REVIEW
An Introduction to Spin Foam Models of Quantum Gravity and BF Theory
General Relativity and Quantum Cosmology · Submitted 21 May 1999 · 16 references
Pith's verdict: A genuinely useful, honest introduction to spin foams that knows exactly where its subject runs out of road; the soft spots are the field's, not the exposition's.
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Referee report
The paper
The paper claims
Baez argues that the quantum geometry of spacetime can be written as a sum over labelled two-dimensional diagrams, and that BF theory is the cleanest place to see why.
The reading
What carries the argument
The load-bearing device is the spin foam itself: a 2-dimensional oriented cell complex whose faces are labelled by irreducible representations of the gauge group and whose edges are labelled by intertwiners between the tensor products of the incident faces. It is defined to be exactly the one-dimension-higher analogue of a spin network, so that a generic slice of a spin foam is a spin network, which is what lets the same object serve as both a quantum state of space and a quantum history of spacetime. The computational engine is the group-integration identity $int dg, rho_1(g) ⊗ rho_2(g) ⊗ rho_3(g) = sum_iota iota iota^*$ (and its four-factor version), which is the statement that both sides project onto the trivial representation; applying it once per dual edge converts the ill-defined product of Dirac deltas into a sum over intertwiners, and the vertex amplitude becomes the evaluation of a small spin network dual to a tetrahedron or 4-simplex. A second device, the q-deformation, replaces $G$ by $U_q g$ with $q = exp(2pi i/(k+h))$; because only finitely many representations survive as 'good', the previously divergent sums become finite.
Extended reading notes
Core claim
The paper's central claim is that spin networks and spin foams are not analogies but the actual output of quantizing a specific, exactly solvable theory. Start with BF theory on an $n$-manifold, with a connection $A$ and an ad-valued $(n-2)$-form $E$, and Lagrangian $L = tr(E wedge F)$. Its field equations, $F = 0$ and $d_A E = 0$, say the connection is flat and $E$ is covariantly closed, so there are no local degrees of freedom. Canonical quantization then gives a gauge-invariant Hilbert space spanned by spin network states, and the operator measuring $E$ over an $(n-2)$-surface acts on a spin network edge labelled by $j$ with eigenvalue proportional to $sqrt{j(j+1)}$ — so length in 3d and area in 4d come out discrete. Path-integral quantization, discretized on the dual 2-skeleton of a triangulation, gives a partition function that is a sum over labellings of dual faces by irreducible representations and dual edges by intertwiners, with each dual vertex contributing a small spin network (a tetrahedron in 3d, a 4-simplex in 4d) evaluated by the usual graphical rules. Baez's point is that this same machinery, with the group replaced by a quantum group, survives the addition of a cosmological term: in 3 dimensions the modified BF action is a difference of two Chern-Simons actions at level $k = 4pi/sqrt{Lambda}$, which yields the Turaev-Viro model with finitely many allowed spins and hence finite, triangulation-independent amplitudes. In 4 dimensions the analogue gives a one-dimensional physical Hilbert space and the Chern-Simons state, and imposing the constraint $E = e wedge e$ — concretely, $|E^+| = |E^-|$ in the self-dual/anti-self-dual splitting — leads to the Barrett-Crane intertwiner and a candidate spin foam model of Riemannian quantum gravity.
Load-bearing premise
The whole path-integral story is told on the dual 2-skeleton of one fixed triangulation, and the author states outright that for a theory with local degrees of freedom like 4-dimensional gravity there is no known justification for that restriction — triangulation independence was a consequence of BF theory having no local degrees of freedom, not a general feature.
Editorial extensions
If this is right
- Length in 3-dimensional Riemannian quantum gravity and area in 4-dimensional BF theory have discrete spectra, with a spin-$j$ edge contributing $sqrt{j(j+1)}$ to any curve or surface it crosses, and using $SO(3)$ instead of $SU(2)$ thins the spectrum to integer spins only.
- 3-dimensional general relativity with a cosmological constant is exactly two copies of Chern-Simons theory at levels $pm k$, so its Hilbert space and time-evolution operators factorize into Chern-Simons data.
- In 4-dimensional BF theory with a cosmological term, the physical Hilbert space is one-dimensional for any compact oriented 3-manifold, and the unique state is the Chern-Simons state, gauge-invariant precisely when $k = 12pi/Lambda$ is an integer.
- Spin foam faces in 4 dimensions give area to surfaces they intersect and spin foam edges give 3-volume to 3-dimensional submanifolds, continuing the pattern by which spin network edges give area and vertices give volume in space.
- The Barrett-Crane intertwiner $iota = sum_j (2j+1)(iota_j ⊗ iota_j)$ is the unique labelling that enforces equal self-dual and anti-self-dual flux under all three ways of splitting a tetrahedron, which singles out one candidate model of 4-dimensional Riemannian quantum gravity.
Reading between the lines
- If the discrete area and length spectra are taken seriously, then a cosmological constant sets a maximum spin and hence a maximum length in 3 dimensions, so the theory would predict both a smallest and a largest geometric scale from two different constants — a pairing that is checkable in principle against any regime where both $hbar$ and $Lambda$ matter.
- The fact that BF theory's partition function converges exactly in the cases where the moduli space of flat connections carries a natural measure suggests the divergence problem is not a technical nuisance but a signal about which dimensions admit a well-defined notion of 'volume of the space of flat connections' at all.
- Because 4-dimensional general relativity has local degrees of freedom while BF theory does not, the fixed-triangulation restriction is plausibly the real dividing line: a spin foam model of gravity would need its amplitudes to be refinement-independent for a reason other than the absence of local excitations, and no such reason is on offer here.
- The observation that spin foam vertices should give 4-volume to regions of spacetime, but that this has not been computed, marks a concrete near-term calculation: evaluating the 4-simplex amplitude's dependence on the ten face spins and matching it against a Regge-style volume would test whether the model has the right semiclassical geometry.
Original abstract
In loop quantum gravity we now have a clear picture of the quantum geometry of space, thanks in part to the theory of spin networks. The concept of `spin foam' is intended to serve as a similar picture for the quantum geometry of spacetime. In general, a spin network is a graph with edges labelled by representations and vertices labelled by intertwining operators. Similarly, a spin foam is a 2-dimensional complex with faces labelled by representations and edges labelled by intertwining operators. In a `spin foam model' we describe states as linear combinations of spin networks and compute transition amplitudes as sums over spin foams. This paper aims to provide a self-contained introduction to spin foam models of quantum gravity and a simpler field theory called BF theory.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
In loop quantum gravity we now have a clear picture of the quantum geometry of space, thanks in part to the theory of spin networks. The concept of `spin foam' is intended to serve as a similar picture for the quantum geometry of spacetime. In general, a spin network is a graph with edges labelled by representations and vertices labelled by intertwining operators. Similarly, a spin foam is a 2-dimensional complex with faces labelled by representations and edges labelled by intertwining operators. In a `spin foam model' we describe states as linear combinations of spin networks and compute transition amplitudes as sums over spin foams. This paper aims to provide a self-contained introduction to spin foam models of quantum gravity and a simpler field theory called BF theory.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | In loop quantum gravity we now have a clear picture of the quantum geometry of space, thanks in part to the theory of spin networks. | background 1.00 | 0.08 | 0.04 | asserted 1.00 |
| s1 | The concept of `spin foam' is intended to serve as a similar picture for the quantum geometry of spacetime. | background 0.98 | 0.06 | 0.05 | asserted 0.79 |
| s2 | In general, a spin network is a graph with edges labelled by representations and vertices labelled by intertwining operators. | background 1.00 | 0.04 | 0.02 | asserted 1.00 |
| s3 | Similarly, a spin foam is a 2-dimensional complex with faces labelled by representations and edges labelled by intertwining operators. | background 0.99 | 0.06 | 0.03 | asserted 1.00 |
| s4 | In a `spin foam model' we describe states as linear combinations of spin networks and compute transition amplitudes as sums over spin foams. | method 0.56 | 0.10 | 0.06 | asserted 1.00 |
| s5 | This paper aims to provide a self-contained introduction to spin foam models of quantum gravity and a simpler field theory called BF theory. | contribution 0.97 | 0.33 | 0.09 | asserted 0.86 |
What was examined, and what was not
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References
How later papers used it
114 later papers cite it
3 later papers by other authors are listed below: 2 used its method or tool and 1 compared its own results with it.
Uses its method or tool 2 of 3 papers with this label
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Used this paper's standard computations of group integrals to obtain the spin foam picture of its model from its formula.
A New Class of Group Field Theories for 1st Order Discrete Quantum Gravity (2007) · 0.93 · paraphrased: the licence does not allow quoting
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Used a discretization involving spin foams from this paper to define its path integral.
Group field theories (2012) · 0.96 · paraphrased: the licence does not allow quoting
Compares with it 1 of 3 papers with this label
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Showed how its saddle point method recovers the results presented in this paper in the simplest case of BF theory in dimension 2.
Quantum Corrections in the Group Field Theory Formulation of the EPRL/FK Models (2010) · 0.90 · paraphrased: the licence does not allow quoting
How the literature uses it
116 arXiv papers cite this in 169 sentences
Papers citing it · 74 sentences without a confident label
Uses its method or tool 3 papers
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Since the boundary BF theory coupled to a bulk gravity can be decomposed classically into a closed form just like the $B$ field in a pure BF theory and a fixed, non-closed form determined by the coupling, one may first quantize the SO$(1,1)$ pure BF theory in loop-quantization formalism [ref] , setting up the complete basis of the boundary Hilbert space, and then use the quantum version of coupling term [the first equality of ([ref])] to choose suitable bulk spin network states via triangulations on a section of the IH defined by boundary `spin-network' states.
The entropy of isolated horizons in non-minimally coupling scalar field theory from BF theory · The second approach · 0.94
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Going through the standard computations [ref] of group integrals, we can obtain from this formula the spin foam picture of our model.
A New Class of Group Field Theories for 1st Order Discrete Quantum Gravity · The new models: action and Feynman amplitudes · 0.93
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To actually define the path integral we use a discretization involving spin foams [ref] .
Group field theories · Discretization of BF theories · 0.96
Compares with it 3 papers
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As a largely simplified explanation, a trivially satisfied constraint equation on the allowed irreducible representation labels in a closed subgraph of the foam admits an unbounded sum over all possible labelings of edges by half-integer representations [ref] .
Network Gravity · Bubble Divergences · 0.83
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The peculiar feature of the divergence of $c_j^(n)$ is reminiscent of the infrared divergence encountered in many spin-foam models [ref] and the regularization may correspond to a nonzero cosmological constant [ref] .
Loop quantum cosmology with higher order holonomy corrections · Summary and discussion · 0.81
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To close this section, let us see how the saddle point method allows us to recover the results presented in [ref] in the simplest case of BF theory in dimension 2.
Quantum Corrections in the Group Field Theory Formulation of the EPRL/FK Models · Two dimensional case · 0.90
Cites it as background 72 papers
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In the absence of a cosmological constant, non-perturbative quantization in the canonical approach, the loop quantum gravity (LQG) based on the BF formulation of gravity [ref] , and the covariant approach, based on spin foams and more precisely the Ponzano-Regge model [ref] , give consistent results.
Spinor Representation of the Hamiltonian Constraint in 3D LQG with a Non-zero Cosmological Constant · Introduction · 0.96
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This idea goes back to Rovelli and Reisenberger ( [ref] , see [ref] for a review), and lies at the foundation of spin foam models as understood in the context of Loop Quantum Gravity.[The mathematical concept as abstract state sum model is much older (see e.g. literature in [ref] ), but differs slightly from the way spin foams are understood in this article.]
On knottings in the physical Hilbert space of LQG as given by the EPRL model · Introduction · 0.92
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Let us start with a brief review of the relevant properties of BF theory [ref] , a topological field theory formulated on the principal bundle of a group $G$ over the spacetime manifold $ℳ$.
Topological Features of the Quantum Vacuum · Constructing the action · 0.99
Discussion
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