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Kiefer C. Quantum gravity

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6<br />

QUANTUM GRAVITY WITH CONNECTIONS AND LOOPS<br />

6.1 Connection and loop variables<br />

In Section 4.3, we encountered a Hamiltonian formulation of GR alternative to<br />

geometrodynamics, using the concepts of connections and loops. In the present<br />

chapter, we shall review approaches to formulate a consistent quantum theory<br />

with such variables, leading to ‘quantum connection dynamics’ or ‘quantum loop<br />

dynamics’. More details and references can be found in Rovelli (2004) and Thiemann<br />

(2001, 2003), Ashtekar and Lewandowski (2004), and Nicolai et al. (2005).<br />

The popular name ‘loop quantum <strong>gravity</strong>’ stems from the use of the loop variables<br />

to be defined in Section 6.1.2.<br />

In the present section, we shall introduce the quantum versions of the connection<br />

and loop variables and discuss the Gauss constraints (4.122) and the<br />

diffeomorphism constraints (4.127). These constraints already give a picture of<br />

the way space might look like on the smallest scales. At least on a kinematical<br />

level (using the Gauss constraints only), a major result can be obtained:<br />

the spectrum of geometric operators representing area or volume in the classical<br />

limit turns out to be discrete (Section 6.2). This has a direct bearing on<br />

the interpretation of black-hole entropy (see Section 7.1). The more complicated<br />

implementation of the Hamiltonian constraint is relegated to Section 6.3. We<br />

treat here only pure <strong>gravity</strong>, but various results can be extended to the case of<br />

standard-model matter (Thiemann 2001).<br />

6.1.1 Connection representation<br />

The connection representation is characterized classically by the Poisson bracket<br />

(4.120) between the densitized tetrad Ej b(y) and the SU(2)-connection Ai a(x).<br />

These variables are then formally turned into operators obeying the commutation<br />

relation ]<br />

[Âi a (x), Êb j (y) =8πβiδj i δb aδ(x, y) . (6.1)<br />

In the functional Schrödinger representation, one can implement this relation<br />

formally through<br />

 i a (x)Ψ[A] =Ai a (x)Ψ[A] , (6.2)<br />

Êj b (y)Ψ[A] =8πβ δ<br />

i δA j Ψ[A] , (6.3)<br />

b<br />

(y)<br />

where the A in the argument of the wave functional is a shorthand for A i a (x).<br />

As in Chapter 5, the constraints are implemented as conditions on allowed wave<br />

functionals. The Gauss constraints (4.122) then becomes<br />

181

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