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Steady-State Eternal Inflation

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arxiv astro-ph/0111191 v2 pith:QXS5ZBG5 submitted 2001-11-09 astro-ph gr-qchep-th

classification astro-phgr-qchep-th
keywords eternallyinflationsteady-stateconstructionforminitialtheoremstime
verification ladder T0 review T1 audit T2 compute T3 formal
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Since the advent of inflation, several theorems have been proven suggesting that although inflation can (and generically does) continue eternally into the future, it cannot be extended eternally into the past to create a ``steady-state'' model with no initial time. Here we provide a construction that circumvents these theorems and allows a self-consistent, geodesically complete, and physically sensible steady-state eternally inflating universe, based on the flat slicing of de Sitter space. This construction could be used as the background space-time for creation events that form big-bang-like regions, and hence could form the basis for a cosmology that is compatible with observations and yet which avoids an initial singularity or beginning of time.

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Cited by 1 Pith paper

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

  1. The BGV Theorem and the Null Convergence Condition

    gr-qc 2026-07 accept novelty 6.0 of 10

    NCC plus ³R≤0 imply BGV for shear-free geodesic orthogonal foliations, but shear and non-geodesic threading make the BGV expansion directional and can evade that guarantee.

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