Originally posted by Hurkyl
I have this feeling that figuring out what a densitized triad is will help intuit the other things.
But basically, I'm just hoping to be able to follow at least one of these papers from the beginning to the end without having to skip over anything.
I will try to copy in the most condensed description I've seen so far and maybe it can serve as focus. This is Ashtekar talking to mathematicians at a June 2001 conference at Stonybrook. The style is mathly as opposed to physish (fewer indices) so it is easier to copy in. Maybe I will eventually be able to get thru these few paragraphs (!) without skipping. Or at least can point to specific hard spots. I feel somewhat the same as you just said, Hurkyl, and want to focus on some exposition condensed enough to get into one PF post. Also want to see how difficult it is to transcribe Ashtekar's notation.
Quote from Asktekar "Quantum Geometry in Action..." Section 2
arXiv:math-ph/0202008 (Feb. 2002)
"Let me now turn to specifics. It is perhaps simplest to begin with a Hamiltonian or symplectic description of general relativity. The phase space is the cotangent bundle. The configuration variable is a connection, A on a fixed 3-manifold Σ representing 'space' and (as in gauge theories) the momenta are the 'electric field' 2-forms E, both of which take values in the Lie-algebra of SU(2). In the present gravitational context, the momenta acquire a geometrical significance: their Hodge-duals *E can be naturally interpreted as orthonormal triads (with density weight 1) and determine the dynamical, Riemannian geometry of Σ. Thus, (in contrast to Wheeler's geometrodynamics) the Riemannian structures on Σ are now built from momentum variables. The basic kinematic objects are holonomies of A, which dictate how spinors are parallel transported along curves, and the 2-forms E, which determine the Riemannian metric of Σ. (Matter couplings to gravity have also been studied extensively [2, 1].)
In the quantum theory, the fundamental excitations of geometry are most conveniently expressed in terms of holonomies [3, 4]. They are thus one-dimensional, polymer-like and, in analogy with gauge theories, can be thought of as 'flux lines of the electric field'. More precisely, they turn out to be flux lines of areas: an elementary flux line deposits a quantum of area on any 2-surface S it intersects. Thus, if quantum geometry were to be excited along just a few flux lines, most surfaces would have zero area and the quantum state would not at all resemble a classical geometry. Semi-classical geometries can result only if a huge number of these elementary excitations are superposed in suitably dense configurations [13, 14]. The state of quantum geometry around you, for example, must have so many elementary excitations that about 10
68 of them intersect the sheet of paper you are reading, to endow it an area of about 100 cm
2. Even in such states, the geometry is still distributional, concentrated on the underlying elementary flux lines; but if suitably coarse-grained, it can be approximated by a smooth metric. Thus, the continuum picture is only an approximation that arises from coarse graining of semi-classical states.
These quantum states span a specific Hilbert space H = L
2(
A; dμ
o), consisting of functions on the space of (suitably generalized) connections which are square integrable with respect to a natural, diffeomorphism invariant (regular, Borel) measure μ
o. This space is very large. However, it can be conveniently decomposed into a family of orthonormal, finite dimensional sub-spaces H=SUM
γ, j H
γ, j, labelled by finite graphs γ each edge of which itself is labelled by a non-trivial irreducible representation of SU(2) (or, a half-integer, or a spin j) [5]. H
γ, j can be regarded as the Hilbert space of a `spin-system'. These spaces are extremely simple to work with; this is why very explicit calculations are feasible. Elements of H
γ, j are referred to as spin-network states [5].
As one would expect from the structure of the classical theory, the basic quantum operators are the holonomies ^h
p along paths p in Σ and the triads ^*E [6]. Both sets of operators are densely defined and self-adjoint on H. Furthermore, a striking result is that all eigenvalues of the triad operators are discrete. This key property is, in essence, the origin of the fundamental discreteness of quantum geometry. For, just as the classical Riemannian geometry of Σ is determined by the triads *E, all Riemannian geometry operators----such as the area operator ^A
S associated with a 2-surface S or the volume operator ^V
R associated with a region R----are constructed from ^*E. However, since even the classical quantities A
S and V
R are non-polynomial functionals of the triads, the construction of the corresponding ^A
S and ^V
R is quite subtle and requires a great deal of care. But their final expressions are rather simple [6].
In this regularization, the underlying background independence turns out to be a blessing. For, diffeomorphism invariance constrains the possible forms of the final expressions severely and the detailed calculations then serve essentially to fix numerical coefficients and other details. Let us illustrate this point with the example of the area operators ^A
S. Since they are associated with 2-surfaces S while the states have 1-dimensional support, the diffeomorphism covariance requires that the action of ^A
S on a state Ψ
γ, j must be concentrated at the intersections of S with γ. The detailed expression bears out this fact: the action of ^A
S on Ψ
γ, j is dictated simply by the spin labels j
I attached to those edges of γ which intersect S. For all surfaces S and 3-dimensional regions R in Σ, ^A
S and ^V
R are densely defined, self-adjoint operators.
All their eigenvalues are discrete. [6]..."
My comment: The notation here differs in minor ways from what's found elsewhere and I have tried to adhere to Ashtekar's notation as much as typographically possible. Make any corrections you see to make, if comparing this with the original paper. Here a hat ^ preceding a symbol says it is an operator. Also the underlying 3D manifold is Σ instead of M, and the 2D surface whose area is to be measured is S. The spin network is written with a lowercase γ instead of the uppercase Γ we've seen elsewhere. Was tempted to change this, but decided best to stick consistently to Ashtekar's notation in this quote.