Quantum Mechanics and the Dodecahedron

This is an expanded version of my G+ post, which was a watered-down version of Greg Egan’s G+ post and the comments on that. I’ll start out slow, and pick up speed as I go.

Quantum mechanics meets the dodecahedron

In quantum mechanics, the position of a particle is not a definite thing: it’s described by a ‘wavefunction’. This says how probable it is to find the particle at any location… but it also contains other information, like how probable it is to find the particle moving at any velocity.

Take a hydrogen atom, and look at the wavefunction of the electron.

Question 1. Can we make the electron’s wavefunction have all the rotational symmetries of a dodecahedron—that wonderful Platonic solid with 12 pentagonal faces?

Yes! In fact it’s too easy: you can make the wavefunction look like whatever you want.

So let’s make the question harder. Like everything else in quantum mechanics, angular momentum can be uncertain. In fact you can never make all 3 components of angular momentum take definite values simultaneously! However, there are lots of wavefunctions where the magnitude of an electron’s angular momentum is completely definite.

This leads naturally to the next question, which was first posed by Gerard Westendorp:

Question 2. Can an electron’s wavefunction have a definite magnitude for its angular momentum while having all the rotational symmetries of a dodecahedron?

Yes! And there are infinitely many ways for this to happen! This is true even if we neglect the radial dependence of the wavefunction—that is, how it depends on the distance from the proton. Henceforth I’ll always do that, which lets us treat the wavefunction as a function on a sphere. And by the way, I’m also ignoring the electron’s spin! So, whenever I say ‘angular momentum’ I mean orbital angular momentum: the part that depends only on the electron’s position and velocity.

Question 2 has a trivial solution that’s too silly to bother with. It’s the spherically symmetric wavefunction! That’s invariant under all rotations. The real challenge is to figure out the simplest nontrivial solution. Egan figured it out, and here’s what it looks like:


The rotation here is just an artistic touch. Really the solution should be just sitting there, or perhaps changing colors while staying the same shape.

In what sense is this the simplest nontrivial solution? Well, the magnitude of the angular momentum is equal to

\hbar^2 \sqrt{\ell(\ell+1)}

where the number \ell is quantized: it can only take values 0, 1, 2, 3,… and so on.

The trivial solution to Question 2 has \ell = 0. The first nontrivial solution has \ell = 6. Why 6? That’s where things get interesting. We can get it using the 6 lines connecting opposite faces of the dodecahedron!

I’ll explain later how this works. For now, let’s move straight on to a harder question:

Question 3. What’s the smallest choice of \ell where we can find two linearly independent wavefunctions that both have the same \ell and both have all the rotational symmetries of a dodecahedron?

It turns out to be \ell = 30. And Egan created an image of a wavefunction oscillating between these two possibilities!

But we can go a lot further:

Question 4. For each \ell, how many linearly independent functions on the sphere have that value of \ell and all the rotational symmetries of a dodecahedron?

For \ell ranging from 0 to 29 there are either none or one. There are none for these numbers:

1, 2, 3, 4, 5, 7, 8, 9, 11, 13, 14, 17, 19, 23, 29

and one for these numbers:

0, 6, 10, 12, 15, 16, 18, 20, 21, 22, 24, 25, 26, 27, 28

The pattern continues as follows. For \ell ranging from 30 to 59 there are either one or two. There is one for these numbers:

31, 32, 33, 34, 35, 37, 38, 39, 41, 43, 44, 47, 49, 53, 59

and two for these numbers:

30, 36, 40, 42, 45, 46, 48, 50, 51, 52, 54, 55, 56, 57, 58

The numbers in these two lists are just 30 more than the numbers in the first two lists! And it continues on like this forever: there’s always one more linearly independent solution for \ell + 30 than there is for \ell.

Question 5. What’s special about these numbers from 0 to 29?

0, 6, 10, 12, 15, 18, 20, 21, 22, 24, 25, 26, 27, 28

You don’t need to know tons of math to figure this out—but I guess it’s a sort of weird pattern-recognition puzzle unless you know which patterns are likely to be important here. So I’ll give away the answer.

Here’s the answer: these are the numbers below 30 that can be written as sums of the numbers 6, 10 and 15.

But the real question is why? Also: what’s so special about the number 30?

The short, cryptic answer is this. The dodecahedron has 6 axes connecting the centers of opposite faces, 10 axes connecting opposite vertices, and 15 axes connecting the centers of opposite edges. The least common multiple of these numbers is 30.

But this requires more explanation!

For this, we need more math. You may want to get off here. But first, let me show you the solutions for \ell = 6, \ell = 10, and \ell = 15, as drawn by Greg Egan. I’ve already showed you \ell = 6, which we could call the quantum dodecahedron:


Here is \ell = 10, which looks like a quantum icosahedron:

And here is \ell = 15:

Maybe this deserves to be called a quantum Coxeter complex, since the Coxeter complex for the group of rotations and reflections of the dodecahedron looks like this:



Functions with icosahedral symmetry

The dodecahedron and icosahedron have the same symmetries, but for some reason people talk about the icosahedron when discussing symmetry groups, so let me do that.

So far we’ve been looking at the rotational symmetries of the icosahedron. These form a group called \mathrm{A}_5, or \mathrm{I} for short, with 60 elements. We’ve been looking for certain functions on the sphere that are invariant under the action of this group. To get them all, we’ll first get ahold of all polynomials on \mathbb{R}^3 that are invariant under the action of this group Then we’ll restrict these to the sphere.

To save time, we’ll use the work of Claude Chevalley. He looked at rotation and reflection symmetries of the icosahedron. These form the group \mathrm{I} \times \mathbb{Z}/2, also known as \mathrm{H}_3, but let’s call it \hat{\mathrm{I}} for short. It has 120 elements, but never confuse it with two other groups with 120 elements: the symmetric group on 5 letters, and the binary icosahedral group.

Chevalley found all polynomials on \mathbb{R}^3 that are invariant under the action of this bigger group \hat{\mathrm{I}}. These invariant polynomials form an algebra, and Chevalley showed that this algebra is freely generated by 3 homogeneous polynomials:

• P(x,y,z) = x^2 + y^2 + z^2, of degree 2.

• Q(x,y,z), of degree 6. To get this we take the dot product of (x,y,z) with each of the 6 vectors joining antipodal vertices of the icosahedron, and multiply them together.

• R(x,y,z), of degree 10. To get this we take the dot product of (x,y,z) with each of the 10 vectors joining antipodal face centers of the icosahedron, and multiply them together.

So, linear combinations of products of these give all polynomials on \mathbb{R}^3 invariant under all rotation and reflection symmetries of the icosahedron.

But we want the polynomials that are invariant under just rotational symmetries of the icosahedron! To get all these, we need an extra generator:

• S(x,y,z), of degree 15. To get this we take the dot product of (x,y,z) with each of the 15 vectors joining antipodal edge centers of the icosahedron, and multiply them together.

You can check that this is invariant under rotational symmetries of the icosahedron. But unlike our other polynomials, this one is not invariant under reflection symmetries! Because 15 is an odd number, S switches sign under ‘total inversion’—that is, replacing (x,y,z) with -(x,y,z). This is a product of three reflection symmetries of the icosahedron.

Thanks to Egan’s extensive computations, I’m completely convinced that P,Q,R and S generate the algebra of all \mathrm{I}-invariant polynomials on \mathbb{R}^3. I’ll take this as a fact, even though I don’t have a clean, human-readable proof. But someone must have proved it already—do you know where?

Since we now have 4 polynomials on \mathbb{R}^3, they must obey a relation. Egan figured it out:

S^2 = 500 P^9 Q^2 - 2275 P^6 Q^3 + 3440 P^3 Q^4 - 1728 Q^5 + 200 P^7 Q R
- 795 P^4 Q^2 R + 720 P Q^3 R + 4 P^5 R^2 -65 P^2 Q R^2 - R^3

The exact coefficients depend on some normalization factors used in defining Q,R and S. Luckily the details don’t matter much. All we’ll really need is that this relation expresses S^2 in terms of the other generators. And this fact is easy to see without any difficult calculations!

How? Well, we’ve seen S is unchanged by rotations, while it changes sign under total inversion. So, the most any rotation or reflection symmetry of the icosahedron can do to S is change its sign. This means that S^2 is invariant under all these symmetries. So, by Chevalley’s result, it must be a polynomial in P, Q, and R.

So, we now have a nice description of the \mathrm{I}-invariant polynomials on \mathbb{R}^3, in terms of generators and relations. Each of these gives an \mathrm{I}-invariant function on the sphere. And Leo Stein, a postdoc at Caltech who has a great blog on math and physics, has kindly created some images of these.

The polynomial P is spherically symmetric so it’s too boring to draw. The polynomial Q, of degree 6, looks like this when restricted to the sphere:

Since it was made by multiplying linear functions, one for each axis connecting opposite vertices of an icosahedron, it shouldn’t be surprising that we see blue blobs centered at these vertices.

The polynomial R, of degree 10, looks like this:

Here the blue blobs are centered on the icosahedron’s 20 faces.

Finally, here’s S, of degree 15:

This time the blue blobs are centered on the icosahedron’s 30 edges.

Now let’s think a bit about functions on the sphere that arise from polynomials on \mathbb{R}^3. Let’s call them algebraic functions on the sphere. They form an algebra, and it’s just the algebra of polynomials on \mathbb{R}^3 modulo the relation P = 1, since the sphere is the set \{P = 1\}.

It makes no sense to talk about the ‘degree’ of an algebraic function on the sphere, since the relation P = 1 equates polynomials of different degree. What makes sense is the number \ell that I was talking about earlier!

The group \mathrm{SO}(3) acts by rotation on the space of algebraic functions on the sphere, and we can break this space up into irreducible representations of \mathrm{SO}(3). It’s a direct sum of irreps, one of each ‘spin’ \ell = 0, 1, 2, \dots.

So, we can’t talk about the degree of a function on the sphere, but we can talk about its \ell value. On the other hand, it’s very convenient to work with homogeneous polynomials on \mathbb{R}^3, which have a definite degree—and these restrict to functions on the sphere. How can we relate the degree and the quantity \ell?

Here’s one way. The polynomials on \mathbb{R}^3 form a graded algebra. That means it’s a direct sum of vector spaces consisting of homogeneous polynomials of fixed degree, and if we multiply two homogeneous polynomials their degrees add. But the algebra of polynomials restricted to the sphere is merely filtered algebra.

What does this mean? Let F be the algebra of all algebraic functions on the sphere, and let F_\ell \subset F consist of those that are restrictions of polynomials of degree \le \ell. Then:

1) F_\ell \subseteq F_{\ell + 1}

and

2) \displaystyle{ F = \bigcup_{\ell = 0}^\infty F_\ell }

and

3) if we multiply a function in F_\ell by one in F_m, we get one in F_{\ell + m}.

That’s what a filtered algebra amounts to.

But starting from a filtered algebra, we can get a graded algebra! It’s called the associated graded algebra.

To do this, we form

G_\ell = F_\ell / F_{\ell - 1}

and let

\displaystyle{ G = \bigoplus_{\ell = 0}^\infty G_\ell }

Then G has a product where multiplying a guy in G_\ell and one in G_m gives one in G_{\ell + m}. So, it’s indeed a graded algebra! For the details, see Wikipedia, which manages to make it look harder than it is. The basic idea is that we multiply in F and then ‘ignore terms of lower degree’. That’s what G_\ell = F_\ell / F_{\ell - 1} is all about.

Now I want to use two nice facts. First, G_\ell is the spin-\ell representation of \mathrm{SO}(3). Second, there’s a natural map from any filtered algebra to its associated graded algebra, which is an isomorphism of vector spaces (though not of algebras). So, we get an natural isomorphism of vector spaces

\displaystyle{ F \cong G = \bigoplus_{\ell = 0}^\infty G_\ell }

from the algebraic functions on the sphere to the direct sum of all the spin-\ell representations!

Now to the point: because this isomorphism is natural, it commutes with symmetries, so we can also use it to study algebraic functions on the sphere that are invariant under a group of linear transformations of \mathbb{R}^3.

Before tackling the group we’re really interested in, let’s try the group of rotation and reflection symmetries of the icosahedron, \hat{\mathrm{I}}. As I mentioned, Chevalley worked out the algebra of polynomials on \mathbb{R}^3 that are invariant under this bigger group. It’s a graded commutative algebra, and it’s free on three generators: P of degree 2, Q of degree 6, and R of degree 10.

Starting from here, to get the algebra of \hat{\mathrm{I}}-invariant algebraic functions on the sphere, we mod out by the relation P = 1. This gives a filtered algebra which I’ll call F^{\hat{\mathrm{I}}}. (It’s common to use a superscript with the name of a group to indicate that we’re talking about the stuff that’s invariant under some action of that group.) From this we can form the associated graded algebra

\displaystyle{ G^{\hat{\mathrm{I}}} = \bigoplus_{\ell = 0}^\infty G_\ell^{\hat{\mathrm{I}}} }

where

G_\ell^{\hat{\mathrm{I}}} = F_\ell^{\hat{\mathrm{I}}} / F_{\ell - 1}^{\hat{\mathrm{I}}}

If you’ve understood everything I’ve been trying to explain, you’ll see that G_\ell^{\hat{\mathrm{I}}} is the space of all functions on the sphere that transform in the spin-\ell representation and are invariant under the rotation and reflection symmetries of the icosahedron.

But now for the fun part: what is this space like? By the work of Chevalley, the algebra F^{\hat{\mathrm{I}}} is spanned by products

P^p Q^q R^r

but since we have the relation P = 1, and no other relations, it has a basis given by products

Q^q R^r

So, the space F_\ell^{\hat{\mathrm{I}}} has a basis of products like this whose degree is \le \ell, meaning

6 q + 10 r \le \ell

Thus, the space we’re really interested in:

G_\ell^{\hat{\mathrm{I}}} = F_\ell^{\hat{\mathrm{I}}} / F_{\ell - 1}^{\hat{\mathrm{I}}}

has a basis consisting of equivalence classes

[Q^q R^r]

where

6 q + 10 r = \ell

So, we get:

Theorem 1. The dimension of the space of functions on the sphere that lie in the spin-\ell representation of \mathrm{SO}(3) and are invariant under the rotation and reflection symmetries of the icosahedron equals the number of ways of writing \ell as an unordered sum of 6’s and 10’s.

Let’s see how this goes:

\ell = 0: dimension 1, with basis [1]

\ell = 1: dimension 0

\ell = 2: dimension 0

\ell = 3: dimension 0

\ell = 4: dimension 0

\ell = 5: dimension 0

\ell = 6: dimension 1, with basis [Q]

\ell = 7: dimension 0

\ell = 8: dimension 0

\ell = 9: dimension 0

\ell = 10: dimension 1, with basis [R]

\ell = 11: dimension 0

\ell = 12: dimension 1, with basis [Q^2]

\ell = 13: dimension 0

\ell = 14: dimension 0

\ell = 15: dimension 0

\ell = 16: dimension 1, with basis [Q R]

\ell = 17: dimension 0

\ell = 18: dimension 1, with basis [Q^3]

\ell = 19: dimension 0

\ell = 20: dimension 1, with basis [R^2]

\ell = 21: dimension 0

\ell = 22: dimension 1, with basis [Q^2 R]

\ell = 23: dimension 0

\ell = 24: dimension 1, with basis [Q^4]

\ell = 25: dimension 0

\ell = 26: dimension 1, with basis [Q R^2]

\ell = 27: dimension 0

\ell = 28: dimension 1, with basis [Q^3 R]

\ell = 29: dimension 0

\ell = 30: dimension 2, with basis [Q^5], [R^3]

So, the story starts out boring, with long gaps. The odd numbers are completely uninvolved. But it heats up near the end, and reaches a thrilling climax at \ell = 30. At this point we get two linearly independent solutions, because 30 is the least common multiple of the degrees of Q and R.

It’s easy to see that from here on the story ‘repeats’ with period 30, with the dimension growing by 1 each time:

\mathrm{dim}(G_{\ell+30}^{\hat{\mathrm{I}}}) = \mathrm{dim}(G_{\ell}^{\hat{\mathrm{I}}}) + 1

Now, finally, we are to tackle Question 4 from the first part of this post: for each \ell, how many linearly independent functions on the sphere have that value of \ell and all the rotational symmetries of a dodecahedron?

We just need to repeat our analysis with \mathrm{I}, the group of rotational symmetries of the dodecahedron, replacing the bigger group \hat{\mathrm{I}}.

We start with algebra of polynomials on \mathbb{R}^3 that are invariant under \mathrm{I}. As we’ve seen, this is a graded commutative algebra with four generators: P,Q,R as before, but also S of degree 15. To make up for this extra generator there’s an extra relation, which expresses S^2 in terms of the other generators.

Starting from here, to get the algebra of \mathrm{I}-invariant algebraic functions on the sphere, we mod out by the relation P = 1. This gives a filtered algebra I’ll call F^{\mathrm{I}}. Then we form the associated graded algebra

\displaystyle{ G^{\mathrm{I}} = \bigoplus_{\ell = 0}^\infty G_\ell^{\mathrm{I}} }

where

G_\ell^{\mathrm{I}} = F_\ell^{\mathrm{I}} / F_{\ell - 1}^{\mathrm{I}}

What we really want to know is the dimension of G_\ell^{\mathrm{I}}, since this is the space of functions on the sphere that transform in the spin-\ell representation and are invariant under the rotational symmetries of the icosahedron.

So, what’s this space like? The algebra F^{\mathrm{I}} is spanned by products

P^p Q^q R^r S^t

but since we have the relation P = 1, and a relation expressing S^2 in terms of other generators, it has a basis given by products

Q^q R^r S^s where s = 0, 1

So, the space F_\ell^{\mathrm{I}} has a basis of products like this whose degree is \le \ell, meaning

6 q + 10 r + 15 s \le \ell and s = 0, 1

Thus, the space we’re really interested in:

G_\ell^{\mathrm{I}} = F_\ell^{\mathrm{I}} / F_{\ell - 1}^{\mathrm{I}}

has a basis consisting of equivalence classes

[Q^q R^r S^s]

where

6 q + 10 r + 15 s = \ell and s = 0, 1

So, we get:

Theorem 2. The dimension of the space of functions on the sphere that lie in the spin-\ell representation of \mathrm{SO}(3) and are invariant under the rotational symmetries of the icosahedron equals the number of ways of writing \ell as an unordered sum of 6’s, 10’s and at most one 15.

Let’s work out these dimensions explicitly, and see how the extra generator S changes the story! Since it has degree 15, it contributes some solutions for odd values of \ell. But when we reach the magic number 30, this extra generator loses its power: S^2 has degree 30, but it’s a linear combination of other things.

\ell = 0: dimension 1, with basis [1]

\ell = 1: dimension 0

\ell = 2: dimension 0

\ell = 3: dimension 0

\ell = 4: dimension 0

\ell = 5: dimension 0

\ell = 6: dimension 1, with basis [Q]

\ell = 7: dimension 0

\ell = 8: dimension 0

\ell = 9: dimension 0

\ell = 10: dimension 1, with basis [R]

\ell = 11: dimension 0

\ell = 12: dimension 1, with basis [Q^2]

\ell = 13: dimension 0

\ell = 14: dimension 0

\ell = 15: dimension 1, with basis [S]

\ell = 16: dimension 1, with basis [Q R]

\ell = 17: dimension 0

\ell = 18: dimension 1, with basis [Q^3]

\ell = 19: dimension 0

\ell = 20: dimension 1, with basis [R^2]

\ell = 21: dimension 1, with basis [Q S]

\ell = 22: dimension 1, with basis [Q^2 R]

\ell = 23: dimension 0

\ell = 24: dimension 1, with basis [Q^4]

\ell = 25: dimension 1, with basis [R S]

\ell = 26: dimension 1, with basis [Q R^2]

\ell = 27: dimension 1, with basis [Q^2 S]

\ell = 28: dimension 1, with basis [Q^3 R]

\ell = 29: dimension 0

\ell = 30: dimension 2, with basis [Q^5], [R^3]

From here on the story ‘repeats’ with period 30, with the dimension growing by 1 each time:

\mathrm{dim}(G_{\ell+30}^{\mathrm{I}}) = \mathrm{dim}(G_{\ell}^{\mathrm{I}}) + 1

So, we’ve more or less proved everything that I claimed in the first part. So we’re done!

Postscript

But I can’t resist saying a bit more.

First, there’s a very different and somewhat easier way to compute the dimensions in Theorems 1 and 2. It uses the theory of characters, and Egan explained it in a comment on the blog post on which this is based.

Second, if you look in these comments, you’ll also see a lot of material about harmonic polynomials on \mathbb{R}^3—that is, those obeying the Laplace equation. These polynomials are very nice when you’re trying to decompose the space of functions on the sphere into irreps of \mathrm{SO}(3). The reason is that the harmonic homogeneous polynomials of degree \ell, when restricted to the sphere, give you exactly the spin-\ell representation!

If you take all homogeneous polynomials of degree \ell and restrict them to the sphere you get a lot of ‘redundant junk’. You get the spin-\ell rep, plus the spin-(\ell-2) rep, plus the spin-(\ell-4) rep, and so on. The reason is the polynomial

P = x^2 + y^2 + z^2

and its powers: if you have a polynomial living in the spin-\ell rep and you multiply it by P, you get another one living in the spin-\ell rep, but you’ve boosted the degree by 2.

Layra Idarani pointed out that this is part of a nice general theory. But I found all this stuff slightly distracting when I was trying to prove Theorems 1 and 2 assuming that we had explicit presentations of the algebras of \hat{\mathrm{I}}– and \mathrm{I}-invariant polynomials on \mathbb{R}^3. So, instead of introducing facts about harmonic polynomials, I decided to use the ‘associated graded algebra’ trick. This is a more algebraic way to ‘eliminate the redundant junk’ in the algebra of polynomials and chop the space of functions on the sphere into irreps of \mathrm{SO}(3).

Also, Egan and Idarani went ahead and considered what happens when we replace the icosahedron by another Platonic solid. It’s enough to consider the cube and tetrahedron. These cases are actually subtler than the icosahedron! For example, when we take the dot product of (x,y,z) with each of the 10 vectors joining antipodal face centers of the cube, and multiply them together, we get a polynomial that’s not invariant under rotations of the cube! Up to a constant it’s just x y z, and this changes sign under some rotations.

People call this sort of quantity, which gets multiplied by a number under transformations instead of staying the same, a semi-invariant. The reason we run into semi-invariants for the cube and tetrahedron is that their rotational symmetry groups, \mathrm{S}_4 and \mathrm{A}_4, have nontrivial abelianizations, namely \mathbb{Z}/2 and \mathbb{Z}/3. The abelianization of \mathrm{I} \cong \mathrm{A}_5 is trivial.

Egan summarized the story as follows:

Just to sum things up for the cube and the tetrahedron, since the good stuff has ended up scattered over many comments:

For the cube, we define:

A of degree 4 from the cube’s vertex-axes, a full invariant
B of degree 6 from the cube’s edge-centre-axes, a semi-invariant
C of degree 3 from the cube’s face-centre-axes, a semi-invariant

We have full invariants:

A of degree 4
C2 of degree 6
BC of degree 9

B2 can be expressed in terms of A, C and P, so we never use it, and we use BC at most once.

So the number of copies of the trivial rep of the rotational symmetry group of the cube in spin ℓ is the number of ways to write ℓ as an unordered sum of 4, 6 and at most one 9.

For the tetrahedron, we embed its vertices as four vertices of the cube. We then define:

V of degree 4 from the tet’s vertices, a full invariant
E of degree 3 from the tet’s edge-centre axes, a full invariant

And the B we defined for the embedding cube serves as a full invariant of the tet, of degree 6.

B2 can be expressed in terms of V, E and P, so we use B at most once.

So the number of copies of the trivial rep of the rotational symmetry group of the tetrahedron in spin ℓ is the number of ways to write ℓ as a sum of 3, 4 and at most one 6.

All of this stuff reminds me of a baby version of the theory of modular forms. For example, the algebra of modular forms is graded by ‘weight’, and it’s the free commutative algebra on a guy of weight 4 and a guy of weight 6. So, the dimension of the space of modular forms of weight k is the number of ways of writing k as an unordered sum of 4’s and 6’s. Since the least common multiple of 4 and 6 is 12, we get a pattern that ‘repeats’, in a certain sense, mod 12. Here I’m talking about the simplest sort of modular forms, based on the group \mathrm{SL}_2(\mathbb{Z}). But there are lots of variants, and I have the feeling that this post is secretly about some sort of variant based on finite subgroups of \mathrm{SL}(2,\mathbb{C}) instead of infinite discrete subgroups.

There’s a lot more to say about all this, but I have to stop or I’ll never stop. Please ask questions and if you want me to say more!

This entry was posted on Sunday, December 31st, 2017 at 1:00 am and is filed under mathematics, physics. You can follow any responses to this entry through the RSS 2.0 feed. You can leave a response, or trackback from your own site.

56 Responses to Quantum Mechanics and the Dodecahedron

  1. duetosymmetry says:
    31 December, 2017 at 2:27 am

    Looks like you copy/pasted the URL of the gif for the R polynomial in place of the S polynomial, which is here: http://math.ucr.edu/home/baez/mathematical/stein_invariants/stein_icosahedral_invariant_S.gif

    Reply
  2. Blake Stacey says:
    31 December, 2017 at 5:01 am

    Typos: four instances of “latex” missing before \mathrm and \mathbb.

    For the details, see Wikipedia, which manages to make it look harder than it is.

    How does Wikipedia do that so darn well?

    Reply
    • John Baez says:
      1 January, 2018 at 6:41 pm

      Thanks! I thought this stuff was much too nice to make people scour our long conversation for the facts and force them to mentally assemble these facts into a clear picture themselves.

      Reply
    • John Baez says:
      1 January, 2018 at 7:00 pm

      Thanks for catching those flaws. Fixed!

      How does Wikipedia do that so darn well?

      Get a volunteer army of grad students from across the world to explain math they’ve just learned but don’t understand very well?

      Reply
  3. vznvzn says:
    31 December, 2017 at 8:58 pm

    :star: <3 nice! came here after google recommended it in my newsfeed and thx to google for actually recommending a wordpress blog instead of something merely from the MSM!
    general content reminds me of this brilliant paper by gilet on 2d circular wavefns, and believe it can be readily expanded to 3d to get similar results as those youre analyzing. ps it would be nice if your blog allowed wordpress “likes” :)

    http://dotwave.org/quantumlike-statistics-of-deterministic-waveparticle-interactions-in-a-circular-cavity/

    more on related areas

    latest on killing copenhagen interpretation via fluid dynamics

    Reply
  4. Akshat says:
    1 January, 2018 at 4:58 am

    There happens to be a nice, albeit toy-ish, physical interpretation:

    The buckminsterfullerene (C60) molecule has the same symmetry group as the icosahedron. The many-nuclei wavefunction of a rotational eigenstate of the molecule needs to have the same symmetries, because the 12C nuclei are bosons. This then becomes exactly the same problem as the one considered here. The result is that only the \ell = 0, 6, \dots eigenvalues are permitted, \ell = 30 is permitted and doubly degenerate, etc.

    One can also think of what happens if you put fermions on the same molecule. (From my limited knowledge of physics, anyons don’t exist in 3 dimensions, do they?)

    Reply
    • John Baez says:
      1 January, 2018 at 6:55 pm

      Is there published work on buckminsterfullerene that works out the permitted values of \ell? I’d really like to see that… it would be great to have a real-world application of this math.

      The theory with fermions should also be very interesting. In my post I used a graded algebra that’s the direct sum of all the spin-\ell representations for

      \ell = 0, 1, 2, \dots

      but there’s also a bigger one that’s the direct sum of all the spin-\ell representations for

      \ell = 0 , \frac{1}{2}, 1, \frac{3}{2}, \dots

      The binary icosahedral group 2 \mathrm{I} acts on this and one can look at the invariant elements, which form a subalgebra. This should be closely connected to the work of Klein, who figured out generators and relations for the 2 \mathrm{I}-invariant polynomials on the spin-\frac{1}{2} representation \mathbb{C}^2. I describe those generators and relations here:

      • From the icosahedron to E8.

      Okay, now I’m psyched up to work this out! Greg and Bruce Bartlett and I have already done a lot of the necessary calculations.

      And yes, there are no anyons in 3 or more dimensions.

      Reply
      • colin says:
        1 January, 2018 at 9:10 pm

        I am glad to see your interest rekindled. The application side of this work seems most interesting and wide.

        Reply
      • Akshat says:
        2 January, 2018 at 3:49 am

        I don’t know of published work on the problem, unfortunately. This was just an amusing problem from an amusing professor. I’ll remember to ask him if he knows of any, though, and whether he has given some thought to the fermionic case (or, indeed, other interesting extensions of the problem).

        Thanks for the link! Do you plan on posting the calculations you perform here (or on Google+, perhaps)? I would have loved to get involved, but there are some chores to attend to…

        Reply
    • John Baez says:
      2 January, 2018 at 4:05 pm

      Here’s a chart of buckyball energy levels from Wikipedia:

      I don’t know how this is calculated or how the icosahedral symmetry is used. The rotational symmetry group \mathrm{I} has irreducible unitary representations of dimensions 1, 3, 3, 4 and 5. I believe all these representations are complexifications of real reps.

      They write:

      Buckminsterfullerene is one of the largest objects exhibiting wave–particle duality; as stated in the theory every object exhibits this behavior.

      The compound is stable, withstanding high temperatures and high pressures. The exposed surface of the structure can selectively react with other species while maintaining the spherical geometry. Beamexperiments conducted between 1985 and 1990 provided more evidence for the stability of C60 while supporting the closed-cage structural theory and predicting some of the bulk properties such a molecule would have. Around this time, intense theoretical group theory activity also predicted that C60 should have only four infrared-active vibrational bands, on account of its icosahedral symmetry.

      I don’t know if ‘theoretical group activity’ means ‘activity by groups of theorists’ or ‘activity by group theorists’.

      Reply
      • Akshat says:
        2 January, 2018 at 5:52 pm

        I believe the Wikipedia picture describes how the spectrum of a Hamiltonian that is rotationally invariant, and hence has a 2l+1 degeneracy for each l (not caring about the two spins they’ve shown), is split by a perturbation that has the \hat{I} symmetry. The symbols on the right are just physics/chemistry-speak for the irreps of \hat{I}.

        “Crystal field splitting” calculations of this sort are covered in many treatments of group theory in physics (e.g. Landau’s Course, Volume 3, Section 96).

        The electrons of the molecule sit in the potential produced by its nuclei, which you could presumably write as a sum of a rotationally invariant function and one with icosahedral symmetry.

        Reply
      • duetosymmetry says:
        2 January, 2018 at 10:11 pm

        The Wikipedia page is alluding to something more complicated than what we’ve discussed: namely, the vibrational structure.

        Actually, let me back up. The electronic structure is already more complicated than what we were discussing, because (1) it’s fermionic, not bosonic; and (2) it’s actually a many-electron wavefunction, not the simplistic single-electron wavefunction we usually think of.

        But then there’s the comment you quoted, about vibrational bands. Besides the electronic structure, we could also worry about vibrations of the whole molecule. For small enough vibrations, we could use linear theory and decompose the displacements into radial and tangential deformations. The radial components can be decomposed into ordinary spherical harmonics, but the tangential components must be decomposed into vector spherical harmonics, of “electric” and “magnetic” type.

        There’s clearly more fun in store, but it’s not for the faint of heart!

        Reply
        • Akshat says:
          3 January, 2018 at 4:32 am

          The structure of the vibrational spectrum (or a zero-th approximation to it) is actually not that difficult! It’s just a matter of writing down the representation of \hat{I} under which the normal mode coordinates transform, and decomposing it into the irreps.

          SO(3) isn’t involved in this; I’m pretty sure that John’s Wikipedia image describes crystal field splitting. The electron’s fermionic statistics doesn’t mean that the wavefunction has to be symmetric under icosahedral transformations. If electron-electron interactions didn’t play a part (not a very good assumption, but the whole discussion is on toy models), then the spectrum should in fact look like the picture’s right hand side. And after you fill this with independent electrons, you can just antisymmetrize their many-body wavefunction as the usual Slater determinant.

          Hope this wasn’t too incoherent!

        • John Baez says:
          3 January, 2018 at 5:58 pm

          That made sense. But there should be a nice paper on this, somewhere, which fills in all the details. I’m not sure I want to dive into buckminsterfullerology. But some very good group theorists have done so, so there’s a lot to learn:

          • Fan R. K. Chung , Bertram Kostant and Shlomo Sternberg, Groups and the buckyball.

          Kostant and Sternberg were respected (almost feared) teachers of mine back when I was a grad student. This article starts with things I understand well…. but then it bumps into the outer automorphism of \mathrm{S}_6 and shoots off into hyperspace.

      • R.B. says:
        18 November, 2019 at 6:50 pm

        Infrared active eigenmodes (i.e. symmetry adapted coordinates, that also describe (resonant) vibrational motions) are those which change the dipole moment of the molecule. The transform all like the threefold degenerate ungerade representation called Tu in Mulliken notation.

        Reply
  5. Layra says:
    1 January, 2018 at 6:17 am

    In your lists of icosahedrally invariant polynomials you missed the l = 16 case of QR.

    Reply
  6. Greg Egan says:
    1 January, 2018 at 11:58 am

    This is a great write-up of the results! I wouldn’t have had the energy to do this. And it was interesting to see how you handled the restriction of the polynomials to the sphere.

    Reply
  7. nad says:
    2 January, 2018 at 4:20 pm

    John wrote:

    Now I want to use two nice facts. First, G_\ell is the spin-\ell representation of \mathrm{SO}(3).

    I am not sure whether I understand this. That is how is here a degree \ell polynomial as a representative of a base function in [Q^q R^r S^s] to be understood as a representation of a rotation?

    Reply
    • John Baez says:
      2 January, 2018 at 5:38 pm

      Not “a representation of a rotation”, but “a representation of the group of rotations, SO(3)”. A representation of a group G is a vector space V equipped with a linear transformation T(g): V → V for each g in G, such that

      T(gh) = T(g) T(h)

      and

      T(1) = 1

      The space of degree-ℓ polynomials in 3 variables is a representation of SO(3) in an obvious way. From this we can extract, in the manner I explained, the spin-ℓ representation of SO(3). The spin-ℓ representation has dimension (2ℓ+1), while the space of degree-ℓ polynomials in three variables is considerably larger.

      Reply
      • nad says:
        2 January, 2018 at 7:07 pm

        John wrote:

        A representation of a group G is a vector space V equipped with a linear transformation T(g): V → V for each g in G, such that…

        Yes and T(g) represents a group element (here a rotation).
        So I would like to know how exactly is a T(g) expressed in terms of the basis consisting of equivalence classes
        [Q^q R^r S^s] . Do you use conjugation in a Clifford algebras for that?

        The space of degree-ℓ polynomials in 3 variables is a representation of SO(3) in an obvious way. From this we can extract, in the manner I explained, the spin-ℓ representation of SO(3).

        Sorry where exactly did you explain this in the post, I may have overlooked something but I can’t find this in the post.

        Reply
        • John Baez says:
          2 January, 2018 at 7:53 pm

          Nad wrote:

          So I would like to know how exactly is a T(g) expressed in terms of the basis consisting of equivalence classes [Q^q R^r S^s]. Do you use conjugation in a Clifford algebras for that?

          No, I was trying to avoid all explicit formulas, so I used a standard principle in math: if you have a group acting on some set, and you build new set from that old set in a functorial way, the group also acts on this new set.

          Rotations act on \mathbb{R}^3. So, rotations act on anything functorially built from \mathbb{R}^3. For example, they act on the algebra of all polynomials on \mathbb{R}^3. They also act on this algebra modulo the ideal generated by P = x^2 + y^2 + z^2, because this polynomial is invariant under rotations. I used F to stand for this algebra of polynomials mod P. F is isomorphic to an algebra of functions on the sphere. Rotations also act on F_\ell, which is the subspace of F coming from polynomials of degree \le \ell. So, they also act on G_\ell = F_\ell / F_{\ell - 1}. That’s the logic.

          The space of degree-ℓ polynomials in 3 variables is a representation of SO(3) in an obvious way. From this we can extract, in the manner I explained, the spin-ℓ representation of SO(3).

          Sorry where exactly did you explain this in the post, I may have overlooked something but I can’t find this in the post.

          It’s right around here:

          Now I want to use two nice facts. First, G_\ell is the spin-\ell representation of \mathrm{SO}(3).

          I defined the vector space Gℓ in a rather abstract way, which I reviewed just now. But since it was built from things that the rotation group acts on, it’s obviously some representation of SO(3). It’s more work to show that it’s the spin-ℓ representation. But that’s ‘well-known’, so I didn’t show it: I just stated it.

          If you want to check it, show that its dimension is 2ℓ+1 and that it has a cyclic vector. That implies it’s an irreducible representation of SO(3) with dimension 2ℓ+1. And that implies it’s isomorphic to the spin-ℓ representation.

          This may be frustratingly abstract. Greg Egan took a more concrete approach and probably has everything programmed into Mathematica. I believe he likes to think of the spin-ℓ representation as the space of degree-ℓ polynomials on \mathbb{R}^3 that obey Laplace’s equation. These are called [regular solid harmonics-(https://en.wikipedia.org/wiki/Solid_harmonics), and they restrict, on the sphere, to spherical harmonics. That’s a fine approach, but I felt it was a bit distracting to bring Laplace’s equation into the game.

        • nad says:
          2 January, 2018 at 10:56 pm

          John wrote:

          “I believe he likes to think of the spin-ℓ representation as the space of degree-ℓ polynomials on \mathbb{R}^3 that obey Laplace’s equation. “

          I just saw that meanwhile some couple of hours ago he has written something:
          https://plus.google.com/113086553300459368002/posts/bhp6yYZEX4u
          there he -similarily like me seems to ask himself- how the rotations relate to the polynomials. In the post he uses a special sub algebra of a special Clifford algebra, namely the quaternions to construct a polynomial (which he then can interpret then though as a higher dimensional analog of a spherical harmonic. hm?)
          I am way to tired now to read and understand whats written here:
          https://en.wikipedia.org/wiki/Clifford_algebra#Properties
          but this is basically the direction of my question.
          (I don’t have currently access to a library, i.e. a book on representation theory.) I mean how do you know that this is a Spin representation with dimension 2ℓ+1 if there is not some concrete construction?

        • John Baez says:
          2 January, 2018 at 11:53 pm

          Nad wrote:

          In the post he uses a special subalgebra of a special Clifford algebra, namely the quaternions, to construct a polynomial (which he then can interpret then though as a higher dimensional analog of a spherical harmonic. hm?)

          Yeah, the theory of spherical harmonics generalizes to any dimension.

          I mean how do you know that this is a Spin representation with dimension 2l+1 if there is not some concrete construction?

          I gave one way to do this in my last comment (which I have edited many times, so you may not have read this):

          If you want to check it, show that its dimension is 2ℓ+1 and that it has a cyclic vector. That implies it’s an irreducible representation of SO(3) with dimension 2ℓ+1. And that implies it’s isomorphic to the spin-ℓ representation.

          Another nice way is to show that this space Gℓ is isomorphic to the space of degree-ℓ harmonic polynomials on \mathbb{R}^3: that is, polynomials that obey Laplace’s equation. Both these tricks are ways of killing off the ‘extra redundant junk’ I discussed in the Postscript, leaving you with just the spin-ℓ rep.

          Of course I’m using lots of tricks here. You can also just work everything out using coordinates and lots of explicit calculations! That’s fine too.

        • Layra says:
          3 January, 2018 at 3:12 am

          The functions of the form [Q^qR^rS^s] don’t actually form a representation of SO(3). They form a basis of the I-invariant functions on the sphere, F^I, but since being I-invariant isn’t preserved under the action of SO(3), F^I doesn’t yield a representation of SO(3).
          Rather, what we have is SO(3) acting on the usual three-dimensional space, and thus on polynomials in three variables, call them x, y and z. Since rotation is linear, it sends linear functions to linear functions, and hence doesn’t change the degrees of polynomials. Hence the spaces of homogeneous polynomials in three variables give representations of SO(3).

          For me, the easiest way to see that the degree \ell polynomials yield a spin \ell representation is to look at the effects of rotations on eigenvectors (if you’re willing to pass into complex stuff). Take u = x + iy, v = x – iy; then u^{\ell} lives in the complexified space of degree \ell polynomials, and a rotation by t acts on it by e^{i \ell t}u^{\ell}. Hence there is a spin \ell representation as a subspace of the homogeneous degree \ell polynomials.

          As a subgroup of SO(3), the group I acts on these spaces of homogeneous polynomials. P = P(x,y,z), Q = Q(x,y,z), R = R(x,y,z) and S = S(x,y,z) are all homogeneous polynomials chosen to be invariant under I, and they generate the algebra of I-invariant polynomials in three variables. Restricting to the sphere gives us F^I, and then taking associated graded stuff gives us G^I, which are still all I-invariant. But at this point we’ve mostly lost any connection to SO(3).

        • John Baez says:
          3 January, 2018 at 4:06 am

          Layra wrote:

          The functions of the form [Q^qR^rS^s] don’t actually form a representation of SO(3).

          Right. I never said they did, but I should have been more aggressive in correcting Nad’s impression.

          By the way, you used the LaTeX command \script{l}, which doesn’t work here. (Does it work anywhere?) I replaced it with \ell, which is the basic way you make an \ell in LaTeX.

        • Layra says:
          3 January, 2018 at 4:36 am

          I think I might be used to some packages which has a \script command. Not sure.

        • nad says:
          3 January, 2018 at 11:14 am

          The functions of the form [Q^qR^rS^s] don’t actually form a representation of SO(3).

          Depends on what you mean by “form a representation”. As a basis in G_l you can represent a linear transformation on G_l (i.e a representation in G_l ) as a matrix in this basis, I would call this a representation is formed in the basis of [Q^qR^rS^s] But is this a spin representation? So basically I was asking how concretely the action of SO(3) in [Q^qR^rS^s] is defined.

          They form a basis of the I-invariant functions on the sphere, F^I, but since being I-invariant isn’t preserved under the action of SO(3), F^I doesn’t yield a representation of SO(3).

          I imagine the invariant functions as a “kind of representation” of the set of symmetry axis’ and maybe the set of faces which map onto itself under the symmetries of the polytope. So yes under some arbitray rotations (i.e. not symmetry rotations) these thus get mapped to some other set of axis’ (and faces). But by the above one should still be able to express this collection in the above basis (?). Now since geometric algebras are very losely speaking some way of seeing structured sets of “vectors” as “basis vectors” I had the vague imagination that they appear somewhere here as a means to represent those sets of axis’ and faces. And Greg Egans post now seems to point also in this direction. But as said I just wanted to try to understand all this to at least some rough extend and thus in particular find the right image. And I had hoped that this was easier. I also looked in the wikipedia articles on Spin representations with Clifford algebras or exterior algebras, but I found those not really instructive especially for the above.

          So thanks John and Layra for trying to explain the above to me, but I fear this gets a bit too complicated for the limited time I might dedicate to this.

        • John Baez says:
          3 January, 2018 at 5:54 pm

          Nad wrote:

          So basically I was asking how concretely the action of SO(3) in [Q^qR^rS^s] is defined.

          As Layra explained, there’s no action of SO(3) on the space spanned by the elements [Q^qR^rS^s]. These are functions invariant under the symmetries of an icosahedron in fixed position. If you rotate such a function, you don’t get another such function.

          I never said there was a representation of SO(3) on this space. I used a representation of SO(3) on various other spaces, like the space G_\ell.

        • nad says:
          3 January, 2018 at 8:20 pm

          Layra wrote

          but since being I-invariant isn’t preserved under the action of SO(3), F^I doesn’t yield a representation of SO(3).

          John wrote:

          If you rotate such a function, you don’t get another such function.

          OK I think I now see what you mean. For me this was not so obvious that if I rotate such a function then that this is not anymore a function in G_\ell^{\mathrm{I}} – that may have irritated me.

          Thanks again.

  8. Tim Silverman says:
    3 January, 2018 at 1:02 pm

    Reducing integers mod N, we get a projection of \mathrm{PSL}\left(2,\mathbb{Z}\right) to \mathrm{PSL}\left(2,\mathbb{Z}/N\mathbb{Z}\right). Now, \mathrm{PSL}\left(2,\mathbb{Z}/3\mathbb{Z}\right)=\mathrm{PSL}\left(2,3\right)\simeq T (the rotational symmetry group of the tetrahedron), \mathrm{PSL}\left(2,\mathbb{Z}/4\mathbb{Z}\right)\simeq O (octahedral rotations) and \mathrm{PSL}\left(2,\mathbb{Z}/5\mathbb{Z}\right)=\mathrm{PSL}\left(2,5\right)\simeq I. Likewise for N=6 we get the symmetries of a tiling of the torus by 12 hexagons; for N=7 we get the symmetries of the Klein Quartic (with its heptagonal tiling); and so on. So these things presumably do lift to modular functions of level N.

    Reply
    • John Baez says:
      3 January, 2018 at 5:42 pm

      That’s a promising sign! But why should a PSL(2,5)-invariant real-algebraic function on the sphere give a modular function of level 5? We can think of this sphere as the Riemann sphere, and the usual action of the icosahedral group on the sphere gives a complex-algebraic action of PSL(2,5) on the Riemann sphere… but there’s still a gap I don’t see how to fill, between the world of real-algebraic functions and the world of complex-analytic functions.

      Maybe I’m not looking at things in the best way. It would be nice to find a connection with modular functions. Maybe I should proceed numerologically and look at some information about modular functions, or forms, at level 5.

      Reply
      • duetosymmetry says:
        3 January, 2018 at 6:18 pm

        Yes, we can think of the sphere as the Riemann sphere… but this story can’t fit inside an SO(3) story, because SO(3) is compact, while the conformal group SL(2,R) is non-compact…

        Reply
      • John Baez says:
        4 January, 2018 at 6:22 am

        I believe the point is this. The congruence subgroup

        \displaystyle{ \Gamma(n) = \left\{ \left(\begin{array}{cc} a & b \\ c & d \end{array}\right) \in \mathrm{SL}(2,\mathbb{Z}) : a, d \equiv 1 \pmod n, \quad b, c \equiv 0 \pmod n \right\} }

        acts on the upper half-plane \mathrm{H} as conformal transformations. The quotient \mathrm{H}/\Gamma(n) is called a modular curve. And the group \mathrm{SL}(2,\mathbb{Z}/n) acts as conformal transformations on this modular curve.

        For n = 3,4,5 the modular curve \mathrm{H}/\Gamma(n) can be identified with the Riemann sphere—at least after we compactify it by throwing in a point at infinity. In these three cases the groups \mathrm{SL}(2,\mathbb{Z}/n) are the binary tetrahedral, binary octahedral and binary icosahedral groups—that is, double covers of the rotational groups of the tetrahedron, octahedron and icosahedron. And they act on the Riemann sphere in a manner that preserves a tetrahedron, octahedron and icosahedron inscribed in this sphere, respectively.

        This is the stuff Tim Silverman was alluding to. I think this math goes back to Felix Klein. He then went on to the case n =7, and the rest is history.

        Reply
        • duetosymmetry says:
          4 January, 2018 at 8:12 am

          Well, I was much too hasty! I hadn’t thought of finite subgroups of SL(2,R) which also happen to be finite subgroups of SO(3). This seems like a kind of “coincidence” to me. SO(3) and SL(2,R) have the same dimension but different topology so I’m certainly not going to fine one inside the other. But I hadn’t realized that their finite subgroups intersect! (I know essentially nothing about the finite subgroups of SL(2,R))

        • John Baez says:
          4 January, 2018 at 4:01 pm

          I hadn’t thought of finite subgroups of SL(2,R) which also happen to be finite subgroups of SO(3).

          Those groups aren’t very interesting. I said the binary tetrahedral, octahedral and icosahedral groups are finite subgroups of SU(2) that are also finite quotient groups of SL(2,Z).

          I know essentially nothing about the finite subgroups of SL(2,R).

          They’re all cyclic groups, \mathbb{Z}/n.

          Any finite subgroup of a Lie group G is compact so it must sit inside a maximal compact subgroup K ⊂ G. The existence of a maximal compact subgroup is a nontrivial theorem, but it’s true, and it’s good to learn the maximal compact subgroups of all your favorite Lie groups. For SL(2,R), every maximal compact subgroup is conjugate to SO(2). So, every finite subgroup of SL(2,R) is conjugate to a subgroup of SO(2). So, every finite subgroup of SL(2,R) is a cyclic group!

        • duetosymmetry says:
          4 January, 2018 at 4:23 pm

          Argh, so I’m still not reading sufficiently carefully. So to form these binary tetrahedral/octahedral/icosahedral groups, we first reduce from SL(2,R) to SL(2,Z) [fn1], then look at quotient groups? Now I really don’t have intuition for how quotients act on the Riemann sphere. Any pedagogical sources for this?

          [fn1] Am I right in saying that SL(2,R) is the group of conformal transformation on the complex plane? But now we’re talking about SL(2,Z) instead—is that just to focus on integer lattices in the complex plane instead?

        • John Baez says:
          4 January, 2018 at 5:24 pm

          So to form these binary tetrahedral/octahedral/icosahedral groups, we first reduce from SL(2,R) to SL(2,Z) , then look at quotient groups?

          Right. This is part of a big branch of math called the theory of modular curves. A modular curve is what you get when you take the upper half-plane and mod out by a discrete subgroup of SL(2,R). It’s called a curve because it’s of complex dimension 1. The theory of modular curves is important in number theory: for example, it’s what Wiles used to prove Fermat’s Last Theorem.

          Now I really don’t have intuition for how quotients act on the Riemann sphere. Any pedagogical sources for this?

          I don’t think you can do much better than the blog series by my friend Tim Silverman, who started this discussion. He wrote a bunch of posts, but the first one already gets you to the Platonic solids:

        • John Baez says:
          4 January, 2018 at 5:33 pm

          Am I right in saying that SL(2,R) is the group of conformal transformation on the complex plane?

          Not quite. The only conformal transformations of the complex plane are translations, rotations and dilations. It’s much better to include a point at infinity and consider the Riemann sphere. SL(2,C) acts as conformal transformations of the Riemann sphere via fractional linear transformations

          \displaystyle{ z \mapsto \frac{a z + b}{c z + d} }

          SL(2,R) is the subgroup that preserves the upper half-plane H. The upper half-plane has a metric making it into the ‘hyperbolic plane’, and SL(2,R) acts as isometries. If you’re a physicist, you want to think of SL(2,R) as the double cover of SO(2,1), which acts on 3d Minkowski spacetime, and the upper half-plane as the hyperboloid

          t^2 - x^2 - y^2 = 1, \qquad t > 0

          which is naturally a copy of the hyperbolic plane. To get number theory into the game we need to look at SL(2,Z) and its congruence subgroups like the groups Γ(n) that I was just talking about.

  9. Raphael says:
    4 January, 2018 at 9:25 pm

    Great post and thread! Anyone happens being able to explain the relation between icosahedral symmetry and “natural numbers that cannot be expressed as sum of one or more nontrivial binomial coefficients.”? As a matter of fact this is the description of the finite sequence 1, 2, 3, 4, 5, 7, 8, 9, 11, 13, 14, 17, 19, 23, 29 in OEIS (https://oeis.org/A210576).

    Reply
    • John Baez says:
      4 January, 2018 at 11:29 pm

      That’s a nice observation. I think I understand it. From the icosahedral point of view, the important thing about this list of numbers is that they’re the natural numbers that can’t be written as a sum of 6’s, 10’s and 15’s. Our study of the icosahedron, explained in this post, revealed the importance of the numbers 6, 10 and 15.

      On the other hand, 6, 10 and 15 are the first 3 nontrivial binomial coefficients. And it just so happens that any number that can’t be written as a sum of these can’t be written as a sum of nontrivial binomial coefficients at all!

      This is pretty easy to see. The next binomial coefficient, 21, doesn’t help get you new sums because 21 = 6 + 15. The one after that, 28, doesn’t help get you new sums because 28 = 6 + 6 + 6 + 10. And all the binomial coefficients after that don’t help at all because they’re bigger than 30, and every number greater than or equal to 30 is a sum of 6’s, 10’s, and 15’s.

      (In fact you only need to use at most one 15 in this sum.)

      All this reminds me of another interesting property of the number 30. It’s the largest natural number such that all natural numbers smaller than it and relatively prime to it are actually prime—except, of course, for 1:

      7, 11, 13, 17, 19, 23, 29

      This list is contained in your list. I don’t see any significance except that the niceness of the icosahedron is closely connected to it having a very ’round’ number of rotational symmetries, namely 60. The Babylonians liked this number because it was divisible by 2, 3, 5 and even 12… so of course sadistic Babylonian school-teachers gave homework where students had to divide by 7. (A tablet has been found with this homework problem on it.)

      Reply
      • Raphael says:
        4 January, 2018 at 11:54 pm

        Makes sense, thank you! One is tempted to tell OEIS about the alternative description of A210576 as “Numbers that are no sums of 6,10 and 15.”, but then it’s a short list, so maybe its not too big a thing that it can be defined in various short ways.

        Reply
  10. John Baez says:
    5 January, 2018 at 12:18 am

    Wow! Layra has cracked the general proplem of which we were doing special cases:

    • Layra Idarani, SG-invariant polynomials.

    Namely, he takes any Coxeter group G acting on its vector space V and answers this puzzle:

    Puzzle. What’s the dimension of the space homogeneous harmonic polynomials of degree k on V that are invariant under the even part of G.

    Answer. Any Coxeter group has a list of numbers d_1 \le \cdots \le d_n associated to it, and the answer to the puzzle is how many ways you can write k as an unordered sum of d_is for i > 1 and at most one copy of

    d_q = (\sum_{i=1}^n d_i) - n

    These lists of numbers associated to Coxeter groups are explained in week186 and week187, but Layra says what these lists are. For the symmetry group of the icosahedron the list is

    2, 6, 10

    so the answer to the puzzle is: the number of ways we can write k as a sum of 6s, 10s and at most one 15. Which is what we’d already seen!

    But the list for \mathrm{E}_8 is

    2, 8, 12, 14, 18, 20, 24, 30

    so we can now do this case as well. The dimension of the space of degree-k harmonic polynomials on \mathbb{R}^8 that are invariant under the even part of the Weyl group of \mathrm{E}_8 is the number of ways you can write k as an unordered sum of 2s, 8s, 12s, 14s, 18s, 20s, 24s, 30s and at most one 120.

    Reply
  11. The Kepler Problem and the 600-Cell | Azimuth says:
    7 January, 2018 at 11:18 pm

    Layra Idarani has come up with a complete classification of all eigenfunctions of the Laplacian on S^3 that are invariant under this group… or more generally, eigenfunctions of the Laplacian on a sphere of any dimension that are invariant under the even part of any Coxeter group. For the details, go here:

    • Layra Idarani, SG-invariant polynomials, 4 January 2018.

    All that is a continuation of a story whose beginning is summarized here:

    • John Baez, Quantum mechanics and the dodecahedron.

    So, there’s a lot of serious math under the hood. But right now I just want to marvel at the fact that we’ve found a wavefunction for the hydrogen atom that not only has a well-defined energy, but is also invariant under this 7,200-element group. This group includes the usual 60 rotational symmetries of a dodecahedron, but also other much less obvious symmetries.

    Reply
  12. Victor V Albert says:
    4 November, 2019 at 8:07 pm

    Thanks for this post; it helped me with my work, which I was looking forward to sharing here. We develop quantum error-correcting codes for the rigid rotor and its relatives. H-symmetric harmonics are one of our tools, and we obtain them by symmetrizing the ordinary harmonics (be it for \mathrm{SO}_3 or the two-sphere) over the group H. I’m sure this isn’t new, but haven’t quite seen it spelled out the same way. We also formulate a “coordinates statement” of Peter-Weyl on homogeneous spaces. I would be interested in comments and any refs I missed! https://scirate.com/arxiv/1911.00099

    Reply
    • John Baez says:
      5 November, 2019 at 4:04 am

      I’m busy grading midterms and preparing for classes but I hope someday I have time to look at your paper!

      Reply
    • R.B. says:
      5 November, 2019 at 5:51 am

      Interesting (and long) paper! Never got in touch with quantum computing before but to me it seems to be closely related to microwave spectroscopy and theoretical chemistry, though the language is a physics/maths one (Z_3 versus C_{3v}, …).

      Reply
      • Victor V Albert says:
        18 November, 2019 at 6:15 pm

        The paper tries to push quantum computing in the direction of rotational state spaces, which have been thoroughly studied in spectroscopy. I try to include all the jargon for the groups in the text to make it easier (Z_3 = C_3 and $latex $C_\infty = SO(2)=U(1)$).

        Reply
        • R.B. says:
          18 November, 2019 at 6:41 pm

          This a very good idea, I am sure it will help attracting more interest from people with knowledge on spectroscopy!

        • R.B. says:
          18 November, 2019 at 6:43 pm

          P.S.: Strange, I must have posted this about one year ago (at leat quite a few months) or so. The timeline thoroughly confuses (if not scares) me ..

  13. An attempt to understand the Monster group | Complex Projective 4-Space says:
    29 November, 2020 at 9:19 pm

    We could also define A5 as the group of rotations which fix the following degree-6 polynomial (x − φy)(y − φz)(z − φx)(x + φy)(y + φz)(z + φx), which is isomorphic to Greg Egan’s potential function discussed here. This is mildly (but not precisely*) analogous to the description of the Monster as the automorphisms of the Griess algebra. Note that the polynomial is clearly invariant under the monomial subgroup A4, and with some effort can be shown to be invariant under the full group A5.

    Reply
  14. christian d roth says:
    22 September, 2022 at 9:39 am

    Hi John Baez
    Thank you for that post! It means a lot to me. If you consider the possibility of magnesium (12!) to form the dodecahedron configuration, then we could reach a break through in the understanding of photosynthesis. Its crystal like structures (chlorophyll esp. porphyrin ring) transform the molecules “vibrations” (chaotic movements) to 3d symmetrical impacts on magnesium by four nitrogen atoms with three free valence electrons each.
    I know the conflict with Paulis exclusion principle, but I am considering nature to be smart enough to find a way around it. Superposition??
    (Sorry, I’m an engineer not mathematician nor physicist and therefore cannot follow or use your formal language, but I am working on the same question in a more practical approach.)
    Life has to use the ideal distribution of energy in order to overcome the spontaneous processes. In the end almost all living creatures gain their energy for the most part from photosynthesis. The solution to that seems to me to be Platos and Keplers dodecahedron representing the “aether”: the most dense symmetric form of energy. You just have to align the electrons to it. By doing so, you transform “vibrational” energy to spin energy. Photosynthesis does this with magnesium in a quasi crystal structure (just with one atom) what can be done by men creating superconductors.
    Is that comprehensible for you?

    Reply

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