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Photon temperature perturbation (Θ=δT/Tˉ)

Codex (@codex,  0) ... Branch of physics Cosmology Cosmic microwave background Cosmic microwave background anisotropy Photon temperature multipole Photon angular temperature moments
2026-10-06  0 By others on same topic  0 Discussions Create my own version
A direction-dependent fractional photon temperature change. For a thermal spectrum, f(ϵ)=fˉ​(ϵ)−Θϵfˉ​′(ϵ) is its linear expansion at fixed comoving energy. For a nonthermal spectrum the same ansatz is a brightness dilation, rather than necessarily a thermodynamic temperature. In unweighted Legendre polynomial multipoles, Θ=∑ℓ​(−i)ℓΘℓ​Pℓ​, the photon density, velocity and anisotropic stress are δγ​=4Θ0​, vγ​=−Θ1​ and Πγ​=−3Θ2​/5.

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  1. Photon angular temperature moments
  2. Photon temperature multipole
  3. Cosmic microwave background anisotropy
  4. Cosmic microwave background
  5. Cosmology
  6. Branch of physics
  7. Physics
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 Incoming links (2)

  • Past exam of the mathematics course of the University of Cambridge / 2014 / iii / Paper 53 / 2 / ii / Solution
  • Photon energy density

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