PlanetPhysics/Potential of Spherical Shell

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Let\, (ξ,η,ζ)\, be a point bearing a [[../CosmologicalConstant/|mass\,]] m\, and\, (x,y,z)\, a variable point. If the distance of these points is r, we can define the potential of\, (ξ,η,ζ)\, in\, (x,y,z)\, as mr=m(xξ)2+(yη)2+(zζ)2. The relevance of this [[../PreciseIdea/|concept]] appears from the fact that its partial derivatives x(mr)=m(xξ)r3,y(mr)=m(yη)r3,z(mr)=m(zζ)r3 are the components of the gravitational force with which the material point\, (ξ,η,ζ)\, acts on one mass unit in the point\, (x,y,z)\, (provided that the measure units are chosen suitably).

The potential of a set of points\, (ξ,η,ζ)\, is the sum of the potentials of individual points, i.e. it may lead to an integral.\\

We determine the potential of all points\, (ξ,η,ζ)\, of a hollow ball, where the matter is located between two concentric spheres with radii R0 and R(>R0). Here the density of mass is assumed to be presented by a continuous [[../Bijective/|function]] \, ϱ=ϱ(r)\, at the distance r from the centre O. Let a be the distance from O of the point A, where the potential is to be determined. We chose O the origin and the ray OA the positive z-axis.

For obtaining the potential in A we must integrate over the ball shell where R0rR. We use the spherical coordinates r, φ and ψ which are tied to the Cartesian coordinates via x=rcosφcosψ,y=rcosφsinψ,z=rsinφ; for attaining all points we set R0rR,π2φπ2,0ψ<2π. The cosines law implies that\, PA=r22arsinφ+a2. Thus the potential is the triple integral

V(a)=R0Rπ2π202πϱ(r)r2cosφr22arsinφ+a2drdφdψ=2πR0Rϱ(r)rdrπ2π2rcosφdφr22arsinφ+a2,

where the factor\, r2cosφ\, is the coefficient for the coordinate changing |(x,y,z)(r,φ,ψ)|=mod|cosφcosψcosφsinψsinφrsinφcosψrsinφsinψrcosφrcosφsinψrcosφcosψ0|.

We get from the latter integral

Failed to parse (unknown function "\sijoitus"): {\displaystyle \begin{matrix} \int_{-\frac{\pi}{2}}^\frac{\pi}{2} \frac{r\cos\varphi\,d\varphi}{\sqrt{r^2-2ar\sin\varphi+a^2}} = -\frac{1}{a}\sijoitus{\varphi=-\frac{\pi}{2}}{\quad\frac{\pi}{2}}\sqrt{r^2-2ar\sin\varphi+a^2} = \frac{1}{a}[(r+a)-|r-a|]. \end{matrix}}

Accordingly we have the two cases:

1.\, The point A is outwards the hollow ball, i.e. a>R.\, Then we have\, |ra|=ar\, for all\, r[R0,R].\, The value of the integral (2) is 2ra, and (1) gets the form V(a)=4πaR0Rϱ(r)r2dr=Ma, where M is the mass of the hollow ball. Thus the potential outwards the hollow ball is exactly the same as in the case that all mass were concentrated to the centre . A correspondent statement concerns the attractive force V(a)=Ma2.

2.\, The point A is in the cavity of the hollow ball, i.e. a<R0 .\, Then\, |ra|=ra\, on the interval of integration of (2). The value of (2) is equal to 2, and (1) yields V(a)=4πR0Rϱ(r)rdr, which is independent on a. That is, the potential of the hollow ball, when the density of mass depends only on the distance from the centre, has in the cavity a constant value, and the hollow ball influences in no way on a mass inside it .

All Sources

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References

  1. {\sc Ernst Lindel\"of}: {\em Differentiali- ja integralilasku ja sen sovellutukset II}.\, Mercatorin Kirjapaino Osakeyhti\"o, Helsinki (1932).

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