Holonomy-flux spinfoam amplitude

Nov, 2012
33 pages
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201320162019202220245201
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 (h,X)TSU(2)(h,X)\simeq \mathcal T^*SU(2) of Hamiltonian loop quantum gravity prescribing the holonomies of the Ashtekar connection A=Γ+γKA=\Gamma + \gamma K, 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