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The eternal fractal in the universe

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arxiv gr-qc/0111048 v2 pith:4PSV3TUH submitted 2001-11-15 gr-qc astro-ph

classification gr-qcastro-ph
keywords eternalfractalinflationconditiondimensiongeometrypointsstochastic
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Models of eternal inflation predict a stochastic self-similar geometry of the universe at very large scales and allow existence of points that never thermalize. I explore the fractal geometry of the resulting spacetime, using coordinate-independent quantities. The formalism of stochastic inflation can be used to obtain the fractal dimension of the set of eternally inflating points (the ``eternal fractal''). I also derive a nonlinear branching diffusion equation describing global properties of the eternal set and the probability to realize eternal inflation. I show gauge invariance of the condition for presence of eternal inflation. Finally, I consider the question of whether all thermalized regions merge into one connected domain. Fractal dimension of the eternal set provides a (weak) sufficient condition for merging.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Stochastic constant-roll inflation beyond the hilltop with the spectral method

    astro-ph.CO 2026-06 unverdicted novelty 6.0 of 10

    Spectral solution of the Fokker-Planck operator for hilltop constant-roll inflation shows rare crossing trajectories dominate the mean, so the median yields a coarse-grained ΔN distribution whose exponential tail flat...

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