May 12, 1996

This Week's Finds in Mathematical Physics (Week 81)

John Baez

I think I'll take a little break on the continuing saga of n-categories. Instead I'll talk about something which is secretly the very same subject, namely loop groups and their central extensions. This is important in string theory. But first I want to say a bit about some very high-energy physics.

1) D. J. Bird et al, Detection of a cosmic ray with measured energy well beyond the expected spectral cutoff due to cosmic microwave radiation, preprint available as astro-ph/9410067

P. Bhattacharjee and G. Sigl, Monopole annihilation and highest energy cosmic rays, preprint available as astro-ph/9412053.

R.J. Protheroe and P.A. Johnson, Are topological defects responsible for the 300 EeV cosmic rays?, preprint available as astro-ph/9605006.

In 1994, folks at the Fly's Eye air shower detector in Utah observed a cosmic ray whose energy was about 320 EeV. In case you forget what an EeV is, it's a unit of energy equal to a billion GeV, and a Gev is equal to a billion ev (electron volts). Current particle accelerators routinely particles with energies about a hundred GeV, but a few hundred EeV is a whole different story! That's about 50 joules, the energy of a one-kilogram mass moving at 10 meters/second, all packed in one particle!

Nobody knows what would produce cosmic rays of this energy. To make the puzzle more mysterious, this energy is above the Greisen-Zatsepin- Kuz'min (or GZK) cutoff for cosmic rays produced at moderate extragalactic distances (30 megaparsecs). The idea of the GZK cutoff is that particles of extremely high energies whizzing through space would interact significantly with the cosmic microwave background radiation, losing energy to produce pions.

So it seems that something is producing really high energy particles, and this something is not too far away, by cosmic standards. Established mechanisms don't get energies that high. A possibility studied by various authors including P. Bhattacharjee and G. Sigl is that these super-energetic cosmic rays are produced by the decay of "topological defects". Various grand unified theories, or GUTs, predict that the strong, weak, and electromagnetic forces all act the the same at really high temperatures, while at low temperatures (like any sort of temperature you'd find around here) a "spontaneous symmetry breaking" occurs which makes them split up into their observed distinct personalities.

Mathematically this is a bit like how a magnet at low temperatures randomly picks out a certain axis of magnetization, breaking the rotational symmetry it possesses at high temperatures. And like in the case of a magnet, one would expect the possibility of "topological defects" where different regions of space pick different ways to break the symmetry, leaving nasty spots like lumps in the carpet that can't be straightened out. Ordinary magnets typically exhibit 2-dimensional "domain walls" between domains having different axes of magnetization. But in various GUTs folks have considered, one can also get 1-dimensional "cosmic strings" and 0-dimensional "topological solitons" including magnetic monopoles --- particles with magnetic charge. None of these topological defects have ever been observed, despite a fair amount of searching. Could super-energetic cosmic rays be the result of a monopole-antimonopole collision?

Alas, Protheroe and Johnson's paper argues that in such decays lots of the energy would go into the production of high-energy γ rays... more than has been observed in the super-energetic cosmic ray showers. So maybe the puzzle has some other answer.

The weekend before last I went to the 11th Geometry Festival, which was held at the University of Maryland. Since I work on quantum gravity, I could be said to be a geometer of sorts --- perhaps a quantum geometer. But geometry means a lot of different things to different people, and this conference concentrated on some aspects of geometry that I don't know much about. In particular, there were talks by Schmuel Weinberger, Bruce Kleiner and G. Wei on the implications of positive and negative curvature for Riemannian geometry.

A talk that was right up my alley was given by Jean-Luc Brylinski. It dealt with themes from his papers with McLaughlin:

2) Jean-Luc Brylinski and Dennis A. McLaughlin, The geometry of degree four characteristic classes and of line bundles on loop spaces, I, Duke Math. Journal 75 (1994), 603-638. II, Duke Math. Journal 83 (1996), 105-139.

Jean-Luc Brylinski, Central extensions and reciprocity laws, preprint.

Jean-Luc Brylinski, Coadjoint orbits of central extensions of gauge groups, preprint.

Jean-Luc Brylinski and Dennis A. McLaughlin, The geometry of two dimensional symbols, preprint.

Let me say a bit about the math underlying these papers, the basic stuff that they build on. One hot topic in mathematical physics in the last decade has been the study of "loop groups". Say you take any Lie group G. Then the "loop group" LG is the set of smooth functions from the circle to G. This becomes a group with pointwise multiplication as the group operation. This sort of group shows up in 2-dimensional quantum field theory, where spacetime could be the cylinder. Then "space" is the circle, and if we are studying gauge theory with gauge group G, the group of gauge transformations over space would be the loop group LG. One main reason for being interested in 2-dimensional quantum field theory is string theory: here we think of the 2-dimensional worldsheet of the string as a spacetime in its own right, and we are often interested in doing gauge theory over this spacetime. For this reason, folks in string theory need to understand all they can about unitary representations of loop groups.

Actually they are interested in projective representations of loop groups. Remember, in quantum mechanics two vectors in a Hilbert space give the same expectation values for any observable if they differ only by a phase. So it is perfectly fine for a group representation R to satisfy the usual law

R(g)R(h) = R(gh)

where g,h are group elements, only up to a phase. So in the definition of a projective representation we weaken the above requirement to

R(g) R(h) = c(g,h) R(gh)

where c(g,h) is a phase depending on g and h. Folks call c(g,h) the "cocycle" of the projective representation.

A projective unitary representation of a group H can also be thought of as a representation of a bigger group H~ called a "central extension" of H. The idea is that this bigger group has a bunch of phases built into it to absorb the phase ambiguities in the projective representation of H. Let U(1) be the unit circle in the complex plane, a group under multiplication. This is the group of phases. We can think of H~ as H x U(1) given a sneaky product designed to soak up the phases produced by the cocycle:

(g, a)(h, b) = (gh, ab c(g,h))

We can define a unitary representation S of H~ as follows:

S(g, a) = R(g)a

It's then obvious that

S(g, a) S(h, b) = S((g, a)(h, b))

so S is really a representation. For this reason, if we are doing quantum theory and we don't like projective representations, it's okay as long as we understand the central extensions of our group of symmetries.

So, instead of thinking about projective representations of loop groups, we can think about central extensions of loop groups. How does one get ahold of these? There is a nice trick which Brylinski described in his talk. To get this trick, we need to assume a bit about the group G. Let's assume it's a connected and simply-connected simple Lie group. I'll explain that in a minute, but some good examples to keep in mind are SU(n) and Spin(n); see "week61" for the definitions and a bit of information about these groups.

Now remember that S^k stands for the k-dimensional sphere, and π_k(X) of a topological space X stands for the set of continuous maps from S^k to X, modulo homotopy. In other words, two continuous maps from S^k to X define the same element of π_k(X) if one can be continously deformed to the other.

Saying that G is connected means that π_0(G) = 0. To understand this you need to realize that S^0 consists of two points. So π_0(G) = 0 means that G consists of one piece, any two points of which can be connected by a continuous path.

Saying that G is simply connected means that π_1(G) = 0. In other words, all loops in G can be "pulled tight". A good example of a group that's NOT simply connected is the group SO(n) of rotations in n dimensional space.. This flaw with SO(n) is why they needed to invent Spin(n); see "week61".

As it turns out, every Lie group has π_2(G) = 0. So all 2-spheres in G can be pulled tight too. Imagine taking a balloon and sticking it in G; then you can always shrink it down to a point in a continuous way without it getting stuck around a hole in G.

Saying that G is simple is an algebraic rather than topological condition, and I explained this condition in "week63". But it has topological ramifications. It implies, for example, that π_3(G) = Z, the group of integers. So to each way of sticking a 3-sphere in G we can associate an integer. One way to compute this integer involves the Killing form on the Lie algebra of G. This is a special inner product on the Lie algebra of G. Using this inner product and the bracket in the Lie algebra we can convert 3 vectors u, v, and w in the Lie algebra into a number as follows:

W(u,v,w) = k <[u,v],w>

Here k is a constant that will make life simpler later. The special property of the Killing form implies that W is totally antisymmetric, and we can use left multiplication to translate W all over the group G obtaining a closed 3-form on G. Call this 3-form W, too. Then, given any smooth function from S^3 into G we can pull back W to S^3 and integrate it over S^3. If we choose the constant k right, the result will be an integer --- the integer we were looking for.

Hmm, this is getting technical. Well, it'll keep getting more technical. Just stop reading when it becomes unpleasant.

Okay, these topological facts about the group G have a bunch of cool consequences. One trick usually goes by the name of the "WZW action", which refers to Wess, Zumino, and Witten. Say we have smooth function f from S^2 to G. Since pi_2(G) = 0 we can extend f to a smooth function F from the 3-dimensional ball, D^3, to G. (This is just another way of "pulling the balloon tight" as mentioned above.) Now we can use F to pull back the magic 3-form W to D^3, and then we can integrate the resulting 3-form over D^3 to get a number S(f) called the Wess-Zumino-Witten action.

Unfortunately, this number depends on the choice of the function F extending f to the ball. Fortunately, it doesn't depend too much on F. Say we extended f to some other function F' from the ball to G. Then F together with F' define a map from S^3 to G, and we know from the previous stuff that the integral of the pullback of W over this S^3 is an integer. So changing our choice of an extension of f only changes S(f) by an integer. This means that the exponential of the WZW action:

exp(2 π i S(f))

is completely well-defined. This is nice in quantum physics, where the exponential of the action is what really matters. Note also that this exponential is just a phase! So we are getting a function

A: Maps(S^2,G) → U(1)

assigning a phase to any map f from S^2 to G.

Now Maps(S^2,G) is sort of like the loop group, since the loop group is just Maps(S^1,G). In particular, it too becomes a group by pointwise multiplication. A bit of calculation shows that A above is a group homomorphism:

A(f) A(g) = A(fg).

This homomorphism is the key to finding the central extension of the loop group. Here's how we do it. By now everyone but the experts has probably fallen asleep at the screen, so I can pull out all the stops.

Here's a useful way to think of a central extensions: a central extension H~ of the group H by the group U(1) is a special sort of short exact sequence of groups:

                 1 → U(1) → H~ → H → 1

By "short exact sequence of groups" I simply mean that U(1) is a subgroup of H~ and that H~ modulo U(1) is H. What's special about central extensions is that U(1) is in the center of H~. You can check that this definition of central extension matches up with our earlier more lowbrow definition.

Now how do we get this short exact sequence? Well, it comes from a short exact sequence of spaces:

                 * → S^1 → D^2 → S^2 → *

This diagram means simply that we can think of the circle as a subspace of the 2-dimensional disc D^2 in an obvious way, and then if we collapse this circle to a point the disc gets squashed down to a 2-sphere. Now, from this short exact sequence we get a short exact sequence of groups
        1 → Maps(S^2,G) → Maps(D^2,G) → Maps(S^1,G) → 1

In other words, Maps(S^2,G) is a normal subgroup of Maps(D^2,G), and if we mod out by this subgroup we get Maps(S^1,G). Now we can use the homomorphism A: Maps(S^2,G) → U(1) to get ourselves another exact sequence like this:
                          i               j
        1 → Maps(S^2,G) → Maps(D^2,G) → Maps(S^1,G) → 1
                |              |              |
              A |              |              | 1
                v              v              v
        1 →  U(1) ----------> L~  --------> Maps(S^1,G) → 1


Remembering that Maps(S^1,G) is the loop group, L~ turns out to be the desired central extension! Concretely we can think of L~ as a quotient group of Maps(D^2,G) x U(1) by the subgroup of pairs of the form (i(f),A(f)) with f in Maps(S^2,G).

There is something fascinating about how spheres of different dimensions --- S^0, S^1, S^2, and S^3 --- conspire together with the topology of the group G to yield the central extension of the loop group LG. It appears that what we are really studying are the closely related cohomology groups:

H^0(Maps(S^3,G)) which is just another way of saying π_3(G)

H^1(Maps(S^2,G)) which describes homomorphisms from Maps(S^2,G) to U(1)

H^2(Maps(S^1,G)) which describes central extensions of Maps(S^1,G)

and

H^3(Maps(S^0,G)) which is just another way of saying H^3(G), where W lives

There is a fourth term in this series which I didn't get around to talking about; it's

H^4(BG) where the degree 4 characteristic class for G-bundles, e.g. the 2nd Chern class for SU(n), lives

Here BG is the "classifying space" of G. I would like to understand more deeply what's going on with this series, because the different terms have a lot to do with physics in different dimensions --- dimensions 0 to 4, the "low dimensions" which are so specially interesting.

I should conclude by noting that while a lot of this appeared in Brylinski's talk, and a lot of it is probably common knowledge among topologists, it was in some conversations with James Dolan that we worked out some of the patterns I mention here.


© 1996 John Baez
baez@math.removethis.ucr.andthis.edu