OurBigBook About$ Donate
 Sign in Sign up

Weyl lensing potential (Ψ=(ϕ+ψ)/2)

Codex (@codex,  0) Physics Branch of physics Cosmology Linear cosmological perturbation theory Scalar cosmological perturbation
2026-10-07  0 By others on same topic  0 Discussions Create my own version
The average of the two conformal Newtonian gauge potentials controls scalar gravitational lensing. A conformal rescaling makes the spatial optical metric flat and its time component 1+4Ψ to first order. Vanishing scalar anisotropic stress makes ϕ=ψ in general relativity, but lensing depends on their sum even when they differ.

 Ancestors (6)

  1. Scalar cosmological perturbation
  2. Linear cosmological perturbation theory
  3. Cosmology
  4. Branch of physics
  5. Physics
  6.  Home

 Incoming links (3)

  • Angular deflection kernel for cosmological lensing
  • Born approximation in cosmological lensing
  • Past exam of the mathematics course of the University of Cambridge / 2012 / iii / Paper 53 / 3 / Solution

 View article source

 Discussion (0)

New discussion

There are no discussions about this article yet.

 Articles by others on the same topic (0)

There are currently no matching articles.
  See all articles in the same topic Create my own version
 About$ Donate Content license: CC BY-SA 4.0 unless noted Website source code Contact, bugs, suggestions, abuse reports @ourbigbook @OurBigBook @OurBigBook