Stable orbits in higher dimensions

In this problem, we denote the number of spatial dimensions by n n . Our universe has 3 spatial dimensions, n = 3 n=3 . Both classical atoms and planetary orbits have stable solutions in n = 3 n=3 , take for example an isolated Hydrogen atom, or the solar system. In both cases, the central potential holding the bound state together is of the form V ( r ) = α r V(r) = -\frac{\alpha}{r} , where α \alpha is a constant and r r is the distance between the two bodies. The constant α \alpha depends on the type of force, electrostatic (for atoms) or gravitational (for planets and stars).

In the case of two planets orbiting each other, for example, we can have 3 kinds of orbits in n = 3 n=3 : elliptical, parabolic and hyperbolic. The stable orbits are the bounded ones that do not escape to infinity, i.e. the elliptical ones. For a two-body-system these orbits are also infinitely long-lived.

What is the maximum number of dimensions n n such that there are stable solutions for atoms and gravitational bound states?

Hint : Take the simplest case of a two-body-system and look for bounded orbits.

Note : Assume that the electrostatic/gravitational potential in any dimension is given by Poisson equation 2 V ( r ) = ρ \nabla^2 V(r) =\rho , where ρ \rho is the charge/mass density.

4 7 There are always stable solutions 5 3 6

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3 solutions

In what way does it become manifest in the fundamental laws of physics that space has three dimensions? (Ehrenfest to Lorentz, private conversation)

Solving the Poisson equation 2 V ( r ) = ρ \nabla^2 V(r)=\rho , we find that the potential goes as V ( r ) = α r 2 n V(r)=-\alpha r^{2-n} in an arbitrary number of dimensions n n . This is intuitive as the force field has more dimensions to spread into in higher n n and as a result it dies faster with increasing distance.

As a concrete example, let's study the motion of two bodies of mass m m moving under the influence of gravity. The motion takes place in a plane. We introduce the polar coordinates in the plane ( r , θ ) (r,\theta) . The two integrals of motion are the total energy of the system E E and the angular momentum L L :

m 2 ( r ˙ 2 + r 2 θ ˙ 2 ) + V ( r ) = E \frac{m}{2} (\dot{r}^2+r^2\dot{\theta}^2) + V(r) = E

m r 2 θ ˙ = L m r^2 \dot{\theta}=L

By elimination of θ ˙ \dot{\theta} , we find for r ˙ \dot{r}

r ˙ = 2 E m 2 V m L 2 m 2 r 2 \dot{r}=\sqrt{\frac{2E}{m}-\frac{2 V}{m} - \frac{L^2}{m^2 r^2} }

which we can rearrange as

r ˙ = 1 r 2 E m r 2 + 2 α m r 4 n L 2 m 2 \dot{r}=\frac{1}{r} \sqrt{\frac{2E}{m} r^2+\frac{2 \alpha}{m} r^{4-n} - \frac{L^2}{m^2} }

In a stable bound system the radial velocity r ˙ \dot{r} has to oscillate between positive and negative values, which means that it has to vanish in at least two points (it can also be identically zero for example). In fact, the quantity under the square root must always be positive between the two values of r for which it is zero. In other words the function 2 E m r 2 + 2 α m r 4 n L 2 m 2 \frac{2E}{m} r^2+\frac{2 \alpha}{m} r^{4-n} - \frac{L^2}{m^2} must vanish in (at least) two points and be positive in between in order for a stable bound orbit to exist. You can easily convince yourself that this is impossible for n > 3 n>3 .

The reason is simple. For n = 4 n=4 the function has at most one real root in r > 0 r>0 and therefore evidently does not satisfy the requirement. For n > 4 n>4 and E < 0 E<0 , the function has again only one real root in r > 0 r>0 . For n > 4 n>4 and E > 0 E>0 , the function has two real roots in r > 0 r>0 and it diverges to + + \infty for both r 0 r \rightarrow 0 and r r \rightarrow \infty which means that it is negative in between. On the other hand, for the critical value of n = 3 n=3 and for E < 0 E<0 , the function has two real roots and it is positive in between. Therefore no stable bound states exist for n > 3 n>3 .

We conclude that in a space with more than three dimensions, there can be no traditional atoms and perhaps no stable structures. In particular, higher dimensional universes cannot contain self-aware observers such as us. This is a hint that there is something special about 3 dimensions. For an interesting discussion along these lines, see this paper .

Amal Hari
Dec 25, 2018

I don't know if its valid but i thought of the answer on a different way,

In a 4 dimensional space our infinite 3-dimensional space is bound as a singular point relatively ,

considering this bounded orbit is present inside 3 dimensions,

evolving these orbits into 4 dimensions means we have to extend orbits beyond infinity , thus breaking stability(relatively)

Since this is true for 4-dimensional space it will also be true for higher dimensions.

In other words for an observer in 4-D this orbit doesn't exist unless the system extends beyond infinity relative to 3-dimensional observer.

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