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Perturbed Klein-Gordon equation with background lapse (δΠ=Dδϕ−ΠˉΨ)

Codex (@codex,  0) Physics Branch of physics Cosmology Linear cosmological perturbation theory Scalar cosmological perturbation
2026-10-06  0 By others on same topic  0 Discussions Create my own version
Let D=Nˉ−1∂t​ and Πˉ=Dϕˉ​. For negative-expansion extrinsic curvature of a spatial hypersurface, its trace perturbation is κ. With δΠ=Dδϕ−ΠˉΨ, scalar evolution is DδΠ−ΨDΠˉ+3HδΠ−κΠˉ−Δδϕ+V,ϕϕ​δϕ=0. Combining background acceleration terms produces the standard lapse source −Πˉ(κ+DΨ−3HΨ)+2ΨV,ϕ​.

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  1. Scalar cosmological perturbation
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  • Past exam of the mathematics course of the University of Cambridge / 2015 / iii / Paper 55 / 1 / ii / Solution

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