Newtonian potential

Source: Wikipedia, the free encyclopedia.

In

electrostatic potential
.

The Newtonian potential of a

integrable function f is defined as the convolution
where the Newtonian kernel Γ in dimension d is defined by

Here ωd is the volume of the unit

d-ball (sometimes sign conventions may vary; compare (Evans 1998) and (Gilbarg & Trudinger 1983
)). For example, for we have

The Newtonian potential w of f is a solution of the

Poisson equation
which is to say that the operation of taking the Newtonian potential of a function is a partial inverse to the Laplace operator. Then w will be a classical solution, that is twice differentiable, if f is bounded and locally
Hölder continuous as shown by Otto Hölder. It was an open question whether continuity alone is also sufficient. This was shown to be wrong by Henrik Petrini
who gave an example of a continuous f for which w is not twice differentiable. The solution is not unique, since addition of any harmonic function to w will not affect the equation. This fact can be used to prove existence and uniqueness of solutions to the Dirichlet problem for the Poisson equation in suitably regular domains, and for suitably well-behaved functions f: one first applies a Newtonian potential to obtain a solution, and then adjusts by adding a harmonic function to get the correct boundary data.

The Newtonian potential is defined more broadly as the convolution

when μ is a compactly supported Radon measure. It satisfies the Poisson equation
in the sense of
positive, the Newtonian potential is subharmonic
on Rd.

If f is a compactly supported continuous function (or, more generally, a finite measure) that is rotationally invariant, then the convolution of f with Γ satisfies for x outside the support of f

In dimension d = 3, this reduces to Newton's theorem that the potential energy of a small mass outside a much larger spherically symmetric mass distribution is the same as if all of the mass of the larger object were concentrated at its center.

When the measure μ is associated to a mass distribution on a sufficiently smooth hypersurface S (a

Neumann problem
for the Laplace equation.

See also

References

  • .
  • Gilbarg, D.; .
  • Solomentsev, E.D. (2001) [1994], "Newton potential", Encyclopedia of Mathematics, EMS Press
  • Solomentsev, E.D. (2001) [1994], "Simple-layer potential", Encyclopedia of Mathematics, EMS Press
  • Solomentsev, E.D. (2001) [1994], "Surface potential", Encyclopedia of Mathematics, EMS Press