Abstract
We study an anisotropic simplicial minisuperspace model with a cosmological constant and a massive scalar field. After obtaining the classical solutions we then compute the semiclassical approximation of the no-boundary wavefunction of the Universe along a steepest-descent contour passing through classical Lorentzian solutions. The oscillatory behaviour of the resulting wavefunction is consistent with the prediction of classical Lorentzian spacetime for the late Universe.
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