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The Laplace Equation

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Part of the book series: Mathematical Engineering ((MATHENGIN))

Abstract

The Laplace equation is the archetypal elliptic equation. It appears in many applications when studying the steady state of physical systems that are otherwise governed by hyperbolic or parabolic operators. Correspondingly, elliptic equations require the specification of boundary data only, and the Cauchy (initial-value) problem does not arise.

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Notes

  1. 1.

    Notice that we have also used the term harmonic to designate a sinusoidal function of one variable. These two usages are unrelated.

  2. 2.

    Strictly speaking, this proof of uniqueness requires the solution to be twice differentiable not just in the interior but also on the boundary of the domain. This requirement can be relaxed if the proof is based on the maximum-minimum principle, that we shall study below.

  3. 3.

    Named after the German mathematician Carl Gottfried Neumann (1832–1925), not to be confused with John von Neumann (1903–1957), the great Hungarian-American mathematician.

  4. 4.

    See [3], p. 98. Notice that, correspondingly, the Dirichlet problem has in general no solution for the hyperbolic and parabolic cases, since the specification of the solution over the whole boundary of a domain will in general lead to a contradiction. For this point see [2], p. 236.

  5. 5.

    See [4], p. 169.

  6. 6.

    Recall that the diameter of a set (in a metric space) is the least upper bound of the distances between all pairs of points of the set.

  7. 7.

    This feature of the solution for the case of the gravitational field was extremely important to Newton, who was at pains to prove it. It is this property that allowed him to conclude that the forces exerted by a homogeneous sphere on empty space are unchanged if the total mass is concentrated at its centre.

  8. 8.

    For the case \(n=2\), we have \(B=1/2\pi \). For \(n=3,\) as we have seen, the value is \(B=-1/4\pi \). For higher dimensions, the value of the constant can be shown to be related to the ‘area’ of the corresponding hyper-sphere, which involves the Gamma function. See [3], p. 96.

  9. 9.

    Good sources are [1, 3, 5].

References

  1. Courant R, Hilbert D (1962) Methods of mathematical physics, vol II. Interscience, Wiley, New York

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  2. Garabedian PR (1964) Partial differential equations. Wiley, New York

    Google Scholar 

  3. John F (1982) Partial differential equations. Springer, Berlin

    Google Scholar 

  4. Petrovsky IG (1991) Lectures on partial differential equations. Dover, New York

    Google Scholar 

  5. Sobolev SL (1989) Partial differential equations of mathematical physics. Dover, New York

    Google Scholar 

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Correspondence to Marcelo Epstein .

Exercises

Exercises

Exercise 11.1

Show that under an orthogonal change of coordinates, the Laplacian retains the form given in Eq. (11.5). If you prefer to do so, work in a two-dimensional setting.

Exercise 11.2

Express the Laplacian in cylindrical coordinates (or polar coordinates, if you prefer to work in two dimensions).

Exercise 11.3

Obtain Eqs. (11.9), (11.10) and (11.11). Show, moreover, that the flux of the gradient of a harmonic function over the boundary of any bounded domain vanishes.

Exercise 11.4

A membrane is extended between two horizontal concentric rigid rings of 500 and 50 mm radii. If the inner ring is displaced vertically upward by an amount of 100 mm, find the resulting shape of the membrane. Hint: Use Eq. (11.23).

Exercise 11.5

Carry out the calculations leading to (11.27). Make sure to use each of the assumptions made about the solution. Find the solution for the two-dimensional case.

Exercise 11.6

Carry out and justify all the steps necessary to obtain Eq. (11.38).

Exercise 11.7

What is the value of G(XP)? How is this value reconciled with Eq. (11.46)?

Exercise 11.8

Adopting polar coordinate in the plane, with origin at the centre of the circle, and denoting the polar coordinates of X by \(\rho , \theta \) and those of Y (at the boundary) by \(R, \psi \), show that the solution to Dirichlet’s problem is given by the expression

$$\begin{aligned} u(\rho , \theta ) = \frac{1}{2\pi }\;\int \limits _0^{2\pi }\;\frac{R^2-\rho ^2}{R^2+\rho ^2-2R\;\rho \;\cos (\theta -\psi )}\;h(\psi )\;d\psi . \end{aligned}$$
(11.50)

where \(h(\psi )\) represents the boundary data. Use Eqs. (11.48) and (11.49) (with a 2 in the denominator).

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Epstein, M. (2017). The Laplace Equation. In: Partial Differential Equations. Mathematical Engineering. Springer, Cham. https://doi.org/10.1007/978-3-319-55212-5_11

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  • DOI: https://doi.org/10.1007/978-3-319-55212-5_11

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