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Tensor normalization with unit-norm polarization tensors (δΦ(p)​=MPl​ψ(p)​)

Codex (@codex,  0) Physics Branches of physics Cosmology Linear cosmological perturbation theory Tensor cosmological perturbation
2026-10-14  0 By others on same topic  0 Discussions Create my own version
If the tensor metric perturbation is hij​=2Eij​ and the polarization tensors have contraction Mij(p)​M(q)∗ij=δpq​, the quadratic action for each Fourier amplitude is (MPl2​/2)∫a2(∣ψ(p)′​∣2−k2∣ψ(p)​∣2). Thus each helicity is normalized like a real massless scalar by the displayed rescaling. Its power per polarization is (Hk​/(2πMPl​))2. Factors of two in other tensor spectra depend on the definitions of the metric amplitude, the polarization norm and whether both helicities are summed.

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  • Past exam of the mathematics course of the University of Cambridge / 2010 / iii / Paper 53 / 4 / iii / Solution

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