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under construction

On the formalization of the process of quantization – by abstract nonsense – from classical ∞-model? data to the corresponding quantum field theory .

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Background and motivation

The search is on for the abstract formalization of the process of quantization – the process that reads in a “classical field theory” – for instance presented in form of a gauge theory or in form of a ∞-model? background field data – and spits out the corresponding quantum field theory.

There is an open problem of mathematical (-physics) model building:

One that is to quantization as, say, symplectic geometry is to Hamiltonian mechanics?

The formalism of FQFT clearly suggests that the fundamental description of quantization is some natural operation on higher functors.

While for various aspects and facets of this question there are well-developed formalisms – such as geometric quantization or deformation quantization or BV-BRST formalism – a full answer is certainly still missing, not the least because the full formalization of the question itself has still to be established.

Considerable progress on this formulation of the question has been achieved with the formalization and proof of the cobordism hypothesis in On the Classification of Topological Field Theories by Jacob Lurie. This at least indicates what the result of any full quantization procedure should be in that it clarifies what exactly a TQFT FQFT is: a morphism from the (∞,n)-category of cobordisms Z:Bord nCZ : Bord_n \to C.

In On the Classification of Topological Field Theories Jacob Lurie indicates some first towards finding a similar formalization of “classical field theory” (in terms of his (,n)(\infty,n)-categories of “families”) and a systematic procedure for turning the classical theory into the quantum theory. These thoughts were further developed in the article Topological Quantum Field Theories from Compact Lie Groups . But for the moment, that, too, remains a bit sketchy.

For the purpose of the present entry this indication of a quantizaton proposal by Lurie et al. mainly serves as a reference for the idea itself that a formalization of something interesting is to be sought here, and of the kind of abstract nonsense answer one hopes to find. We will however discuss a somewhat different-looking approach. It may well be related to the Lurie-et al proposal in the end, but for the time being we shall not concentrate on that relation.

Rather, the approach for a formalization of the quantization procedure that shall be discussed at this entry here draws from a few different sources:

  1. The observation that a classical background field that should serve as the input for a quantization of a σ\sigma-model that describes the dynamics of an object charged under this field is encoded by differential cocycles as as described at differential cohomology in an (∞,1)-topos.

  2. The idea that by applying a pull-push quantization prescription a differential cocycle on a target space XX gives rise to a differential cocycle on a parameter space Σ\Sigma, which may be thought of as one of the bordisms appearing in the FQFT-description of quantum field theory.

    The pull-push operation here is akin to that in geometric ∞-function theory, where a quantum field theory is obtained from a ∞-model? target space object XX by homming extended cobordism cospans Σ inΣΣ out\Sigma_in \to \Sigma \leftarrow \Sigma_{out} into the target object and then pull-pushing geometric function objects through the resulting spans of configuration space objects [Σ in,X][Σ,X][Σ out,X][\Sigma_{in},X] \leftarrow [\Sigma,X] \to [\Sigma_{out},X].

    The main result of David Ben-Zvi et. al.‘s work on this approach is that they point out that as soon as the geometric function object one uses satisfies the two fundamental theorems of geometric infinity-function theory, a considerable amount of rich structure that has in parts been known by itself gets unified into one coherent elegant story: the nature of partition functions (i.e. traces), of centers, of Hochschild (co)homology, Deligne-Kontsevich-statements, etc. all are understood by means of a suitable geometric function theory as induced from the underlying geometry of configuration space objects [Σ,X][\Sigma,X] as well as the loop space objects of XX.

    The resulting pull-push operation is an example or a generalization of what John Baez discusses under the term groupoidification.

  3. The observation that a differential coccycle on a Lorentzian manifold Σ\Sigma gives rise to a local net of observables, as used in the formalizaton of QFT known as AQFT. (As described here).

    So the procedure discussed here regards differential cocycles on target space as classicai field theories, regards their quantization as a way to obtain a differential cocycle on Lorentzian parameter space, and identifies this as a quantum field theory by associating a local net of observables to it.

    These local nets, in turn, are akin to factorization algebras, which in the Euclidean (meaning non-Lorentzian setting) relate back to cobordism representations via the notion of topological chiral homology. However the – physically crucial – Lorentzian structure invoked here is not otherwise considered in these functorial axiomatization of quantum field theory.

General ambient structure

The ambient context is the (∞,1)-topos H:=Sh (,1)(CartSp)\mathbf{H} := Sh_{(\infty,1)}(CartSp) of Lie ∞-groupoids and the (,2)(\infty,2)-topos of smooth (,1)(\infty,1)-categories, which we model, respectively, as the left Bousfield localization of the model structure on functors [CartSp op,sSet Quillen][CartSp^{op}, sSet_{Quillen}] and [CartSp op,sSet +][CartSp^{op}, sSet^+], respectively, where

For the definition of the path ∞-groupoid functor Π\mathbf{\Pi} and the induced theory of differential cohomology in an (∞,1)-topos, we make use of the discussion at differential cohomology in an (∞,1)-topos – survey.

When working with fibrant objects in the model, we will frequently use the constructions and notation from category of fibrant objects. Notably for BG\mathbf{B}G a fibrant delooping object in the model we write (BG) I(\mathbf{B}G)^I for the path object we write EG\mathbf{E}G for the pullback

EG * (BG) I d 1 BG \array{ \mathbf{E}G &\to& * \\ \downarrow && \downarrow \\ (\mathbf{B}G)^I &\stackrel{d_1}{\to}& \mathbf{B}G }

and EGBG\mathbf{E}G \to \mathbf{B}G for the remaining map, induced from d 0:(BG) IBGd_0 : (\mathbf{B}G)^I \to \mathbf{B}G.

The charged particle

We describe the general theory for the simple example of the charged particle.

Target space and background field

The background field for the charged particle that we want to consider is the electromagnetic field. The data involved is

  • the target space XX – a smooth manifold;

  • the structure group or gauge group G=U(1)G = U(1);

  • a choice of representation

    ρ:BGVect , \rho : \mathbf{B}G \to Vect_{\mathbb{C}} \,,

    taken to be the canonical representation on V=V = \mathbb{C};

  • the background field given by a

    • a U(1)U(1)-principal bundle PXP \to X classified by a cocycle g:XBU(1)g : X \to \mathbf{B}U(1) in H\mathbf{H} which in the model is given by an anafunctor XYBU(1)X \stackrel{\simeq}{\leftarrow} Y \to \mathbf{B}U(1);

    • a connection \nabla on this bundle, which in the model is given by a diagram

      Y g BU(1) Π(Y) EBU(1), \array{ Y &\stackrel{g}{\to}& \mathbf{B}U(1) \\ \downarrow && \downarrow \\ \mathbf{\Pi}(Y) &\stackrel{\nabla}{\to}& \mathbf{E}\mathbf{B}U(1) } \,,

      and whose field strength is given by the composite

      F:Π(Y)EBU(1)B 2U(1). F : \mathbf{\Pi}(Y) \stackrel{\nabla}{\to} \mathbf{E}\mathbf{B}U(1) \to \mathbf{B}^2 U(1) \,.

Parameter space and kinetic action

Let Σ=\Sigma = \mathbb{R} be the parameter space, the worldline, regarded as a Lorentzian manifold and write Π(Σ)\mathbf{\Pi}(\Sigma) for the Lorentzian path category.

To define the kinetic action, we first form the ρ\rho-associated background field

X g BU(1) ρ Vect Π(X) EBU(1) EBU(1) BU(1)Vect \array{ X &\stackrel{g}{\to}& \mathbf{B}U(1) &\stackrel{\rho}{\to}& Vect \\ \downarrow && \downarrow && \downarrow \\ \mathbf{\Pi}(X) &\stackrel{\nabla}{\to}& \mathbf{E} \mathbf{B}U(1) &\stackrel{}{\to}& \mathbf{E}\mathbf{B}U(1) \coprod_{\mathbf{B}U(1)} Vect }

and then pull this back to the extended configuration space X×ΣX \times \Sigma.

The morphisms in the product category Π(X)×Π(Σ)\mathbf{\Pi}(X) \times \mathbf{\Pi}(\Sigma) are paths γ X:[0,1]X\gamma_X : [0,1] \to X in XX on whose base we have a (pseudo)Riemannian metric, which is the pullback of the metric μ Σ\mu_\Sigma on Σ\Sigma along γ Σ:[0,1]Σ\gamma_\Sigma : [0,1] \to \Sigma. We can consider the kinetic action to be a differential cocycle

Σ×X BU(1) Vect Π(Σ)×Π(X) EBU(1) EBU(1) BU(1)Vect \array{ \Sigma \times X &\stackrel{}{\to}& \mathbf{B}U(1) &\stackrel{}{\to}& Vect \\ \downarrow && \downarrow && \downarrow \\ \mathbf{\Pi}(\Sigma) \times \mathbf{\Pi}(X) &\to& \mathbf{E} \mathbf{B}U(1) &\stackrel{}{\to}& \mathbf{E}\mathbf{B}U(1) \coprod_{\mathbf{B}U(1)} Vect }

which sends the path γ X:[0,1]X\gamma_X : [0,1] \to X of parameter length γ Σ:[0,1]Σ\gamma_\Sigma : [0,1] \to \Sigma to

exp(1i 0 1|γ X| 2dγ Σ. \mathbb{C} \stackrel{\exp(-\frac{1}{i \hbar}\int_{0}^1 |\gamma'_X|^2 d \gamma_\Sigma}{\to} \mathbb{C} \,.

Notice that Π(X)×Π(Σ)Π(X×Σ)\mathbf{\Pi}(X)\times \mathbf{\Pi}(\Sigma) \simeq \mathbf{\Pi}(X \times \Sigma).

The quantization

The total action is differential cocycle

Σ×X Vect Π(Σ)×Π(X) exp(S kin)tra EB BU(1)Vect. \array{ \Sigma \times X &\stackrel{}{\to}& Vect \\ \downarrow && \downarrow \\ \mathbf{\Pi}(\Sigma) \times \mathbf{\Pi}(X) &\stackrel{\exp(S_{kin})tra_\nabla}{\to}& \mathbf{E}\mathbf{B}\mathbb{R} \coprod_{\mathbf{B}U(1)} Vect } \,.

We want to consider the diagram

Σ×X Vect Σ Π(Σ)×Π(X) EBU(1) BU(1)Vect Π(Σ) \array{ \Sigma \times X & \to& Vect \\ \downarrow & \searrow && \searrow \\ \Sigma && \mathbf{\Pi}(\Sigma)\times \mathbf{\Pi}(X) &\to& \mathbf{E}\mathbf{B}U(1)\coprod_{\mathbf{B}U(1)} Vect \\ & \searrow & \downarrow \\ && \mathbf{\Pi}(\Sigma) }

and use it to obtain a differential cocycle on Σ\Sigma, by forming something like a lax pullback (“comma object”) of the point inclusion

* * Vect Vect BU(1)EBU(1), \array{ * &\to& * \\ \downarrow && \downarrow \\ Vect &\to& Vect \coprod_{\mathbf{B}U(1)} \mathbf{E}\mathbf{B}U(1) } \,,

where the left vertical morphism picks the ground field \mathbb{C}, along this cocycle. For the underlying cocycle this is obtained as the ordinary pullback of EVect\mathbf{E}Vect defined as the ordinary pullback

EVect * k Vect I d 1 Vect, \array{ \mathbf{E}Vect &\to& * \\ \downarrow && \downarrow^{\mathrlap{k}} \\ Vect^I &\stackrel{d_1}{\to}& Vect } \,,

where II is the interval category, Vect IVect^I the functor category and k:*Vectk : * \to Vect picks the ground field vector space. Via the remaining map d 0:Vect IVectd_0 : Vect^I \to Vect this maps to VectVect and then further to Vect BU(1)EBU(1)Vect \coprod_{\mathbf{B}U(1)} \mathbf{E}\mathbf{B}U(1).

The pullback of

EVect EVect Vect VectEBU(1) \array{ \mathbf{E}Vect &\to& \mathbf{E}Vect \\ \downarrow && \downarrow \\ Vect &\to& Vect \coprod \mathbf{E}\mathbf{B}U(1) }

along our differential cocycle, i. e. the pullback of the top part of the diagram

EVect Σ×X Vect EVect Σ Π(Σ)×Π(X) EBU(1) BU(1)Vect Π(Σ) \array{ && \mathbf{E}Vect \\ && \downarrow & \searrow \\ \Sigma \times X & \to& Vect && \mathbf{E}Vect \\ \downarrow & \searrow && \searrow & \downarrow \\ \Sigma && \mathbf{\Pi}(\Sigma)\times \mathbf{\Pi}(X) &\to& \mathbf{E}\mathbf{B}U(1)\coprod_{\mathbf{B}U(1)} Vect \\ & \searrow & \downarrow \\ && \mathbf{\Pi}(\Sigma) }

is over X×ΣX \times \Sigma the total space of the pullback of the underlying vector bundle EE on XX to X×ΣX \times \Sigma, and over Π(X×Σ)\mathbf{\Pi}(X \times \Sigma) is a groupoid E ΠE_{\mathbf{\Pi}}

E E Π X×Σ Π(X×Σ) Σ Π(Σ). \array{ E &\to& E_{\mathbf{\Pi}} \\ \downarrow && \downarrow \\ X\times \Sigma &\to& \mathbf{\Pi}(X \times \Sigma) \\ \downarrow && \downarrow \\ \Sigma &\to& \mathbf{\Pi}(\Sigma) } \,.

To see what EE ΠE \to E_{\mathbf{\Pi}} is like, first notice that we have a fibration sequence

V V E V//U(1) * * x X g BU(1) ρ Vect \array{ && && V \\ && && \downarrow \\ V &\to& E &\to & V//U(1) &\to& * \\ \downarrow && \downarrow && \downarrow && \downarrow \\ {*} &\stackrel{x}{\to} &X &\stackrel{g}{\to}& \mathbf{B}U(1) &\stackrel{\rho}{\to}& Vect }

with the bottom right square a lax pullback and everything else homotopy pullbacks. Here VV is the vector space that ρ:BU(1)Vect\rho : \mathbf{B}U(1) \to Vect is a representation on (which for the electromagnetic field will be \mathbb{C} itself).

The groupoid E ΠE_{\mathbf{\Pi}} has the following description:

  • its objects are triples (x,σ,v)(x,\sigma, v), where vE xv \in E_{x} is a vector in the fiber of EE over xx;

  • its morphisms are triples (xγy,σσ,v)(x \stackrel{\gamma}{\to} y, \sigma \to \sigma', v) that go from (x,σ,v)(x,\sigma,v) to (y,σ,exp( 0 1|...|)ρ((γ)))(v)(y, \sigma', \exp(\int_0^1 |...|) \rho(\nabla(\gamma)))(v), i.e. from a vector in the fiber over the source to the corresponding vector in the fiber over the target, obtained by evaluating the action functional on the path.

To obtain from this a cocycle on Σ\Sigma, we proceed as follows: we regard an interval σ:=[σ in,σ out]Π(Σ) 1\sigma := [\sigma_{in}, \sigma_{out}] \in \mathbf{\Pi}(\Sigma)_1 as a cospan

σ in σ σ out σ in Π(σ) σ out, \array{ \sigma_{in} &\to& \sigma &\leftarrow& \sigma_{out} \\ \downarrow && \downarrow && \downarrow \\ \sigma_{in} &\to& \mathbf{\Pi}(\sigma) &\leftarrow& \sigma_{out} \,, }

where in the top row we regard these subsets of Σ\Sigma as discrete smooth sub-categories, and in the bottom row form the path \infty-groupoids.

Then we take sections of E E Π Σ Π(Σ)\array{E &\to& E_{\mathbf{\Pi}}\\ \downarrow && \downarrow \\ \Sigma &\to& \mathbf{\Pi}(\Sigma)} to produce a span of sections

[σ in σ in,E E Π] Σ[σ Π(σ),E E Π] Σ[σ out σ out,E E Π] Σ. \left[ \array{ \sigma_{in} \\ \downarrow \\ \sigma_{in} } \,, \array{ E \\ \downarrow \\ E_{\mathbf{\Pi}} } \right]_\Sigma \leftarrow \left[ \array{ \sigma \\ \downarrow \\ \mathbf{\Pi}(\sigma) } \,, \array{ E \\ \downarrow \\ E_{\mathbf{\Pi}} } \right]_\Sigma \to \left[ \array{ \sigma_{out} \\ \downarrow \\ \sigma_{out} } \,, \array{ E \\ \downarrow \\ E_{\mathbf{\Pi}} } \right]_\Sigma \,.

of smooth \infty-groupoids.

Consider an \infty-groupoid

Ψ[σ in σ in,E E Π] Σ \Psi \to \left[ \array{ \sigma_{in} \\ \downarrow \\ \sigma_{in} } \,, \array{ E \\ \downarrow \\ E_{\mathbf{\Pi}} } \right]_\Sigma

over the left foot. Under groupoid cardinality, if Ψ\Psi is tame, this corresponds to a collection of rational numbers over vectors in fibers of EE. Under “degrupoidification” we may think of this as specifying a section |Ψ|Γ(E)|\Psi| \in \Gamma(E). The above span is supposed to give us the propagation of this state along σ\sigma.

To determine this, consider the special case where Ψ\Psi is a “delta-section”, *(x,σ in,v)* \mapsto (x,\sigma_{in}, v) supported on a single vector vv in a single fiber E xE_x over xx. Then its pull-push through this span yields the \infty-groupoid over EE, which over (y,σ out,w)(y,\sigma_{out},w) consists of the set of paths γ:xy\gamma : x \to y such that w=exp(...)ρ(γ)(v)w = \exp(\int...)\rho(\gamma)(v), i.e. such that ww is the vector obtained from applying the action to vv along this path.

If everything were suitably finite, we could take cardinalities of the result and obtain the familiar path integral (sum)

Ψ(y)= xγyexp(S kin(γ))tra (γ)Ψ(x). \Psi'(y) = \int_{x \stackrel{\gamma}{\to} y} \exp( S_{kin}(\gamma)) tra_\nabla(\gamma) \Psi(x) \,.

Last revised on April 13, 2010 at 10:31:59. See the history of this page for a list of all contributions to it.