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Free boundary problem

From Wikipedia, the free encyclopedia
Type of partial differential equation

Inmathematics, afree boundary problem (FB problem) is apartial differential equation to be solved for both an unknown functionu{\displaystyle u} and an unknowndomainΩ{\displaystyle \Omega }. The segmentΓ{\displaystyle \Gamma } of theboundary ofΩ{\displaystyle \Omega } which is not known at the outset of the problem is thefree boundary.

FBs arise in various mathematical models encompassing applications that ranges from physical to economical, financial and biological phenomena, where there is an extra effect of the medium. This effect is in general a qualitative change of the medium and hence an appearance of aphase transition: ice to water, liquid to crystal, buying to selling (assets), active to inactive (biology), blue to red (coloring games), disorganized to organized (self-organizing criticality). An interesting aspect of such a criticality is the so-called sandpile dynamic (or Internal DLA).

The most classical example is the melting of ice: Given a block of ice, one can solve theheat equation given appropriate initial andboundary conditions to determine its temperature. But, if in any region the temperature is greater than the melting point of ice, this domain will be occupied by liquid water instead. The boundary formed from the ice/liquid interface is controlled dynamically by the solution of the PDE.

Another famous example of a free boundary problem appearing in a different context is that of the valuation ofAmerican options. Because the timing of the exercise is not fixed, unlike for European options, the effective strike price takes the form of a free boundary that must be solved as part of the valuation process.

Two-phase Stefan problems

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The melting of ice is aStefan problem for the temperature fieldT{\displaystyle T}, which is formulated as follows. Consider a medium occupying a regionΩ{\displaystyle \Omega } consisting of two phases, phase 1 which is present whenT>0{\displaystyle T>0} and phase 2 which is present whenT<0{\displaystyle T<0}. Let the two phases havethermal diffusivitiesα1{\displaystyle \alpha _{1}} andα2{\displaystyle \alpha _{2}}. For example, the thermal diffusivity of water is 1.4×10−7 m2/s, while the diffusivity of ice is 1.335×10−6 m2/s.

In the regions consisting solely of one phase, the temperature is determined by the heat equation: in the regionT>0{\displaystyle T>0},

Tt=(α1T)+Q{\displaystyle {\frac {\partial T}{\partial t}}=\nabla \cdot (\alpha _{1}\nabla T)+Q}

while in the regionT<0{\displaystyle T<0},

Tt=(α2T)+Q.{\displaystyle {\frac {\partial T}{\partial t}}=\nabla \cdot (\alpha _{2}\nabla T)+Q.}

This is subject to appropriate conditions on the (known) boundary ofΩ{\displaystyle \Omega };Q{\displaystyle Q} represents sources or sinks of heat.

LetΓt{\displaystyle \Gamma _{t}} be the surface whereT=0{\displaystyle T=0} at timet{\displaystyle t}; this surface is the interface between the two phases. Letν{\displaystyle \nu } denote the unit outward normal vector to the second (solid) phase. TheStefan condition determines the evolution of the surfaceΓ{\displaystyle \Gamma } by giving an equation governing the velocityV{\displaystyle V} of the free surface in the directionν{\displaystyle \nu }, specifically

LV=α1νT1α2νT2,{\displaystyle LV=\alpha _{1}\partial _{\nu }T_{1}-\alpha _{2}\partial _{\nu }T_{2},}

whereL{\displaystyle L} is the latent heat of melting. ByT1{\displaystyle T_{1}} we mean the limit of the gradient asx{\displaystyle x} approachesΓt{\displaystyle \Gamma _{t}} from the regionT>0{\displaystyle T>0}, and forT2{\displaystyle T_{2}} we mean the limit of the gradient asx{\displaystyle x} approachesΓt{\displaystyle \Gamma _{t}} from the regionT<0{\displaystyle T<0}.

In this problem, we know beforehand the whole regionΩ{\displaystyle \Omega } but we only know the ice-liquid interfaceΓ{\displaystyle \Gamma } at timet=0{\displaystyle t=0}. To solve the Stefan problem we not only have to solve the heat equation in each region, but we must also track the free boundaryΓ{\displaystyle \Gamma }.

The one-phase Stefan problem corresponds to taking eitherα1{\displaystyle \alpha _{1}} orα2{\displaystyle \alpha _{2}} to be zero; it is a special case of the two-phase problem. In the direction of greater complexity we could also consider problems with an arbitrary number of phases.

Obstacle problems

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Another famous free-boundary problem is theobstacle problem, which bears close connections to the classicalPoisson equation. The solutions of the differential equation

2u=f,u|Ω=g{\displaystyle -\nabla ^{2}u=f,\qquad u|_{\partial \Omega }=g}

satisfy a variational principle, that is to say they minimize the functional

E[u]=12Ω|u|2dxΩfudx{\displaystyle E[u]={\frac {1}{2}}\int _{\Omega }|\nabla u|^{2}\,\mathrm {d} x-\int _{\Omega }fu\,\mathrm {d} x}

over all functionsu{\displaystyle u} taking the valueg{\displaystyle g} on the boundary. In the obstacle problem, we impose an additional constraint: we minimize the functionalE{\displaystyle E} subject to the condition

uφ{\displaystyle u\leq \varphi \,}

inΩ{\displaystyle \Omega }, for some given functionφ{\displaystyle \varphi }.

Define the coincidence setC as the region whereu=φ{\displaystyle u=\varphi }. Furthermore, define the non-coincidence setN=ΩC{\displaystyle N=\Omega \setminus C} as the region whereu{\displaystyle u} is not equal toφ{\displaystyle \varphi }, and the free boundaryΓ{\displaystyle \Gamma } as the interface between the two. Thenu{\displaystyle u} satisfies the free boundary problem

2u=f in N,u=g{\displaystyle -\nabla ^{2}u=f{\text{ in }}N,\quad u=g}

on the boundary ofΩ{\displaystyle \Omega }, and

uφ in |Ω,u=φ on Γ.{\displaystyle u\leq \varphi {\text{ in }}|\Omega ,\quad \nabla u=\nabla \varphi {\text{ on }}\Gamma .\,}

Note that the set of all functionsv{\displaystyle v} such thatvφ{\displaystyle v\leq \varphi } is convex. Where the Poisson problem corresponds to minimization of a quadratic functional over alinear subspace of functions, the free boundary problem corresponds to minimization over aconvex set.

Connection with variational inequalities

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Many free boundary problems can profitably be viewed asvariational inequalities for the sake of analysis. To illustrate this point, we first turn to the minimization of a functionF{\displaystyle F} ofn{\displaystyle n} real variables over a convex setC{\displaystyle C}; the minimizerx{\displaystyle x} is characterized by the condition

F(x)(yx)0 for all yC.{\displaystyle \nabla F(x)\cdot (y-x)\geq 0{\text{ for all }}y\in C.\,}

Ifx{\displaystyle x} is in the interior ofC{\displaystyle C}, then the gradient ofF{\displaystyle F} must be zero; ifx{\displaystyle x} is on the boundary ofC{\displaystyle C}, the gradient ofF{\displaystyle F} atx{\displaystyle x} must be perpendicular to the boundary.

The same idea applies to the minimization of a differentiable functionalF{\displaystyle F} on a convex subset of aHilbert space, where the gradient is now interpreted as a variational derivative. To concretize this idea, we apply it to the obstacle problem, which can be written as

Ω(2u+f)(vu)dx0 for all vφ.{\displaystyle \int _{\Omega }(\nabla ^{2}u+f)(v-u)\,\mathrm {d} x\geq 0{\text{ for all }}v\leq \varphi .}

This formulation permits the definition of a weak solution: usingintegration by parts on the last equation gives that

Ωu(vu)dxΩf(vu)dx for all vφ.{\displaystyle \int _{\Omega }\nabla u\cdot \nabla (v-u)\mathrm {d} x\leq \int _{\Omega }f(v-u)\,\mathrm {d} x{\text{ for all }}v\leq \varphi .}

This definition only requires thatu{\displaystyle u} have one derivative, in much the same way as the weak formulation of elliptic boundary value problems.

Regularity of free boundaries

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In the theory ofelliptic partial differential equations, one demonstrates the existence of aweak solution of a differential equation with reasonable ease using somefunctional analysis arguments. However, the weak solution exhibited lies in a space of functions with fewer derivatives than one would desire; for example, for the Poisson problem, we can easily assert that there is a weak solution which is inH1{\displaystyle H^{1}}, but it may not have second derivatives. One then applies some calculus estimates to demonstrate that the weak solution is in fact sufficiently regular.

For free boundary problems, this task is more formidable for two reasons. For one, the solutions often exhibit discontinuous derivatives across the free boundary, while they may be analytic in any neighborhood away from it. Secondly, one must also demonstrate the regularity of the free boundary itself. For example, for the Stefan problem, the free boundary is aC1/2{\displaystyle C^{1/2}} surface.

Related Problems

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From a purely academic point of view free boundaries belong to a larger class of problems usually referred to as overdetermined problems, or asDavid Kinderlehrer andGuido Stampacchia addressed it in their book: The problem of matching Cauchy data. Other related FBP that can be mentioned are Pompeiu problem, Schiffer’s conjectures. See the external links below.

Another approach used to model similar problems is thePhase-field model.

References

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  • Alexiades, Vasilios (1993),Mathematical Modeling of Melting and Freezing Processes, Hemisphere Publishing Corporation,ISBN 1-56032-125-3
  • Friedman, Avner (1982),Variational Principles and Free Boundary Problems, John Wiley and Sons, Inc.,ISBN 978-0-486-47853-1
  • Kinderlehrer, David; Stampacchia, Guido (1980),An Introduction to Variational Inequalities and Their Applications, Academic Press,ISBN 0-89871-466-4
  • Caffarelli, Luis; Salsa, Sandro (2005),A geometric approach to free boundary problems. Graduate Studies in Mathematics, American Mathematical Society, Providence, RI,ISBN 0-8218-3784-2
  • Petrosyan, Arshak; Shahgholian, Henrik; Uraltseva, Nina (2012),Regularity of Free Boundaries in Obstacle-Type Problems. Graduate Studies in Mathematics, American Mathematical Society, Providence, RI,ISBN 978-0-8218-8794-3
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