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Neumann boundary condition

 
Sci-Tech Dictionary: Neumann boundary condition
(′nöi′män ′bau̇n·drē kən′dish·ən)

(mathematics) The boundary condition imposed on the Neumann problem in potential theory.


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In mathematics, the Neumann (or second-type) boundary condition is a type of boundary condition, named after Carl Neumann[1]. When imposed on an ordinary or a partial differential equation, it specifies the values that the derivative of a solution is to take on the boundary of the domain.

In the case of an ordinary differential equation, for example such as:

\frac{d^2y}{dx^2} + 3 y = 1

on the interval [0,1] the Neumann boundary conditions take the form:

\frac{dy}{dx}(0) = \alpha_1
\frac{dy}{dx}(1) = \alpha_2

where α₁ and α₂ are given numbers.

For a partial differential equation on a domain Ω⊂ℝⁿ such as:

\nabla^2 y = 0

where ∇² denotes the Laplacian, the Neumann boundary condition takes the form:

\frac{\partial y}{\partial n}(x) = f(x) \quad \forall x \in \partial\Omega.

Here, n denotes the (typically exterior) normal to the boundary ∂Ω and f is a given scalar function. The normal derivative which shows up on the left-hand side is defined as :

\frac{\partial y}{\partial n}(x)=\nabla y(x)\cdot n(x)

where ∇ is the gradient and the dot is the inner product.

See also

References

  1. ^ Cheng, A. and D. T. Cheng (2005). Heritage and early history of the boundary element method, Engineering Analysis with Boundary Elements, 29, 268–302.

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