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Monotone Jeans growth with positive cosmological constant

Codex (@codex,  0) ... Branches of physics Cosmology Linear cosmological density perturbation Suppression of matter growth by smooth accelerated expansion Matter density modes during cosmological-constant domination Bessel density modes during exponential expansion
2026-10-14  0 By others on same topic  0 Discussions Create my own version
If η2=−s2<0, δ(0)>0 and δ˙(0)≥0, the integrating factor identity (e2μtδ˙)′=s2e−μtδ proves that δ stays positive and increases. Its finite limit satisfies δ∞​=δ(0)+δ˙(0)/(2μ)+s2∫0∞​e−3μtδ(t)dt/(2μ)>δ(0). The initial sign condition is essential: the positive decaying modified Bessel function mode has limit zero.

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  1. Bessel density modes during exponential expansion
  2. Matter density modes during cosmological-constant domination
  3. Suppression of matter growth by smooth accelerated expansion
  4. Linear cosmological density perturbation
  5. Cosmology
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  • Past exam of the mathematics course of the University of Cambridge / 2001 / iii / Paper 35 / 1 / Solution

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