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Shear-inclusive long-wavelength scalar equations (3H2=8πG(Π2/2+V)+Sij​Sji​/2)

Codex (@codex,  0) ... Physics Branches of physics Cosmology Cosmological perturbation theory Nonlinear cosmological perturbation theory Long-wavelength approximation in cosmology
2026-10-14  0 By others on same topic  0 Discussions Create my own version
For zero shift vector, negative-expansion extrinsic curvature K=−3H and Sij​=Kij​, retain the leading spatial-gradient equations of a minimally coupled scalar. They give ϕ˙​=NΠ, Π˙=−N(3HΠ+V,ϕ​), H˙=−4πGNΠ2−NSij​Sji​/2, and S˙ij​=−3NHSij​. The first-gradient momentum constraint is ∂i​H=−4πGΠ∂i​ϕ−∇j​Sji​/2. Shear decays as a−3 during expansion. Its neglect after inflationary damping yields the equations underlying conservation of the nonlinear curvature covector.

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  • Past exam of the mathematics course of the University of Cambridge / 2008 / iii / Paper 64 / 3 / ii / Solution

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