The twistorial structure of loop-gravity transition amplitudes
Simone Speziale, Wolfgang M. Wieland

TL;DR
This paper introduces a twistorial approach to loop quantum gravity, clarifying classical geometries, simplifying constraints, and deriving transition amplitudes, thereby providing new insights into the theory's structure and dynamics.
Contribution
It develops a twistorial framework for loop quantum gravity, linking classical and quantum aspects, and derives transition amplitudes using twistor space methods.
Findings
Identifies dihedral angles as canonical pairs in twistor space
Constructs a spinorial version of simple projected spin networks
Derives EPRL transition amplitudes from a twistor space path integral
Abstract
The spin foam formalism provides transition amplitudes for loop quantum gravity. Important aspects of the dynamics are understood, but many open questions are pressing on. In this paper we address some of them using a twistorial description, which brings new light on both classical and quantum aspects of the theory. At the classical level, we clarify the covariant properties of the discrete geometries involved, and the role of the simplicity constraints in leading to SU(2) Ashtekar-Barbero variables. We identify areas and Lorentzian dihedral angles in twistor space, and show that they form a canonical pair. The primary simplicity constraints are solved by simple twistors, parametrized by SU(2) spinors and the dihedral angles. We construct an SU(2) holonomy and prove it to correspond to the (lattice version of the) Ashtekar-Barbero connection. We argue that the role of secondary…
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