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Let $\Omega$ be a domain with smooth boundary $\partial \Omega$, $\bar{\Omega}$ is compact.

The Neumann problem:$f \in C^{\infty}(\bar{\Omega})$,$g\in C^{\infty}(\partial \bar{\Omega})$. Find a function $\varphi \in C^{\infty}(\bar{\Omega})$ satisfying $\Delta \varphi=f$ on $\bar{\Omega}$ and $\frac{\partial}{\partial \overrightarrow{n}}\varphi=g$ on $\partial \bar{\Omega}$. ($\Delta$ is the Laplace operator, $\overrightarrow{n}$ is the unit normal vector field.)

How to prove the Neumann problem has a solution if and only if $\int_{\bar\Omega}{fdx}=\int_{\partial \bar{\Omega}}{gdS}$ ?

Maybe I can solve the case of $g=0$.

notime
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1 Answers1

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Edit: I have changed the proof of the \eqref{cc}$ \implies $\eqref{np} to correct an error in the reasoning pointed out by the asker. The development is now necessarily more complicated but entirely correct. I'd like to thank Prof. Alberto Cialdea for the useful discussion on the topic and the suggestion to use Fredholm theory and the equivalent Neumann problem for the Laplace equation.


What we want to prove is that the following Neumann problem $$ \color{green}{ \begin{cases} \Delta \varphi(x)=f(x) & x\in\bar{\Omega}\\ \frac{\partial}{\partial \vec{n}}\varphi(x)=g(x)& x\in\partial\bar{\Omega} \end{cases}\label{np}\tag{NP}} $$ is solvable if and only if the following compatibility condition $$ \color{blue}{ \int\limits_\bar{\Omega}f(x)\mathrm{d}x=\int\limits_{\partial\bar{\Omega}}g(x)\mathrm{d}\sigma_x. \label{cc}\tag{CC}} $$ holds (with obvious meaning of the symbols), i.e. \eqref{np}$ \iff $\eqref{cc}. Let's proceed with proving the two opposite implications.

  1. \eqref{np}$ \implies $\eqref{cc}. Integrating on the domain $\bar{\Omega}$ both members of the Poisson equation $\Delta \varphi=f$ from \eqref{np} we get: $$ \int\limits_\bar{\Omega}\Delta \varphi(x)\mathrm{d}x=\int\limits_\bar{\Omega}f(x)\mathrm{d}x. \label{1}\tag{1} $$ Now, remembering that $\Delta=\nabla\cdot\nabla=\operatorname{div}\operatorname{grad}$ and applying the Gauss-Green (divergence) theorem and the Neumann boundary condition from \eqref{np} to the first side of equation \eqref{1}, we have $$ \begin{split} \int\limits_\bar{\Omega}\Delta \varphi(x)\mathrm{d}x &=\int\limits_\bar{\Omega}\nabla\cdot\nabla \varphi(x)\mathrm{d}x = \int\limits_{\partial\bar{\Omega}}\nabla \varphi(x)\cdot\vec{n}_x\mathrm{d}\sigma_x \\ &= \int\limits_{\partial\bar{\Omega}}\frac{\partial}{\partial \vec{n}}\varphi(x)\mathrm{d}\sigma_x = \int\limits_{\partial\bar{\Omega}}g(x)\mathrm{d}\sigma_x, \end{split} $$ thus $$ \int\limits_\bar{\Omega}\Delta \varphi(x)\mathrm{d}x=\int\limits_{\partial\bar{\Omega}}g(x)\mathrm{d}\sigma_x, \label{2}\tag{2} $$ and this implies condition \eqref{cc}.
  2. \eqref{cc}$ \implies $\eqref{np}. Perhaps the easiest (and classical) way to prove this step is to transform problem \eqref{np} into a Fredholm integral equation of the second kind, and verify that the necessary (and sufficient, see the notes below) condition for its unique solvability is \eqref{cc}. To proceed in this way, we'll reduce problem \eqref{np} to the corresponding one for the Laplace equation and then apply the result known for the Neumann problem for harmonic functions. Let $$ s(x-y)= \begin{cases} \dfrac{1}{2\pi}\log|{x}-{y}| & n=2\\ \\ -\dfrac{1}{(n-2)|\sigma_n}|{x}-{y}|^{2-n} & n\ge 3 \end{cases} $$ be the fundamental solution supported in $y\in\Omega\subset\Bbb R^n$ of the Laplace operator: if we formally define $$ \begin{align} \varphi^\ast(x)&=\varphi(x)-\int\limits_\bar{\Omega}s(x-y)f(y)\mathrm{d}y & x\in\Omega \\ g^\ast(x)&=g(x)-\frac{\partial}{\partial \vec{n}}\int\limits_\bar{\Omega}s(x-y)f(y)\mathrm{d}y & \: x\in\partial\Omega\label{3}\tag{3} \end{align} $$ we have that $\varphi(x)$ solves \eqref{np} if and only if $\varphi^\ast(x)$ is harmonic and solves $$ \color{brown}{ \begin{cases} \Delta \varphi^\ast(x)=0 & x\in\bar{\Omega}\\ \frac{\partial}{\partial \vec{n}}\varphi^\ast(x)=g^\ast(x)& x\in\partial\bar{\Omega} \end{cases}\label{hnp}\tag{HNP}} $$ Now let's search for $\varphi^\ast(x)$ by expressing it as a single layer potential, i.e. $$ \varphi^\ast(x)= \int\limits_{\partial\bar{\Omega}}s(x-y) \mu(y)\mathrm{d}\sigma_y,\label{4}\tag{4} $$ and searching for the unknown (charge) density $\mu(x)$, $x\in\partial\bar{\Omega}$. By applying the classical jump formula for the first derivatives of harmonic functions to \eqref{4} (see for example [2], §22.7, pp. 304-306), i.e. $$ \lim_{\substack{x\to x_0 \\ x\in \vec{n}_{x_0}^+}} \frac{\partial}{\partial \vec{n}_{x}} \int\limits_{\partial\bar{\Omega}}s(x-y)\mu(y)\mathrm{d}\sigma_y = -\frac{1}{2}\mu(x_0) + \frac{\partial}{\partial \vec{n}_{x_0}} \int\limits_{\partial\bar{\Omega}}s(x_0-y)\mu(y)\mathrm{d}\sigma_y $$ we get the following Fredholm integral equation for the unknown density $\mu(x)$ $$ g^\ast(x)= - \frac{1}{2}\mu(x) + \int\limits_{\partial\bar{\Omega}} \frac{\partial}{\partial \vec{n}_{x}} s(x-y)\mu(y)\mathrm{d}\sigma_y \label{5}\tag{5} $$ whose sufficient condition for solvability, by Fredholm's alternative theorem (see for example [2], §16.3, pp. 225-227), is $$ \color{purple}{ \int\limits_{\partial\bar{\Omega}}g^\ast(x)\mathrm{d}\sigma_x=0 \label{hcc}\tag{HCC}} $$ Now let's analyze condition \eqref{hcc}: substituting \eqref{3} in it, we have $$ \begin{split} \int\limits_{\partial\bar{\Omega}}g^\ast(x)\mathrm{d}\sigma_x &= \int\limits_{\partial\bar{\Omega}}\bigg[g(x) - \frac{\partial}{\partial \vec{n}}\int\limits_\bar{\Omega}s(x-y)f(y)\mathrm{d}y\bigg]\mathrm{d}\sigma_x\\ & = \int\limits_{\partial\bar{\Omega}} g(x) \mathrm{d}\sigma_x -\int\limits_{\partial\bar{\Omega}}\frac{\partial}{\partial \vec{n}}\int\limits_\bar{\Omega}s(x-y)f(y)\mathrm{d}y\,\mathrm{d}\sigma_x\\ & \text{and applying the divergence theorem}\\ & = \int\limits_{\partial\bar{\Omega}} g(x) \mathrm{d}\sigma_x -\int\limits_\bar{\Omega} \Delta\int\limits_\bar{\Omega}s(x-y)f(y)\mathrm{d}y\,\mathrm{d}x\\ & = \int\limits_{\partial\bar{\Omega}} g(x) \mathrm{d}\sigma_x -\int\limits_\bar{\Omega} f(x) \mathrm{d}x \end{split}\label{6}\tag{6} $$ and the proof is then finished.

Final notes on the method of proof of the implication \eqref{cc}$ \implies $\eqref{np}.

  • The same very same method can be used to prove directly the equivalence \eqref{cc}$ \iff $\eqref{np}: as alluded above, condition \eqref{hcc} (and his equivalent condition \eqref{cc} for Poisson's equation), is de facto a necessary and sufficient condition for the solvability of integral equation \eqref{5}. This is the approach followed for example by V.S. Vladimirov for the Laplace equation ([2], §23.5, pp. 315-318) which, however, does not explicitly deals with Poisson's equation, i.e. does not provide the ansatz \eqref{3} nor the development \eqref{6}.
  • The same method can also be used to prove the existence and uniqueness of the weak solution (and thus the weak formulation) of the Neumann problem \eqref{np} even for the more general divergence form equation, $$ \operatorname{div}\big(k(x)\nabla \varphi(x)\big)-a(x)\varphi(x)=f(x) $$ obviously without any reference nor use of potential theory. To see why, it is sufficient to remember that the weak formulation of problem \eqref{np} is simply a set of integral identities to be satisfied by the solution $\varphi$: the details can be found in reference [1], chapter IV, §1.2, 1.6.

[1] V. P. Mikhailov (1978), Partial differential equations, Translated from the Russian by P.C. Sinha. Revised from the 1976 Russian ed., Moscow: Mir Publishers, p. 396 MR0601389, Zbl 0388.3500.

[2] V. S. Vladimirov (1971)[1967], Equations of mathematical physics, Translated from the Russian original (1967) by Audrey Littlewood. Edited by Alan Jeffrey, (English), Pure and Applied Mathematics, Vol. 3, New York: Marcel Dekker, Inc., pp. vi+418, MR0268497, Zbl 0207.09101.

  • Thanks, why does $CC \implies NP$ follows simply by reversing of the previously listed steps?I don't think it's obvious. – notime May 07 '19 at 14:47
  • @XingyingLi you are welcome. I will add a better explanation later, by expanding point 2. – Daniele Tampieri May 07 '19 at 14:54
  • @XingyingLi done. I tend to be quite brief on the final parts of answers, so if you need further explanations, do not hesitate asking. – Daniele Tampieri May 07 '19 at 15:33
  • I can't understand this step:since (2) implies that $$ \frac{\partial}{\partial\vec{n}}\varphi(x)=g(x)\quad\text{ for almost all }x\in\partial\bar{\Omega}$$. – notime May 07 '19 at 20:43
  • I know that"$\int_{\partial{\bar{\Omega}}}{\frac{\partial}{\partial\overrightarrow{n}}\varphi ds_x}=\int_{\partial{\bar{\Omega}}}{gds_x}$". – notime May 07 '19 at 20:49
  • @XingyingLi I apologize for mi later in answering, but I am traveling so It is a little more difficult for me to reply to you. First I did not stated that we must obviously assume $g=\operatorname{trace}(f)$, otherwise, as you correctly note, you can only prove the equality of the two integrals, and then deduce a relationship between the trace of $\varphi$. – Daniele Tampieri May 08 '19 at 17:20
  • @XingyingLi I’ll add something as soon as I can – Daniele Tampieri May 08 '19 at 18:08
  • When you derive (HCC) you use Fredholm alternative theorems. But those theorem gives the condition of the function being orthonormal to the solutions of the adjoint homogeneus Fredholm equation, (see the same reference you mention). How does it realte to (HCC)? I think there are many steps left there and I cannot fill the gaps. – Jose Pérez Cano Jun 02 '22 at 10:35
  • @JosePérezCano Your question is completely justified. The central nontrivial detail is that $\ker(I-K)=\mathrm{span}{\mathrm{id}_\Omega}$, where $I-K$ denotes the operator being applied to $\mu$ on the RHS at (5). The proof of this fact involves the Fredholm theorem. For more details, see p. 134--136 at G. Folland (1995), Introduction to partial differential equations, Princeton: Princeton University Press, xii+324 pp. MR1357411 – gpr1 May 25 '23 at 22:20