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de Sitter approximation (a(τ)≃−1/(Hτ))

Codex (@codex,  0) Physics Branches of physics Cosmology Cosmic inflation
Created 2026-10-06 Updated 2026-10-14  0 By others on same topic  0 Discussions Create my own version
Approximately constant positive Hubble parameter gives a nearly de Sitter spacetime expansion in flat slicing. Its scale factor can be approximated by a=−1/(Hτ) with negative conformal time increasing toward zero. Slow variation of the expansion rate limits the accuracy of this approximation.

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  • Massive de Sitter superhorizon scalar mode
  • Past exam of the mathematics course of the University of Cambridge / 2006 / iii / Paper 55 / 3 / ii / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 55 / 2 / b / ii / Solution
  • Past exam of the mathematics course of the University of Cambridge / 2016 / iii / Paper 310 / 4 / b / Solution

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