12.07.2015 Views

Approaches to Quantum Gravity

Approaches to Quantum Gravity

Approaches to Quantum Gravity

SHOW MORE
SHOW LESS
  • No tags were found...

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

260 E. Livine(i) Either we work with functionals of the connection A. Then a basis of quantum states isprovided by spin networks for the Lorentz group. These are labelled by unitary representationsof sl(2, C), they diagonalize C 1 (sl) and C 2 (sl), but they do not diagonalizeC(su). Therefore they do not diagonalize the area opera<strong>to</strong>r.(ii) Or we work with functionals of both the connection A and the time normal field χ.This is possible when A and χ commute (see (14.15)). It is possible <strong>to</strong> introduceprojected spin networks, which project on given eigenvalues of C(su) and thereforediagonalize the area opera<strong>to</strong>r. We will discuss the details of these states later.In the following, we will work with the latter alternative. Then the irreducible unitaryrepresentations (of the principal series) of sl(2, C) are labelled by a couple ofnumbers (n ∈ N,ρ ≥ 0). The Casimir’s values are then:C 1 = n 2 − ρ 2 − 1, C 2 = 2nρ, C = j ( j + 1), with j ≥ n. (14.16)The restriction j ≥ n comes from the decomposition of the sl(2, C) representationson su(2) irreducible representations. Moreover this condition ensures that the areaeigenvalues are all real (and positive) for any value of (λ, μ). This is a nice consistencycheck. Note however that, since the formula involves the real parameter ρ,we lose the discreteness of the spectrum, which was a key result of LQG!Now, it seems that we do not have any preferred choice of connection, andtherefore no rigorous prediction on the area spectrum. This would be an extra ambiguitybesides the choice of the Immirzi parameter γ . Instead, we choose <strong>to</strong> imposefurther constraints on the connection A(λ, μ) and two criteria naturally appear.(i) We require that the connection behaves properly under space-time diffeomorphisms,generated by H a and H.(ii) We require that the connection be commutative, i.e that {A, A} D vanishes.Unfortunately, these two conditions are not compatible. As we will see in the nextsections, the first choice corresponds <strong>to</strong> the only unique choice of a covariant connectionand is the one used by the proposed Covariant LQG. Very interestingly,the area spectrum for this covariant connection does not depend on the Immirziparameter γ . While this resolves the Immirzi ambiguity, it is still complicated <strong>to</strong>quantize the theory due <strong>to</strong> the non-commutativity of the connection. On the otherhand, the second criteria leads <strong>to</strong> a unique commutative Lorentz extension of theAshtekar–Barbero connection. It allows us <strong>to</strong> recover the su(2) structure and areaspectrum and Immirzi ambiguity of the real formulation of LQG.This raises the issue of the space-time covariance of the standard formulation ofLQG based on the Ashtekar–Barbero connection. Although there is no doubt thatH a and H satisfy the same algebra as the genera<strong>to</strong>rs of the space-time diffeomorphisms,the action of H on the connection is not the usual one. This means thatthis connection is not a space-time 1-form and thus does not have a clear geometric

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!