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Inflation and Eternal Inflation

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arxiv astro-ph/0002156 v1 pith:4SNTTM72 submitted 2000-02-07 astro-ph

classification astro-ph
keywords inflationeternalmodelsalongalthoughambiguitiesarguedarguments
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The basic workings of inflationary models are summarized, along with the arguments that strongly suggest that our universe is the product of inflation. The mechanisms that lead to eternal inflation in both new and chaotic models are described. Although the infinity of pocket universes produced by eternal inflation are unobservable, it is argued that eternal inflation has real consequences in terms of the way that predictions are extracted from theoretical models. The ambiguities in defining probabilities in eternally inflating spacetimes are reviewed, with emphasis on the youngness paradox that results from a synchronous gauge regularization technique. Vilenkin's proposal for avoiding these problems is also discussed.

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Cited by 5 Pith papers

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

  1. False vacuum decay in a two-dimensional quantum spin system

    quant-ph 2026-07 unverdicted novelty 6.0 of 10

    Tree tensor network simulations of the 2D quantum Ising model match semi-classical predictions for false vacuum decay rate, effective interface tension, and critical bubble size.

  2. Electroweak First-Order Phase Transition Triggered by Non-Gaussian Fluctuations of a $\mathbb{Z}_2$-Symmetric Spectator Scalar

    hep-ph 2026-06 unverdicted novelty 6.0 of 10

    Non-Gaussian primordial fluctuations of a Z2-symmetric spectator scalar trigger a strong first-order electroweak phase transition, with the field serving as cold dark matter and generating a stochastic gravitational w...

  3. It\^{o}, Stratonovich, and zoom-in schemes in stochastic inflation

    astro-ph.CO 2024-11 accept novelty 6.0 of 10

    An alternating drift-and-kick 'zoom-in' scheme for stochastic inflation is equivalent to the Itô interpretation, and the Itô-Stratonovich difference vanishes in the full non-Markovian setup.

  4. Stochastic inflation with an extremely large number of $e$-folds

    hep-ph 2019-08 accept novelty 6.0 of 10

    A shallow local minimum added to a hilltop inflation potential can make the typical number of e-folds as large as 10^(10^10), enough for light scalars to reach Bunch-Davies equilibrium.

  5. Does Eternal Inflation Violate the Smeared Null Energy Condition?

    gr-qc 2026-06 unverdicted novelty 5.0 of 10

    In canonical single-field eternal inflation, stochastic upward fluctuations do not violate the SNEC within the semiclassical slow-roll regime due to parametrically bounded drift and a strong timescale hierarchy N_SNEC ≫ N_BR.

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