### Why Higher Geometric Quantization

The largest single presentation was a pair of talks on “The Motivation for Higher Geometric Quantum Field Theory” by Urs Schreiber, running to about two and a half hours, based on these notes. This was probably the clearest introduction I’ve seen so far to the motivation for the program he’s been developing for several years. Broadly, the idea is to develop a higher-categorical analog of geometric quantization (GQ for short).

One guiding idea behind this is that we should really be interested in quantization over (higher) stacks, rather than merely spaces. This leads inexorably to a higher-categorical version of GQ itself. The starting point, though, is that the defining features of stacks capture two crucial principles from physics: the gauge principle, and locality. The gauge principle means that we need to keep track not just of connections, but gauge transformations, which form respectively the objects and morphisms of a groupoid. “Locality” means that these groupoids of configurations of a physical field on spacetime is determined by its local configuration on regions as small as you like (together with information about how to glue together the data on small regions into larger regions).

Some particularly simple cases can be described globally: a scalar field gives the space of all scalar functions, namely maps into ; sigma models generalise this to the space of maps for some other target space. These are determined by their values pointwise, so of course are local.

More generally, physicists think of a field theory as given by a fibre bundle (the previous examples being described by trivial bundles ), where the fields are sections of the bundle. Lagrangian physics is then described by a form on the jet bundle of , i.e. the bundle whose fibre over consists of the space describing the possible first derivatives of a section over that point.

More generally, a field theory gives a procedure for taking some space with structure – say a (pseudo-)Riemannian manifold – and produce a moduli space of fields. The Sigma models happen to be *representable functors*: for some , the representing object. A prestack is just any functor taking to a moduli space of fields. A stack is one which has a “descent condition”, which amounts to the condition of locality: knowing values on small neighbourhoods and how to glue them together determines values on larger neighborhoods.

The Yoneda lemma says that, for reasonable notions of “space”, the category from which we picked target spaces embeds into the category of stacks over (Riemannian manifolds, for instance) and that the embedding is faithful – so we should just think of this as a generalization of space. However, it’s a generalization we need, because gauge theories determine non-representable stacks. What’s more, the “space” of sections of one of these fibred stacks is also a stack, and this is what plays the role of the moduli space for gauge theory! For higher gauge theories, we will need higher stacks.

All of the above is the classical situation: the next issue is how to quantize such a theory. It involves a generalization of Geometric Quantization (GQ for short). Now a physicist who actually uses GQ will find this perspective weird, but it flows from just the same logic as the usual method.

In ordinary GQ, you have some classical system described by a phase space, a manifold equipped with a pre-symplectic 2-form . Intuitively, describes how the space, locally, can be split into conjugate variables. In the phase space for a particle in -space, these “position” and “momentum” variables, and ; many other systems have analogous conjugate variables. But what really matters is the form itself, or rather its cohomology class.

Then one wants to build a Hilbert space describing the quantum analog of the system, but in fact, you need a little more than to do this. The Hilbert space is a space of sections of some bundle whose sections look like copies of the complex numbers, called the “prequantum line bundle“. It needs to be equipped with a connection, whose curvature is a 2-form in the class of : in general, . (If is not symplectic, i.e. is degenerate, this implies there’s some symmetry on , in which case the line bundle had better be equivariant so that physically equivalent situations correspond to the same state). The easy case is the trivial bundle, so that we get a space of functions, like (for some measure compatible with ). In general, though, this function-space picture only makes sense locally in : this is why the choice of prequantum line bundle is important to the interpretation of the quantized theory.

Since the crucial geometric thing here is a bundle over the moduli space, when the space is a stack, and in the context of higher gauge theory, it’s natural to seek analogous constructions using higher bundles. This would involve, instead of a (pre-)symplectic 2-form , an -form called a (pre-)-plectic form (for an introductory look at this, see Chris Rogers’ paper on the case over manifolds). This will give a higher analog of the Hilbert space.

Now, maps between Hilbert spaces in QG come from Lagrangian correspondences – these might be maps of moduli spaces, but in general they consist of a “space of trajectories” equipped with maps into a space of incoming and outgoing configurations. This is a *span* of pre-symplectic spaces (equipped with pre-quantum line bundles) that satisfies some nice geometric conditions which make it possible to push a section of said line bundle through the correspondence. Since each prequantum line bundle can be seen as maps out of the configuration space into a classifying space (for , or in general an -group of phases), we get a square. The action functional is a cell that fills this square (see the end of 2.1.3 in Urs’ notes). This is a diagrammatic way to describe the usual GQ construction: the advantage is that it can then be repeated in the more general setting without much change.

This much is about as far as Urs got in his talk, but the notes go further, talking about how to extend this to infinity-stacks, and how the Dold-Kan correspondence tells us nicer descriptions of what we get when linearizing – since quantization puts us into an Abelian category.

I enjoyed these talks, although they were long and Urs came out looking pretty exhausted, because while I’ve seen several others on this program, this was the first time I’ve seen it discussed from the beginning, with a lot of motivation. This was presumably because we had a physically-minded part of the audience, whereas I’ve mostly seen these for mathematicians, and usually they come in somewhere in the middle and being more time-limited miss out some of the details and the motivation. The end result made it quite a natural development. Overall, very helpful!

November 16, 2014 at 4:58 pm

How does one generate space-time itself in this formalism?

November 16, 2014 at 6:27 pm

One doesn’t: this formalism only becomes relevant once space-time is already around.

Presumably, among the jobs of a truly unified theory of physics would be to account for the geometry of spacetime as well as the fields that live on it simultaneously. That is, do both of the jobs currently done by quantum field theory and general relativity. Right now, each of GR and QFT assume that the other has done its job (GR finds spacetime geometry that expresses the gravitational effect of some given matter fields, and QFT calculates the behaviour of matter on a given geometry). In some special cases, we can combine them by looking for solutions to both problems which are consistent with each other, but (a) it’s only possible in very special situations like highly symmetric universes, and (b) still quite hard.

This approach lives firmly on the quantum field theory side of that split – so presumably it’s not the end of the story as far as physics goes. But it does help address some of the mathematical problems with QFT, which is the less mathematically rigorous of the two. Hopefully that’s a step toward a theory that really combines both jobs.

December 1, 2014 at 2:33 am

Sounds great. Have you tried attacking the emergent spacetime problem from a cat theoretic perspective? The lesson, from the string/M-theory side, seems to be that noncommutative geometry plays a role, at least from the worldvolume perspective. The gauge symmetries can be viewed as symmetries of brane configurations, e.g., U(3) symmetry from three coincident branes. The matrix theory approach takes a C*-algebra, which describes such configurations in their fully noncommutative coordinates. And from the lesson of Connes, it’s better to focus on the spectral geometry of the brane configuration. So in an abstract sense, one can study the worldvolume in terms of its C*-algebra bundle structure (and its associated bundle of spectral noncommutative topological spaces).