arXiv · 1308.0687
Anisotropic Spinfoam Cosmology
Abstract
The dynamics of a homogeneous, anisotropic universe are investigated within the context of spinfoam cosmology. Transition amplitudes are calculated for a graph consisting of a single node and three links - the `Daisy graph' - probing the behaviour a classical Bianchi I spacetime. It is shown further how the use of such single node graphs gives rise to a simplification of states such that all orders in the spin expansion can be calculated, indicating that it is the vertex expansion that contains information about quantum dynamics.
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Julian Rennert, David Sloan. 2013-11-20. Anisotropic Spinfoam Cosmology. https://doi.org/10.1088/0264-9381%2F31%2F1%2F015017
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