Laplace's equation
In mathematics, Laplace's equation is a second-order partial differential equation named after Pierre-Simon Laplace who first studied its properties. This is often written as:
where ∆ = ∇^{2} is the Laplace operator^{[1]} (see below) and is a scalar function.
Laplace's equation and Poisson's equation are the simplest examples of elliptic partial differential equations. The general theory of solutions to Laplace's equation is known as potential theory. The solutions of Laplace's equation are the harmonic functions, which are important in many fields of science, notably the fields of electromagnetism, astronomy, and fluid dynamics, because they can be used to accurately describe the behavior of electric, gravitational, and fluid potentials. In the study of heat conduction, the Laplace equation is the steady-state heat equation.
Contents
Definition
In three dimensions, the problem is to find twice-differentiable real-valued functions f, of real variables x, y, and z, such that
or
This is often written as
or, especially in more general contexts,
where ∆ = ∇^{2} is the Laplace operator or "Laplacian"
where ∇ ⋅ is the divergence operator (also symbolized "div") which maps vector functions to scalar functions, and ∇ is the gradient operator (also symbolized "grad") which maps scalar functions to vector functions. Hence the Laplacian Δf ≝ div grad f maps the scalar function f to a scalar function.
If the right-hand side is specified as a given function, h(x, y, z), i.e., if the whole equation is written as
then it is called "Poisson's equation".
The Laplace equation is also a special case of the Helmholtz equation.
Boundary conditions
The Dirichlet problem for Laplace's equation consists of finding a solution φ on some domain D such that φ on the boundary of D is equal to some given function. Since the Laplace operator appears in the heat equation, one physical interpretation of this problem is as follows: fix the temperature on the boundary of the domain according to the given specification of the boundary condition. Allow heat to flow until a stationary state is reached in which the temperature at each point on the domain doesn't change anymore. The temperature distribution in the interior will then be given by the solution to the corresponding Dirichlet problem.
The Neumann boundary conditions for Laplace's equation specify not the function φ itself on the boundary of D, but its normal derivative. Physically, this corresponds to the construction of a potential for a vector field whose effect is known at the boundary of D alone.
Solutions of Laplace's equation are called harmonic functions; they are all analytic within the domain where the equation is satisfied. If any two functions are solutions to Laplace's equation (or any linear homogeneous differential equation), their sum (or any linear combination) is also a solution. This property, called the principle of superposition, is very useful, e.g., solutions to complex problems can be constructed by summing simple solutions.
Laplace equation in two dimensions
The Laplace equation in two independent variables has the form
Analytic functions
The real and imaginary parts of a complex analytic function both satisfy the Laplace equation. That is, if z = x + iy, and if
then the necessary condition that f(z) be analytic is that the Cauchy–Riemann equations be satisfied:
where u_{x} is the first partial derivative of u with respect to x. It follows that
Therefore u satisfies the Laplace equation. A similar calculation shows that v also satisfies the Laplace equation. Conversely, given a harmonic function, it is the real part of an analytic function, f(z) (at least locally). If a trial form is
then the Cauchy–Riemann equations will be satisfied if we set
This relation does not determine ψ, but only its increments:
The Laplace equation for φ implies that the integrability condition for ψ is satisfied:
and thus ψ may be defined by a line integral. The integrability condition and Stokes' theorem implies that the value of the line integral connecting two points is independent of the path. The resulting pair of solutions of the Laplace equation are called conjugate harmonic functions. This construction is only valid locally, or provided that the path does not loop around a singularity. For example, if r and θ are polar coordinates and
then a corresponding analytic function is
However, the angle θ is single-valued only in a region that does not enclose the origin.
The close connection between the Laplace equation and analytic functions implies that any solution of the Laplace equation has derivatives of all orders, and can be expanded in a power series, at least inside a circle that does not enclose a singularity. This is in sharp contrast to solutions of the wave equation, which generally have less regularity.
There is an intimate connection between power series and Fourier series. If we expand a function f in a power series inside a circle of radius R, this means that
with suitably defined coefficients whose real and imaginary parts are given by
Therefore
which is a Fourier series for f. These trigonometric functions can themselves be expanded, using multiple angle formulae.
Fluid flow
Let the quantities u and v be the horizontal and vertical components of the velocity field of a steady incompressible, irrotational flow in two dimensions. The continuity condition for an incompressible flow is that
and the condition that the flow be irrotational is that
If we define the differential of a function ψ by
then the continuity condition is the integrability condition for this differential: the resulting function is called the stream function because it is constant along flow lines. The first derivatives of ψ are given by
and the irrotationality condition implies that ψ satisfies the Laplace equation. The harmonic function φ that is conjugate to ψ is called the velocity potential. The Cauchy–Riemann equations imply that
Thus every analytic function corresponds to a steady incompressible, irrotational fluid flow in the plane. The real part is the velocity potential, and the imaginary part is the stream function.
Electrostatics
According to Maxwell's equations, an electric field (u, v) in two space dimensions that is independent of time satisfies
and
where ρ is the charge density. The first Maxwell equation is the integrability condition for the differential
so the electric potential φ may be constructed to satisfy
The second of Maxwell's equations then implies that
which is the Poisson equation. The Laplace equation can be used in three-dimensional problems in electrostatics and fluid flow just as in two dimensions.
Laplace equation in three dimensions
Fundamental solution
A fundamental solution of Laplace's equation satisfies
where the Dirac delta function δ denotes a unit source concentrated at the point (x′, y′, z′). No function has this property: in fact it is a distribution rather than a function; but it can be thought of as a limit of functions whose integrals over space are unity, and whose support (the region where the function is non-zero) shrinks to a point (see weak solution). It is common to take a different sign convention for this equation than one typically does when defining fundamental solutions. This choice of sign is often convenient to work with because −Δ is a positive operator. The definition of the fundamental solution thus implies that, if the Laplacian of u is integrated over any volume that encloses the source point, then
The Laplace equation is unchanged under a rotation of coordinates, and hence we can expect that a fundamental solution may be obtained among solutions that only depend upon the distance r from the source point. If we choose the volume to be a ball of radius a around the source point, then Gauss' divergence theorem implies that
It follows that
on a sphere of radius r that is centered on the source point, and hence
Note that, with the opposite sign convention (used in physics), this is the potential generated by a point particle, for an inverse-square law force, arising in the solution of Poisson equation. A similar argument shows that in two dimensions
where log(r) denotes the natural logarithm. Note that, with the opposite sign convention, this is the potential generated by a pointlike sink (see point particle), which is the solution of the Euler equations in two-dimensional incompressible flow.
Green's function
A Green's function is a fundamental solution that also satisfies a suitable condition on the boundary S of a volume V. For instance,
may satisfy
Now if u is any solution of the Poisson equation in V:
and u assumes the boundary values g on S, then we may apply Green's identity, (a consequence of the divergence theorem) which states that
The notations u_{n} and G_{n} denote normal derivatives on S. In view of the conditions satisfied by u and G, this result simplifies to
Thus the Green's function describes the influence at (x′, y′, z′) of the data f and g. For the case of the interior of a sphere of radius a, the Green's function may be obtained by means of a reflection (Sommerfeld 1949): the source point P at distance ρ from the center of the sphere is reflected along its radial line to a point P' that is at a distance
Note that if P is inside the sphere, then P' will be outside the sphere. The Green's function is then given by
where R denotes the distance to the source point P and R′ denotes the distance to the reflected point P′. A consequence of this expression for the Green's function is the Poisson integral formula. Let ρ, θ, and φ be spherical coordinates for the source point P. Here θ denotes the angle with the vertical axis, which is contrary to the usual American mathematical notation, but agrees with standard European and physical practice. Then the solution of the Laplace equation with Dirichlet boundary values g inside the sphere is given by
- (Zachmanoglou 1986, p. 228)
where
is the cosine of the angle between (θ, φ) and (θ′, φ′). A simple consequence of this formula is that if u is a harmonic function, then the value of u at the center of the sphere is the mean value of its values on the sphere. This mean value property immediately implies that a non-constant harmonic function cannot assume its maximum value at an interior point.
Electrostatics
In free space the Laplace equation of any electrostatic potential must equal zero since ρ (charge density) is zero in free space.
Taking the gradient of the electric potential we get the electrostatic field
Taking the divergence of the electrostatic field, we obtain Poisson's equation, that relates charge density and electric potential
In the particular case of the empty space (ρ = 0) Poisson's equation reduces to Laplace's equation for the electric potential.
Using a uniqueness theorem and showing that a potential satisfies Laplace's equation (second derivative of V should be zero i.e. in free space) and the potential has the correct values at the boundaries, the potential is then uniquely defined.
A potential that doesn't satisfy Laplace's equation together with the boundary condition is an invalid electrostatic potential.
Laplace equation in Schwarzschild metric
S. Persides^{[2]} solved the Laplace equation in Schwarzschild spacetime. Using the canonical variables r, θ, φ the solution is
where Y_{l}(θ, φ) is a spherical harmonic function, and
Here P_{l} and Q_{l} are Legendre functions of the first and second kind, respectively, while r_{s} is the Schwarzschild radius. The parameter l is an arbitrary non-negative integer.
See also
- 6-sphere coordinates, a coordinate system under which Laplace's equation becomes R-separable
- Helmholtz equation, a general case of Laplace's equation.
- Spherical harmonic
- Quadrature domains
- Potential theory
- Potential flow
- Bateman transform
- Earnshaw's theorem uses the Laplace equation to show that stable static ferromagnetic suspension is impossible
- Vector Laplacian
- Fundamental solution
Notes
- ^ The delta symbol, Δ, is also commonly used to represent "a change in" some quantity, e.g. ∆Q ≝ Q + δ or ∆Q ≝ Q + εQ for some very small scalars δ or ε. Its use to represent the Laplacian should not be confused with this use.
- ^ Persides, S. (1973). "The Laplace and poisson equations in Schwarzschild's space-time". Journal of Mathematical Analysis and Applications. 43 (3): 571–578. doi:10.1016/0022-247X(73)90277-1.
References
- Evans, L. C. (1998). Partial Differential Equations. Providence: American Mathematical Society. ISBN 0-8218-0772-2.
- Petrovsky, I. G. (1967). Partial Differential Equations. Philadelphia: W. B. Saunders.
- Polyanin, A. D. (2002). Handbook of Linear Partial Differential Equations for Engineers and Scientists. Boca Raton: Chapman & Hall/CRC Press. ISBN 1-58488-299-9.
- Sommerfeld, A. (1949). Partial Differential Equations in Physics. New York: Academic Press.
- Zachmanoglou, E. C. (1986). Introduction to Partial Differential Equations with Applications. New York: Dover.
External links
- Hazewinkel, Michiel, ed. (2001) [1994], "Laplace equation", Encyclopedia of Mathematics, Springer Science+Business Media B.V. / Kluwer Academic Publishers, ISBN 978-1-55608-010-4
- Laplace Equation (particular solutions and boundary value problems) at EqWorld: The World of Mathematical Equations.
- Example initial-boundary value problems using Laplace's equation from exampleproblems.com.
- Weisstein, Eric W. "Laplace's Equation". MathWorld.
- Find out how boundary value problems governed by Laplace's equation may be solved numerically by boundary element method