},0\} belongs to the same space. Now, we assume that u~kC0,α(Ω~)\widetilde{u}_{k}\in C^{0,\alpha}(\widetilde{\Omega}) for any k=2,.,m1k=2,....,m-1. Then, since um2C0,α(Ω~)u_{m-2}\in C^{0,\alpha}(\widetilde{\Omega}), and u~m+um2C0,α~(Ω~)C0,α(Ω~)\widetilde{u}_{m}+u_{m-2}\in C^{0,\widetilde{\alpha}}(\widetilde{\Omega})\subset C^{0,\alpha}(\widetilde{\Omega}), we have u~mC0,α(Ω~)\widetilde{u}_{m}\in C^{0,\alpha}(\widetilde{\Omega}).

By the above theorem, we can choose the support of test functions within the open set {u~m>0}\{\widetilde{u}_{m}>0\}, which leads to the following first variation formula for JmJ_{m}.

Proposition 3.7 (First variation formula)

Any minimizer uu of JmJ_{m} for m=2,3,,Mm=2,3,\dots,M, satisfies the following equation:

Ω(u2um1+um2h2ϕ+u+um22ϕ)𝑑x=0\int_{\Omega}\left(\frac{u-2u_{m-1}+u_{m-2}}{h^{2}}\phi+\nabla\frac{u+u_{m-2}}{2}\cdot\nabla\phi\right)dx=0 (15)

for all ϕC0(Ω{u>0})\phi\in C_{0}^{\infty}(\Omega\cap\{u>0\}).

Proof Since {u>0}\{u>0\} is an open set by Theorem 3.2, we can calculate the first variation of JmJ_{m} using u+εϕu+\varepsilon\phi with ϕC0(Ω{u>0})\phi\in C_{0}^{\infty}(\Omega\cap\{u>0\}) as a test function. The result then follows by noting that there exists ε0>0\varepsilon_{0}>0 such that χ𝒮m(u+εϕ)=χ𝒮m(u)\chi_{\mathcal{S}_{m}(u+\varepsilon\phi)}=\chi_{\mathcal{S}_{m}(u)} for |ε|<ε0|\varepsilon|<\varepsilon_{0}.

4 Definition and existence of weak solutions

In this section, we will construct weak solutions to Problem 1 in the one dimensional setting. First, we state the definition.

Definition 4.1 (Weak solution)

For a given T>0T>0, a weak solution is defined as a function uH1((0,T);L2(Ω))L((0,T);H01(Ω))u\in H^{1}((0,T);L^{2}(\Omega))\cap L^{\infty}((0,T);H^{1}_{0}(\Omega)) satisfying the following equality, for all test functions ϕC0(Ω×[0,T){u>0})\phi\in C_{0}^{\infty}(\Omega\times[0,T)\cap\{u>0\}):

0TΩ(utϕt+uϕ)𝑑x𝑑tΩv0ϕ(x,0)𝑑x=0.\int_{0}^{T}\int_{\Omega}\left(-u_{t}\phi_{t}+\nabla u\cdot\nabla\phi\right)dxdt-\int_{\Omega}v_{0}\phi(x,0)dx=0. (16)

Moreover, we require that u0u\equiv 0 is satisfied outside of {u>0}\{u>0\}, and that u(0,x)=u0(x)u(0,x)=u_{0}(x) in Ω\Omega in the sense of traces.

Remark 1

This weak solution contains two pieces of information, namely, the wave equation on the positive part {u>0}\{u>0\}, and harmonicity on the interior of the complement. If we assume the above weak solution preserves energy and has a regular free boundary, we can formally derive a free boundary condition solely from the definition of the weak solution. If we consider more general settings, such as including an adhesion term, the problem becomes more complicated and requires a different notion of a weak solution. For details, see Remark 3.

In constructing our weak solution, we carry out interpolation in time of the cut-off minimizers {um}\{u_{m}\} of JmJ_{m}, and introduce the notion of approximate weak solutions. In particular, we define u¯h\overline{u}^{h} and uhu^{h} on Ω×(0,T)\Omega\times(0,T) by

u¯h(x,t)\displaystyle\overline{u}^{h}(x,t) =\displaystyle= um(x),m=0,1,2,,M\displaystyle u_{m}(x),\qquad m=0,1,2,\dots,M
uh(x,t)\displaystyle u^{h}(x,t) =\displaystyle= t(m1)hhum(x)+mhthum1(x),m=1,2,3,,M\displaystyle\displaystyle\frac{t-(m-1)h}{h}u_{m}(x)+\frac{mh-t}{h}u_{m-1}(x),\qquad m=1,2,3,\dots,M

for (x,t)Ω×((m1)h,mh](x,t)\in\Omega\times((m-1)h,mh]. These functions allow us to construct the following approximate solution based on the first variation formula (Proposition 3.7).

Definition 4.2 (Approximate weak solution)

We call a sequence of functions {um}𝒦\{u_{m}\}\subset\mathcal{K} an approximate weak solution of Problem 1 if the functions u¯h\overline{u}^{h} and uhu^{h} defined above satisfy

hTΩ(uth(t)uth(th)hϕ+u¯h(t)+u¯h(t2h)2ϕ)𝑑x𝑑t=0\displaystyle\int_{h}^{T}\int_{\Omega}\left(\frac{u^{h}_{t}(t)-u^{h}_{t}(t-h)}{h}\phi+\nabla\frac{\overline{u}^{h}(t)+\overline{u}^{h}(t-2h)}{2}\cdot\nabla\phi\right)\,dx\,dt=0\quad
for allϕC0(Ω×[0,T){uh>0}),\displaystyle\qquad\qquad\hbox{for all}\,\,\,\phi\in C_{0}^{\infty}(\Omega\times[0,T)\cap\{u^{h}>0\}),
uh0inΩ×(0,T){uh>0}.\displaystyle\qquad\qquad u^{h}\equiv 0\quad\mbox{\rm in}\quad\Omega\times(0,T)\setminus\{u^{h}>0\}. (17)

We further require that the initial conditions uh(x,0)=u0(x)u^{h}(x,0)=u_{0}(x) and uh(x,h)=u0(x)+hv0(x)u^{h}(x,h)=u_{0}(x)+hv_{0}(x) are fulfilled.

If one can pass to the limit as h0h\rightarrow 0, then the above approximate weak solutions are expected to converge to a weak solution defined above. In the one-dimensional setting, that is dimΩ=1\hbox{dim}\,\Omega=1, by energy estimate (10) in Section 3, we obtain the following convergence result, as in [7].

Lemma 4.3 (Limit of approximate weak solution)

Let Ω\Omega\subset\mathbb{R} be a bounded open interval. Then, there exists a decreasing sequence {hj}j=1\{h_{j}\}_{j=1}^{\infty} with hj0+h_{j}\to 0+ (denoted as hh again) and uH1((0,T);L2(Ω))L((0,T);H01(Ω))u\in H^{1}((0,T);L^{2}(\Omega))\cap L^{\infty}((0,T);H^{1}_{0}(\Omega)) such that

uth\displaystyle u^{h}_{t} utweakly  in L((0,T);L2(Ω)),\displaystyle\rightharpoonup u_{t}\quad\hbox{weakly $*$ in\,\,}L^{\infty}((0,T);L^{2}(\Omega)), (18)
u¯h\displaystyle\nabla\overline{u}^{h} uweakly  in L((0,T);L2(Ω)),\displaystyle\rightharpoonup\nabla u\quad\hbox{weakly $*$ in\,\,}L^{\infty}((0,T);L^{2}(\Omega)), (19)
uh\displaystyle u_{h} uuniformly on [0,T)×Ω.\displaystyle\rightrightarrows u\quad\hbox{uniformly on\,\,}[0,T)\times\Omega. (20)

Moreover, uu is continuous on Ω×(0,T)\Omega\times(0,T), and satisfies the initial condition u(x,0)=u0(x)u(x,0)=u_{0}(x).

Proof. Rewriting the energy estimate (10) with u¯h\overline{u}^{h} and uhu^{h}, we have

uth(t)L2(Ω)2+u¯h(t)L2(Ω)2Cfor a.e.t(0,T),\|u^{h}_{t}(t)\|^{2}_{L^{2}(\Omega)}+\|\nabla\overline{u}^{h}(t)\|_{L^{2}(\Omega)}^{2}\leq C\quad\hbox{for a.e.}\,\,t\in(0,T), (21)

which together with the fact that uhu0u^{h}-u_{0} has zero trace on Ω\partial\Omega immediately implies (18) and (19). Regarding (20), we first prove the equicontinuity of the family {uh}\{u^{h}\} using (21) and the fact that, when Ω\Omega is an interval, for any fH01(Ω)f\in H^{1}_{0}(\Omega), we have

fL(Ω)CfL2(Ω)1/2fL2(Ω)1/2.\|f\|_{L^{\infty}(\Omega)}\leq C\|f\|_{L^{2}(\Omega)}^{1/2}\|f^{\prime}\|_{L^{2}(\Omega)}^{1/2}.

Indeed, for any t,s[0,T)t,s\in[0,T)

uh(t)uh(s)L(Ω)2\displaystyle\|u^{h}(t)-u^{h}(s)\|_{L^{\infty}(\Omega)}^{2} \displaystyle\leq Cuh(t)uh(s)L2(Ω)uh(t)uh(s)L2(Ω)\displaystyle C\|u^{h}(t)-u^{h}(s)\|_{L^{2}(\Omega)}\|\nabla u^{h}(t)-\nabla u^{h}(s)\|_{L^{2}(\Omega)}
\displaystyle\leq Cstuth(τ)L2(Ω)𝑑τ\displaystyle C\int_{s}^{t}\|u_{t}^{h}(\tau)\|_{L^{2}(\Omega)}\,d\tau
\displaystyle\leq C|ts|,\displaystyle C|t-s|,

and thus

|uh(b,t)uh(a,s)|\displaystyle|u^{h}(b,t)-u^{h}(a,s)| \displaystyle\leq |uh(b,t)uh(a,t)|+|uh(a,t)uh(a,s)|\displaystyle|u^{h}(b,t)-u^{h}(a,t)|+|u^{h}(a,t)-u^{h}(a,s)|
=\displaystyle= |abxuh(ξ,t)𝑑ξ|+|uh(a,t)uh(a,s)|\displaystyle\left|\int_{a}^{b}\frac{\partial}{\partial x}u^{h}(\xi,t)\,d\xi\right|+|u^{h}(a,t)-u^{h}(a,s)|
\displaystyle\leq uhL((0,T);L2(Ω))|ba|1/2+C|ts|1/2.\displaystyle\|\nabla u^{h}\|_{L^{\infty}((0,T);L^{2}(\Omega))}|b-a|^{1/2}+C|t-s|^{1/2}.

Moreover, the uniform boundedness of the family {uh}\{u^{h}\} follows as a by-product. Therefore, invoking the Ascoli-Arzelà theorem concludes the proof of (20).

The following lemma is needed to prove the existence of weak solutions.

Lemma 4.4

Under the assumption of Lemma 4.3, define w¯h(x,t):=0\overline{w}^{h}(x,t):=0 if t(0,h]t\in(0,h], and w¯h(x,t):=u¯h(t2h)\overline{w}^{h}(x,t):=\overline{u}^{h}(t-2h) when t(h,T)t\in(h,T). Then,

w¯huweakly  in L((0,T);L2(Ω)).\nabla\overline{w}^{h}\rightharpoonup\nabla u\quad\hbox{weakly $*$ in\,\,}L^{\infty}((0,T);L^{2}(\Omega)).

Proof. In the following argument, we omit the space variable xx for simplicity. We fix UL1((0,T);L2(Ω))U\in L^{1}((0,T);L^{2}(\Omega)) and extend it by zero outside of (0,T)(0,T). The extended function, denoted again by UU, belongs to L1((,);L2(Ω))L^{1}((-\infty,\infty);L^{2}(\Omega)). We calculate as follows:

|0Tw¯h(t),U(t)L2(Ω)𝑑t0Tu(t),U(t)L2(Ω)𝑑t|\displaystyle\Bigl{|}\int_{0}^{T}\langle\nabla\overline{w}^{h}(t),U(t)\rangle_{L^{2}(\Omega)}\,dt-\int_{0}^{T}\langle\nabla u(t),U(t)\rangle_{L^{2}(\Omega)}\,dt\Bigr{|}
=|hT2hu¯h(t),U(t+2h)𝑑t0Tu(t),U(t)𝑑t|\displaystyle=\Bigl{|}\int_{-h}^{T-2h}\langle\nabla\overline{u}^{h}(t),U(t+2h)\rangle\,dt-\int_{0}^{T}\langle\nabla u(t),U(t)\rangle\,dt\Bigr{|}
|0T2hu¯h(t),U(t+2h)U(t)𝑑t|\displaystyle\leq\Bigl{|}\int_{0}^{T-2h}\langle\nabla\overline{u}^{h}(t),U(t+2h)-U(t)\rangle\,dt\Bigr{|}
+|0Tu¯h(t)u(t),U(t)dt|+|T2hTu¯h(t)u(t),U(t)dt|\displaystyle\quad+\Bigl{|}\int_{0}^{T}\langle\nabla\overline{u}^{h}(t)-\nabla u(t),U(t)\rangle\,dt\Bigr{|}+\Bigl{|}\int_{T-2h}^{T}\langle\nabla\overline{u}^{h}(t)-\nabla u(t),U(t)\rangle\,dt\Bigr{|}
+|h0u¯h(t),U(t+2h)dt|+|T2hTu(t),U(t)dt|\displaystyle\quad+\Bigl{|}\int_{-h}^{0}\langle\nabla\overline{u}^{h}(t),U(t+2h)\rangle\,dt\Bigr{|}+\Bigl{|}\int_{T-2h}^{T}\langle\nabla u(t),U(t)\rangle\,dt\Bigr{|}
CU(t+2h)U(t)L2(Ω)𝑑t+|0Tu¯h(t)u(t),U(t)𝑑t|\displaystyle\leq C\int_{-\infty}^{\infty}\|U(t+2h)-U(t)\|_{L^{2}(\Omega)}\,dt+\Bigl{|}\int_{0}^{T}\langle\nabla\overline{u}^{h}(t)-\nabla u(t),U(t)\rangle\,dt\Bigr{|}
+CT2hTU(t)L2(Ω)𝑑t+Ch2hU(t)L2(Ω)𝑑t,\displaystyle\qquad+C\int_{T-2h}^{T}\|U(t)\|_{L^{2}(\Omega)}\,dt+C\int_{h}^{2h}\|U(t)\|_{L^{2}(\Omega)}\,dt, (22)

where the constant CC is independent of hh. Letting h0+h\to 0+, the second term converges to 0 by (19), and the remaining terms vanish thanks to the integrability of UU.

We now arrive at the following theorem:

Theorem 4.5 (Existence weak solutions to Problem 1)

Let Ω\Omega be a bounded domain in \mathbb{R}. Then Problem 1 has a weak solution in the sense of Definition 4.1.

Proof. The proof is similar to that in [12] and [5]. Without loss of generality, we can consider Ω=(0,1)\Omega=(0,1). By the definition of an approximate weak solution (17), we have

hTΩ(uth(t)uth(th)hφ+u¯h(t)+u¯h(t2h)2φ)𝑑x𝑑t=0\displaystyle\int_{h}^{T}\int_{\Omega}\left(\frac{u^{h}_{t}(t)-u^{h}_{t}(t-h)}{h}\varphi+\nabla\frac{\overline{u}^{h}(t)+\overline{u}^{h}(t-2h)}{2}\cdot\nabla\varphi\right)dxdt=0\quad
φ𝒞(u¯h):=C0(Ω×[0,T){u¯h>0}),\displaystyle\qquad\qquad\forall\varphi\in\mathcal{C}(\overline{u}^{h}):=C_{0}^{\infty}(\Omega\times[0,T)\cap\{\overline{u}^{h}>0\}),
uh0inΩ×(0,T){uh>0}.\displaystyle\qquad\qquad u^{h}\equiv 0\quad\mbox{\rm in}\quad\Omega\times(0,T)\setminus\{u^{h}>0\}. (23)

We fix ψ𝒞(u)\psi\in\mathcal{C}(u), where uu is obtained in Lemma 4.3. Since uu is continuous on Ω×(0,T)\Omega\times(0,T), there exists η>0\eta>0 such that uηu\geq\eta on sptψ\hbox{spt}\,\psi. By Lemma 4.3, the subsequence {uh}\{u^{h}\} converges to uu uniformly, and there exists h0>0h_{0}>0 such that

max(x,t)Ω×(0,T)|uh(x,t)u(x,t)|η2for allh<h0.\max_{(x,t)\in\Omega\times(0,T)}|u^{h}(x,t)-u(x,t)|\leq\frac{\eta}{2}\quad\hbox{for all}\,\,\,h<h_{0}.

Therefore, we have uhu|uhu|η/2u^{h}\geq u-|u^{h}-u|\geq\eta/2 on sptψ\hbox{spt}\,\,\psi for any h(0,h0)h\in(0,h_{0}). Note that u¯h(x,t)=uh(x,kh)\overline{u}^{h}(x,t)=u^{h}(x,kh) for any t((k1)h,kh]t\in((k-1)h,kh], and u¯hη/2>0\overline{u}^{h}\geq\eta/2>0 on spt ψ\psi for any h(0,h0)h\in(0,h_{0}). This implies that (23) holds for any test function φ𝒞(u)\varphi\in\mathcal{C}(u) whenever h<h0h<h_{0}. The time-discretized term can be rearranged as

hTuth(t)uth(th)hφ(t)𝑑t=hTuth(t)φ(t)φ(t+h)h𝑑t1h0huth(t)φ(t+h)𝑑t+1hThTuth(t)φ(t+h)𝑑t.\int_{h}^{T}\frac{u^{h}_{t}(t)-u^{h}_{t}(t-h)}{h}\varphi(t)\,dt=\int_{h}^{T}u_{t}^{h}(t)\frac{\varphi(t)-\varphi(t+h)}{h}\,dt\\ -\frac{1}{h}\int_{0}^{h}u_{t}^{h}(t)\varphi(t+h)\,dt+\frac{1}{h}\int_{T-h}^{T}u_{t}^{h}(t)\varphi(t+h)\,dt.

Hence, using Lemma 4.3 and Lemma 4.4, and passing to h0+h\to 0+ in (23), we obtain

0TΩ(utφt+uφ)𝑑x𝑑tΩv0φ(x,0)𝑑x=0φ𝒞(u),\int_{0}^{T}\int_{\Omega}\left(-u_{t}\varphi_{t}+\nabla u\cdot\nabla\varphi\right)dxdt-\int_{\Omega}v_{0}\varphi(x,0)dx=0\qquad\forall\varphi\in\mathcal{C}(u),

which was our goal.

Remark 2

Note that the fact that (23) holds for any test function φ\varphi compactly supported in the support of the limit function uu, is a consequence of the uniform convergence of the approximating sequence {uh}\{u^{h}\}, which was in turn obtained thanks to Ascoli-Arzelà theorem through an imbedding argument. However, this imbedding is available only in spatial dimension 1, restricting our existence result. We are not aware of any method to extend this limit passage relying on imbedding theorems, except for the recent results in [1, 2], where a different definition of weak solution through the subsolution property allows proving existence in arbitrary dimension. Nevertheless, the good point of our strategy, common to [1, 2], is that a uniform estimate is available for the approximations and hence a unique limit function can be identified. The open question is how much can be said about this limit. On the other hand, the energy-preserving property of our approximation scheme could be exploited not only numerically in building robust numerical algorithms, but also theoretically in proving uniqueness of solutions for certain wave-types problems. The existing analyses using variational approach were not successful in proving uniqueness, and hence investigating the new scheme from this viewpoint presents an interesting direction for future research.

Remark 3

As a remark concluding this section, we present formal ideas on a possible approach to deal with the free boundary condition. For this purpose we generalize Problem 1 to the setting of a hyperbolic free boundary problem with an adhesion term, which delineates the role of the free boundary condition and is of interest in applications. We calculate the first variation of the following action integral:

J(u):=0TΩ((ut)2χ{u>0}|u|2Q2χ{u>0})𝑑x𝑑tJ(u):=\int_{0}^{T}\int_{\Omega}\Bigl{(}(u_{t})^{2}\chi_{\{u>0\}}-|\nabla u|^{2}-Q^{2}\chi_{\{u>0\}}\Bigr{)}\,dx\,dt

where QQ is a constant which expresses the adhesion force. When energy is conserved, i.e., when the function uu does not change its value from positive to zero as time passes, we can, under appropriate assumptions, calculate the first variation, as well as the inner variation, of the functional JJ. However, if energy is not conserved, we can calculate neither the first variation nor the inner variation due to the presence of the Q2Q^{2}-term containing the characteristic function. To overcome this difficulty, we consider a smoothing of the characteristic function within the adhesion term by a function BεB_{\varepsilon} defined by Bε(u)=1uβε(s)𝑑sB_{\varepsilon}(u)=\int_{-1}^{u}\beta_{\varepsilon}(s)\,ds, where βε(u):=1εβ(uε)\beta_{\varepsilon}(u):=\frac{1}{\varepsilon}\beta(\frac{u}{\varepsilon}), and β:[0,1]\beta:\mathbb{R}\to[0,1] is a smooth function satisfying β=0\beta=0 outside [1,1][-1,1], β(s)𝑑s=1\int_{\mathbb{R}}\beta(s)\,ds=1, and B(0)=12B(0)=\frac{1}{2}. After smoothing, we can calculate the first variation to obtain an expression for the following problem:

(Pε){χ{u>0}¯utt=Δu12Q2βε(u)inΩ×(0,T),u(x,0)=u0(x)inΩ,ut(x,0)=v0(x)inΩ,u(x,t)|Ω=ψ(x,t)withψ(x,0)=u0onΩ,(\hbox{P}_{\varepsilon})\begin{cases}\chi_{\overline{\{u>0\}}}\,u_{tt}&=\Delta u-\frac{1}{2}Q^{2}\beta_{\varepsilon}(u)\quad\hbox{in}\,\,\Omega\times(0,T),\\ u(x,0)&=u_{0}(x)\quad\hbox{in}\,\,\Omega,\\ u_{t}(x,0)&=v_{0}(x)\quad\hbox{in}\,\,\Omega,\\ u(x,t)|_{\partial\Omega}&=\psi(x,t)\,\,\hbox{with}\,\,\psi(x,0)=u_{0}\,\,\,\hbox{on}\,\,\partial\Omega,\end{cases}

where u0,v0u_{0},v_{0} are the same as in Problem 1, and ψ\psi is a given function. Now, we set the following hypotheses:

(H1)

The existence of a solution uεu_{\varepsilon} to (Pε)(\hbox{P}_{\varepsilon}).

(H2)

The existence of a function u:Ω×(0,T)u:\Omega\times(0,T)\to\mathbb{R} such that uεuu_{\varepsilon}\to u in an appropriate topology as ε0\varepsilon\downarrow 0 and such that the following holds:

(H2.1)

uttΔu=0u_{tt}-\Delta u=0 in Ω×(0,T){u>0}\Omega\times(0,T)\cap\{u>0\}.

(H2.2)

The free boundary {u>0}\partial\{u>0\} is regular, N(𝒟{u>0})<\mathscr{H}^{N}(\mathcal{D}\cap\partial\{u>0\})<\infty for any 𝒟Ω×(0,T)N×(0,T)\mathcal{D}\subset\subset\Omega\times(0,T)\subset\mathbb{R}^{N}\times(0,T), and |Du|0|Du|\not=0 on Ω×(0,T){u>0}\Omega\times(0,T)\cap\partial\{u>0\}. Here, Du=(ux1,,uxN,ut)Du=(u_{x_{1}},...,u_{x_{N}},u_{t}), and N\mathscr{H}^{N} is the NN-dimensional Hausdorff measure.

(H2.3)

uu is a subsolution in the following sense:

0TΩ(χ{u>0}¯uttζ+uζ)dxdt0\int_{0}^{T}\int_{\Omega}\Bigl{(}\chi_{\overline{\{u>0\}}}\,\,u_{tt}\,\zeta+\nabla u\cdot\nabla\zeta\Bigl{)}\,dx\,dt\leq 0

for arbitrary nonnegative ζC0(Ω×(0,T))\zeta\in C_{0}^{\infty}(\Omega\times(0,T)).

Starting from (Pε)(\hbox{P}_{\varepsilon}), and employing (H1), (H2.1) and (H2.2), we can show that the limit function uu satisfies the following free boundary condition [11]:

|u|2ut2=Q2onΩ×(0,T){u>0}.|\nabla u|^{2}-u_{t}^{2}=Q^{2}\quad\hbox{on}\,\,\,\Omega\times(0,T)\cap\partial\{u>0\}. (24)

Now, for any 𝒟Ω×(0,T)\mathcal{D}\subset\subset\Omega\times(0,T), we define a linear functional ff on C0(𝒟)C_{0}^{\infty}(\mathcal{D}) corresponding to Δuχ{u>0}¯utt\Delta u-\chi_{\overline{\{u>0\}}}\,u_{tt} as follows:

f(ζ):=𝒟(χ{u>0}¯uttζ+uζ)𝑑x𝑑t.f(\zeta):=-\int_{\mathcal{D}}\Bigl{(}\chi_{\overline{\{u>0\}}}\,\,u_{tt}\,\zeta+\nabla u\cdot\nabla\zeta\Bigr{)}\,dx\,dt.

Since ff is a positive linear functional on C0(𝒟)C_{0}^{\infty}(\mathcal{D}) by (H2.3), ff can be extended to a positive linear functional on C0(𝒟)C_{0}(\mathcal{D}). Riesz’s representation theorem asserts there exists a unique positive Radon measure μf\mu_{f} on 𝒟\mathcal{D} such that f(ζ)=𝒟ζ𝑑μff(\zeta)=\int_{\mathcal{D}}\zeta\,d\mu_{f}. In this sense, we can say that Δuχ{u>0}¯utt\Delta u-\chi_{\overline{\{u>0\}}}\,\,u_{tt} is a positive Radon measure on 𝒟\mathcal{D}.

On the other hand, we can calculate the value of f(ζ)f(\zeta) from (24). By splitting the integral domain into four parts, 𝒟{u>0}\mathcal{D}\cap\{u>0\}, 𝒟{u>0}\mathcal{D}\cap\partial\{u>0\}, 𝒟{u=0}\mathcal{D}\cap\partial\{u=0\}^{\circ}, 𝒟{u=0}\mathcal{D}\cap\{u=0\}^{\circ}, noting that all terms vanish except for 𝒟{u>0}\mathcal{D}\cap\partial\{u>0\} by the integration by parts, and χ{u>0}¯=1\chi_{\overline{\{u>0\}}}=1 on {u>0}\partial\{u>0\}, we get

𝒟(χ{u>0}¯uttζ+uζ)𝑑x𝑑t=𝒟((χ{u>0}¯ζ)tut+uζ)𝑑x𝑑t\displaystyle\int_{\mathcal{D}}\left(\chi_{\overline{\{u>0\}}}\,\,u_{tt}\zeta+\nabla u\cdot\nabla\zeta\right)\,dx\,dt=\int_{\mathcal{D}}\left(-(\chi_{\overline{\{u>0\}}}\,\,\zeta)_{t}u_{t}+\nabla u\cdot\nabla\zeta\right)\,dx\,dt
=𝒟{u>0}(χ{u>0}¯ζutut|Du|+ζuu|Du|)dN\displaystyle=\int_{\mathcal{D}\cap\partial\{u>0\}}-\Bigl{(}\chi_{\overline{\{u>0\}}}\,\,\zeta\cdot u_{t}\cdot\frac{-u_{t}}{|Du|}+\zeta\nabla u\cdot\frac{-\nabla u}{|Du|}\Bigr{)}\,d\mathscr{H}^{N}
=𝒟{u>0}ut2|u|2|Du|ζ𝑑N=𝒟{u>0}Q2|Du|ζ𝑑N(by(24)).\displaystyle=\int_{\mathcal{D}\cap\partial\{u>0\}}\frac{u_{t}^{2}-|\nabla u|^{2}}{|Du|}\,\,\zeta\,d\mathscr{H}^{N}=\int_{\mathcal{D}\cap\partial\{u>0\}}\frac{-Q^{2}}{|Du|}\,\,\zeta\,d\mathscr{H}^{N}\quad(\hbox{by}\,\,\,(\ref{free_boundary_cond})).

From the above and the definition of ff, we observe that

μf=Q2|Du|N{u>0}.\mu_{f}=\frac{Q^{2}}{|Du|}\mathscr{H}^{N}\lfloor\partial\{u>0\}. (25)

In this sense, the positive Radon measure Δuχ{u>0}¯utt\Delta u-\chi_{\overline{\{u>0\}}}\,\,u_{tt} has its support in the free boundary {u>0}\partial\{u>0\}. Formally, we can rewrite (25) as follows:

χ{u>0}¯uttΔu=Q2|Du|N{u>0}.\chi_{\overline{\{u>0\}}}\,u_{tt}-\Delta u=-\frac{Q^{2}}{|Du|}\mathscr{H}^{N}\lfloor\partial\{u>0\}. (26)

Summarizing the above, starting from the smoothed problem (PεP_{\varepsilon}), under the hypotheses (H1)-(H2), we formally derive a hyperbolic degenerate equation with adhesion force. This equation (26) includes all information about the hyperbolic free boundary problem, that is, the wave equation uttΔu=0u_{tt}-\Delta u=0 in the set {u>0}\{u>0\}, the free boundary condition |u|2ut2=Q2|\nabla u|^{2}-u_{t}^{2}=Q^{2} on Ω×(0,T){u>0}\Omega\times(0,T)\cap\partial\{u>0\}, and the Laplace equation Δu=0\Delta u=0 in the set {u<0}\{u<0\} a.e. t(0,T)t\in(0,T).

5 Numerical Results

5.1 Numerical analysis of the one-dimensional problem

In this section, we present several numerical results for the equation (1) obtained by the minimization of the Crank-Nicolson type functional

Jm(u):=\displaystyle J_{m}(u):= Ω({u>0}{um1>0}{um2>0})|u2um1+um2|22h2𝑑x\displaystyle\int_{\Omega\cap(\{u>0\}\cup\{u_{m-1}>0\}\cup\{u_{m-2}>0\})}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\,dx
+14Ω|u+um2|2𝑑x.\displaystyle\qquad+\frac{1}{4}\int_{\Omega}|\nabla u+\nabla u_{m-2}|^{2}\,dx.

and compare them with results due to the original discrete Morse flow method of [10], which uses the functional

J~m(u):=Ω({u>0}{um1>0})|u2um1+um2|22h2𝑑x+12Ω|u|2𝑑x.\widetilde{J}_{m}(u):=\int_{\Omega\cap(\{u>0\}\cup\{u_{m-1}>0\})}\frac{|u-2u_{m-1}+u_{m-2}|^{2}}{2h^{2}}\,dx+\frac{1}{2}\int_{\Omega}|\nabla u|^{2}\,dx.

In the numerical calculation, we simply use the functional ImI_{m} without the restriction of the integration domain and the corresponding functional I~m\widetilde{I}_{m} for the original discrete Morse flow method. Subsequently, for a minimizer u~m,m2\widetilde{u}_{m},\,m\geq 2, of ImI_{m} or I~m\widetilde{I}_{m}, we define

um:=max{u~m,0}.u_{m}:=\max\{\widetilde{u}_{m},0\}.

We regard umu_{m} as a numerical solution at time level t=mht=mh. The minimization problems are discretized by the finite element method, where the approximate minimizer is a continuous function over the domain and piece-wise linear over each element.

In the one-dimensional case, equation (1) has been employed in describing the dynamics of a string hitting a plane with zero reflection constant. In two dimensions, the graph of the solution may be considered as representing a soap film touching a water surface. Another important application of this model is the volume constrained problem describing the motion of scalar droplets over a flat surface (see, e.g., [5], and Section 5.2).

Having in mind the model of a string hitting an obstacle, let us first consider problem (1) in the open interval Ω=(0,1)\Omega=(0,1), with the initial condition

u0(x):={4x+0.2 if 0x<1/4,43(x1)+0.2 otherwise ,u_{0}(x):=\left\{\begin{aligned} &4x+0.2&&\text{ if }0\leq x<1/4,\\ &-\frac{4}{3}(x-1)+0.2&&\text{ otherwise },\end{aligned}\right.

and v00v_{0}\equiv 0. Figure 1 shows the behavior of the numerical solution for both methods. For the Crank-Nicolson method, the corners in the graph of the solution are kept, even as time progresses. This is not the case for the discrete Morse flow method, where corners are smoothed.

Refer to caption
Refer to caption
Refer to caption
Refer to caption
Figure 1: Numerical solution at four distinct times for the Crank-Nicolson method (blue) and the original discrete Morse flow method (red). The time step size is h=1.0×104h=1.0\times 10^{-4} and the spacial mesh size is Δx=h\Delta x=h.

Figure 2 shows that the free boundary condition (2) is satisfied when the string peels off the obstacle.

Refer to caption
Figure 2: Free boundary corresponding to the motion in Figure 1. The curves are obtained by plotting the boundary of the set {(t,x);u(x,t)<ε}\{(t,x);u(x,t)<\varepsilon\} for a small ε>0\varepsilon>0.

Figure 3 shows that the energy is lost when the string touches the obstacle, while the energy is preserved before and after the contact of the string with the obstacle. For the sake of comparison, we note that the energy of the solution obtained by discrete Morse flow decays even during the non-contact stage.

Refer to caption
Figure 3: Evolution of the energy of the numerical solution for both methods.

To test the energy decay tendency of both methods, we solved the problem without free boundary with the initial condition u0=sin(2nπx)u_{0}=\sin(2n\pi x), and v00v_{0}\equiv 0. It was found that, for the original discrete Morse flow, energy decay becomes prominent with decreasing time resolution and increasing wave frequency. On the other hand, as can be observed in Figure 4, the Crank-Nicolson method preserves energy independent of the time resolution and wave frequency.

Refer to caption
Figure 4: Comparison of energy decay tendency for both methods using the initial data u0=sin(2nπx)u_{0}=\sin(2n\pi x) and v00v_{0}\equiv 0. Here, Δx=h\Delta x=h is used.

Although the Crank-Nicolson method displays excellent energy-preserving properties, it appears to include an incorrect phase-shift, as is the case with the original discrete Morse flow. We summarize the features of both methods in Table 1.

C-N DMF
energy conserved decays
free boundary condition holds holds
high harmonic wave preserved decays
including constraints possible possible
phase shift occurs occurs
Table 1: Main features of the two methods compared in this section.

5.2 Higher dimensions and more general problems

In this section, we investigate the energy preservation properties of the proposed scheme in the two dimensional setting. In particular, the functional (4) is used to approximate a solution of the wave equation with initial conditions u0(x,y)=sin(πx)sin(πy),v0(x,y)=0u_{0}(x,y)=\sin(\pi x)\sin(\pi y),v_{0}(x,y)=0 and Dirichlet zero boundary condition, where the domain Ω=(0,1)×(0,1)\Omega=(0,1)\times(0,1).

The functional value corresponding to a given function uu is approximated using P1P_{1} finite elements, and the functional minimization is performed using a steepest descent algorithm. Here Ω\Omega has been uniformly partitioned into N=5684N=5684 elements.

Using several different values of the time step h,h, we compared the energy of the numerical solution obtained using the Crank-Nicolson scheme with that obtained from the standard discrete Morse flow. The total energy is computed using the finite element method on the functional:

nh(u)=Ω(12|uun1h|2+|u|22)𝑑x.\displaystyle\mathcal{E}^{h}_{n}(u)=\int_{\Omega}\Bigl{(}\frac{1}{2}\left|\frac{u-u_{n-1}}{h}\right|^{2}+\frac{|\nabla u|^{2}}{2}\Bigr{)}\,dx. (27)

The results are shown in Figure 5, where the time steps were h=0.0005+0.005×kh=0.0005+0.005\times k, k=0,1,2,3,4,5k=0,1,2,3,4,5. Our results confirm the energy preservation properties of the proposed scheme.

Refer to caption
Figure 5: Comparison of the Crank-Nicolson scheme with the original discrete Morse flow for a 2-dimensional problem.

We have also used the proposed method to investigate the numerical solution of a more complicated model equation describing droplet motions.

Refer to caption
Figure 6: Crank-Nicolson type minimizing movement approximation of droplet motion, with the free boundary illustrated as the black curves.. Time is designated by the integer values within the figure, so that the initial condition corresponds to number 1 and all graphs are plotted at equal time intervals, except for the last one showing the stationary state reached after sufficiently long time.

The target equations correspond to volume constrained formulations of the original problem. In particular, volume and non-negativity constraints are added to the functionals by means of indicator functions:

𝒥mi(u)=Ω(|u2um1i+um2i|22h2+14|ui+um2i|2+)𝑑x+Ψ1(u)+Ψ2i,m(u),\mathcal{J}^{i}_{m}(u)=\int_{\Omega}\left(\frac{|u-2u^{i}_{m-1}+u^{i}_{m-2}|^{2}}{2h^{2}}+\frac{1}{4}|\nabla u^{i}+\nabla u^{i}_{m-2}|^{2}+\right)dx\\ +\Psi_{1}(u)+\Psi^{i,m}_{2}(u),

where each indicator function is defined as follows:

Ψ1(u)\displaystyle\Psi_{1}(u) ={0,if u(x)0 for N-a.e. xΩ,otherwise,\displaystyle={\begin{cases}{0,}&\text{if }{u(x)\geq 0\text{ for }\mathcal{L}^{N}\text{-a.e. }x\in\Omega}\\ {\infty,}&{\text{otherwise}}\\ \end{cases}},
Ψ2i,m(u)\displaystyle\Psi_{2}^{i,m}(u) ={0,if Ωu(x)𝑑x=Vmi,otherwise.\displaystyle={\begin{cases}{0,}&\text{if }{\int_{\Omega}u(x)dx=V^{i}_{m}}\\ {\infty,}&{\text{otherwise.}}\\ \end{cases}}

Here VmiV^{i}_{m} denotes the volume of droplet ii at time step mm.

By minimizing functionals 𝒥mi\mathcal{J}_{m}^{i} for each droplet, we are able to compute approximate solutions to the volume constrained problem. The results are shown in Figure 6. For each ii, the initial condition is prescribed as a collection of spherical caps, and we observe the droplets oscillate while coalescing into larger groups.

6 Conclusions

We have shown the existence of weak solutions to a hyperbolic free boundary problem by minimizing a Crank-Nicolson type functional in the one-dimensional setting. This new functional was shown to preserve the energy correctly both on continuous and discrete levels, which is of significance in both theoretical analysis and numerical simulations. Future tasks include extending our result to higher dimensions and to developing computational methods for investigating the numerical properties of the free boundary problem.

Acknowledgments

E. Ginder would like to acknowledge the support of JSPS Kakenhi Grant number 17K14229. The research of the fourth author was partially funded by a joint research project with YKK Corporation. The research of the last author was supported by JSPS Kakenhi Grant numbers 19K03634 and 18H05481. We would also like to thank the anonymous referees for their constructive comments.

References

  • [1] (MR3973177) M. Bonafini, M. Novaga and G. Orlandi, A variational scheme for hyperbolic obstacle problems, Nonlin. Anal., 188 (2019), 389–404.
  • [2] M. Bonafini, V.P.C. Le, M. Novaga and G. Orlandi, On the obstacle problem for fractional semilinear wave equations, preprint, arXiv2011.02246.
  • [3] (MR2165387) X. Chen, S. Cui and A. Friedman, A hyperbolic free boundary problem modeling tumor growth: asymptotic behavior, Trans. Am. Math. Soc., 357 (2005), 4771–4804.
  • [4] M. Giaquinta, Multiple Integrals in the Calculus of Variations and Nonlinear Elliptic Systems, Princeton University Press, 1983.
  • [5] (MR2671935) E. Ginder and K. Svadlenka, A variational approach to a constrained hyperbolic free boundary problem, Nonlinear Anal., 71 (2009), e1527–e1537.
  • [6] (MR4226659) T. Iguchi and D. Lannes, Hyperbolic free boundary problems and applications to wave-structure interactions, preprint, arXiv1806.07704.
  • [7] K. Kikuchi, Constructing a solution in time semidiscretization method to an equation of vibrating string with an obstacle, Nonlinear Anal., 71 (2009), 1227–1232.
  • [8] (MR1725685) K. Kikuchi and S. Omata, A free boundary problem for a one dimensional hyperbolic equation, Adv. Math. Sci. Appl., 9 (1999), 775–786.
  • [9] O. Ladyzhenskaya and N. Uraltseva, Linear and Quasilinear Elliptic Equations, 1st edition, Academic Press, 1968.
  • [10] (MR2083621) S. Omata, A numerical treatment of film motion with free boundary, Adv. Math. Sci. Appl., 14 (2004), 129–137.
  • [11] (MR3746196) S. Omata, A hyperbolic obstacle problem with an adhesion force, in Mathematics for Nonlinear Phenomena-Analysis and Computation (eds Y. Maekawa and S. Jimbo), Springer Proceedings in Mathematics and Statistics, 215 (2017), 261–269.
  • [12] K. Svadlenka and S. Omata, Mathematical modeling of surface vibration with volume constraint and its analysis, Nonlinear Anal., 69 (2008), 3202–3212.
  • [13] (MR2253223) H. Yoshiuchi, S. Omata, K. Svadlenka and K. Ohara, Numerical solution of film vibration with obstacle, Adv. Math. Sci. Appl., 16 (2006), 33–43.