Holonomy-flux spinfoam amplitude
Nov, 2012Citations per year
Abstract: (arXiv)
We introduce a holomorphic representation for the Lorentzian EPRL spinfoam on arbitrary 2-complexes. The representation is obtained via the Ashtekar-Lewandowski-Marolf-Mour\~ao-Thiemann heat kernel coherent state transform. The new variables are classical holonomy-flux phase space variables of Hamiltonian loop quantum gravity prescribing the holonomies of the Ashtekar connection , and their conjugate gravitational fluxes. For small heat kernel `time' the spinfoam amplitude is peaked on classical space-time geometries, where at most countably many curvatures are allowed for non-zero Barbero-Immirzi parameter. We briefly comment on the possibility to use the alternative flipped classical limit.Note:
- 33 pages
- 04.60.Gw
- 04.60.Nc
- 04.60.Pp
- spin: foam
- space-time: classical
- quantum gravity: loop space
- heat kernel
- Immirzi parameter
- coherent state
- holomorphic
References(46)
Figures(0)
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