Simulated shadows and disk images of the rotating LQG black bounce show parameter-dependent shadow contraction, Doppler asymmetry, and hat-like lensed image morphology.
Spinfoams: Foundations
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abstract
Spinfoams provide a framework for the dynamics of loop quantum gravity that is manifestly covariant under the full four-dimensional diffeomorphism symmetry group of general relativity. In this way they complete the ideal of three-dimensional diffeomorphism covariance that consistently motivates loop quantum gravity at every step. Specifically, spinfoam models aim to provide a projector onto, and a physical inner product on, the simultaneous kernel of all of the constraints of loop quantum gravity by means of a discretization of the gravitational path integral. In the limit of small Planck constant, they are closely related to the path integral for Regge calculus, while at the same time retaining all of the tools of a canonical quantum theory of gravity. They may also be understood as generalizations of well-understood state sum models for topological quantum field theories. In this chapter, we review all of these aspects of spinfoams, as well as review in detail the derivation of the currently most used spinfoam model, the EPRL model, calculational tools for it, and the various extensions of it in the literature. We additionally summarize some of the successes and open problems in the field.
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The shadow and accretion disk images of the rotation loop quantum black bounce
Simulated shadows and disk images of the rotating LQG black bounce show parameter-dependent shadow contraction, Doppler asymmetry, and hat-like lensed image morphology.