2008
DOI: 10.1088/0264-9381/25/19/195024
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A Immirzi-like parameter for 3D quantum gravity

Abstract: We study an Immirzi-like ambiguity in three-dimensional quantum gravity. It shares some features with the Immirzi parameter of four-dimensional loop quantum gravity: it does not affect the equations of motion, but modifies the Poisson brackets and the constraint algebra at the canonical level. We focus on the length operator and show how to define it through non-commuting fluxes. We compute its spectrum and show the effect of this Immirzi-like ambiguity. Finally, we extend these considerations to 4d gravity an… Show more

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Cited by 38 publications
(108 citation statements)
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“…It is important to comment that our results have not been reported in the literature, and as a special case those results reported in [4,5] are reproduced. In addition, we would also remark that for BL theory we shall construct the Dirac brackets by eliminating the second class constraints and there will remain first class ones.…”
Section: Introductionsupporting
confidence: 63%
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“…It is important to comment that our results have not been reported in the literature, and as a special case those results reported in [4,5] are reproduced. In addition, we would also remark that for BL theory we shall construct the Dirac brackets by eliminating the second class constraints and there will remain first class ones.…”
Section: Introductionsupporting
confidence: 63%
“…However, in this work the structure of the constraints is not complete, thus, in order to compare the FJ method with the Dirac one it is mandatory to perform the Dirac analysis on the full phase space by following all Dirac steps. It is well known that three-dimensional gravity with a cosmological constant can be written as a Chern-Simons theory [1][2][3][4][5]. In fact, if the principal gauge bundle G over M is given by G = SU(2) for 3d Euclidean gravity, then we can enlarge the group G toG, whereG could be SO(4), ISO(3) or SO(3, 1), depending on the sign of the cosmological constant , it being positive, zero or negative respectively.…”
Section: Hamiltonian Dynamics For Three-dimensional Bl Gravitymentioning
confidence: 99%
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“…This defines the discrete BF action. Then, we have simplicity constraints at the level of each tetrahedron of the simplicial complex [22] (see also [29]). These constraints impose the restriction on the classical discrete Lie algebra B variables constraining the set of B f variables to be determined by a discrete tetrad field [28] and thus giving gravity from BF theory.…”
Section: C(b F ⊂E ) E I F Tr(b F H F (G E∈∂f ))mentioning
confidence: 99%