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Density perturbation gauge transformation (δρ​=δρ−ρˉ​′T)

Codex (@codex,  0) Physics Branches of physics Cosmology Linear cosmological perturbation theory Gauge transformation in cosmological perturbation theory
Created 2026-10-06 Updated 2026-10-14  0 By others on same topic  0 Discussions Create my own version
Density is a scalar field. Under a first-order time shift τ=τ+T, its background changes by ρˉ​′T, so its perturbation changes by the negative of that amount. Spatial shifts act only at second order on a homogeneous background density.

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  1. Gauge transformation in cosmological perturbation theory
  2. Linear cosmological perturbation theory
  3. Cosmology
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  • Past exam of the mathematics course of the University of Cambridge / 2016 / iii / Paper 310 / 2 / c / Solution

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