back now with time to take a closer look
http://arxiv.org/abs/gr-qc/0603085
Exotic Statistics for Loops in 4d BF Theory
John C. Baez, Derek K. Wise, Alissa S. Crans
40 pages, many figures
"After a review of exotic statistics for point particles in 3d BF theory, and especially 3d quantum gravity, we show that loop-like defects in 4d BF theory obey exotic statistics governed by the
'loop braid group'. This group has a set of generators that switch two loops just as one would normally switch point particles, but also a set of generators that switch two loops by passing one through the other. The first set generates a copy of the symmetric group, while the second generates a copy of the braid group. Thanks to recent work of Xiao-Song Lin, we can give a presentation of the whole loop braid group, which turns out to be isomorphic to the 'braid permutation group' of Fenn, Rimanyi and Rourke. In the context 4d BF theory this group naturally acts on the moduli space of flat G-bundles on the complement of a collection of unlinked unknotted circles in R^3. When G is unimodular, this gives a unitary representation of the loop braid group. We also discuss 'quandle field theory', in which the gauge group G is replaced by a quandle."
exerpts from introduction, page 2 and following
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Exotic statistics also arise naturally in the context of 3d quantum gravity. As we ‘turn on gravity’, letting Newton’s gravitational constant kappa become nonzero, ordinary quantum field theory on 3d Minkowski spacetime deforms into a theory where the Poincaré group goes over to a quantum group called the kappa-Poincaré group. Moreover, if we begin with a field theory of bosons, their statistics become exotic as we turn on gravity. For a thorough treatment of these fascinating phenomena, see the papers by Freidel and collaborators [11, 12], the paper by Krasnov [20], and the many references therein.
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So, the exotic statistics reduce to ordinary bosonic statistics in the limit where Newton’s constant goes to zero. They also reduce to bosonic statistics in the limit where the particles are at rest relative to each other, since then p1 and p2 become proportional and their commutator vanishes.
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The corrections to the usual law for addition of energy-momenta are interesting in themselves. Like the exotic statistics, these corrections become negligible in the limit kappa ->0. Under the name of ‘doubly special relativity’, modified laws for adding energy-momentum have already been studied by many authors. The paper by Freidel, Kowalski-Glikman and Smolin [12] gives a good account of how these modifications arise in 3d quantum gravity; their paper also explains more of the history of this subject.
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It would be wonderful to generalize all the above results to 4d gravity, but for now all we can handle is a simpler theory: 4d BF theory. This may eventually be relevant to gravity, since one can describe general relativity in 4 dimensions either as the result of constraining 4d BF theory with a certain gauge group, or perturbing around 4d BF theory with some other gauge group. The first approach goes back to Plebanski [28], and it underlies a great deal of work on spin foam models of quantum gravity [1, 25, 27], especially the Barrett–Crane model. The second approach goes back to MacDowell and Mansouri [22], and has recently been explored by Freidel and Starodubtsev [13].
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kappa is just a convenient multiple of G, like 8 pi G
Here's an assortment of references, some of many.
[11] L. Freidel and D. Louapre, Ponzano-Regge model revisited I: gauge fixing, observables and interacting spinning particles, Class. Quant. Grav. 21 (2004), 5685-5726. Also available as hep-th/0401076.
L. Freidel and D. Louapre, Ponzano-Regge model revisited II: equivalence with Chern-Simons, available as gr-qc/0410141 L. Freidel and E. R. Livine, Ponzano-Regge model revisited III: Feynman diagrams and effective field theory, available as hep-th/0502106.
[12] L. Freidel, J. Kowalski-Glikman and L. Smolin, 2+1 gravity and doubly special relativity, Phys. Rev. D69 (2004), 044001. Also available as hep-th/0307085.
[13] L. Freidel and A. Starodubtsev, Quantum gravity in terms of topological observables, available as hep-th/0501191.
[20] K. Krasnov, Quantum gravity with matter via group field theory, available as hep-th/0505174.
[21] Xiao-Song Lin, The motion group of the unlink and its representations, preprint, 2005.
[22] S. W. MacDowell and F. Mansouri, Unified geometric theory of gravity and supergravity, Phys. Rev. Lett. 38 (1977), 739–742. Erratum, ibid. 38 (1977), 1376.
[25] D. Oriti, Spin Foam Models of Quantum Spacetime, Ph.D. thesis, University of Cambridge. Also available as gr-qc/0311066.
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random comments
Derek Wise is a student of Baez at UC Riverside. He gave a talk at the October Loops '05 conference.
there are some new (to me) symmetry groups, fascinating pictures, the article draws quite a bit on unpublished "loop braid group" work by XiaoSong Lin, could be a help to Freidel in extending his 3D results (gravity and matter) to 4D.
I suspect paper will be important in physics, but can't tell for sure: hope other people look at it.
It is amazingly understandable. For the first time I get some inkling of why DSR happens.
I am up to page 6. It explains where the different classes of particles come from in 3D physics. a little "standard model" for a lowerdimension world.