Weyl−Lewis−Papapetrou coordinates

In general relativity, the Weyl−Lewis−Papapetrou coordinates are a set of coordinates, used in the solutions to the vacuum region surrounding an axisymmetric distribution of mass–energy. They are named for Hermann Weyl, T. Lewis, and Achilles Papapetrou.[1][2][3]

Details

The square of the line element is of the form:[4]

where (t, ρ, ϕ, z) are the cylindrical Weyl−Lewis−Papapetrou coordinates in 3 + 1 spacetime, and λ, ν, ω, and B, are unknown functions of the spatial non-angular coordinates ρ and z only. Different authors define the functions of the coordinates differently.

See also

References

  1. Weyl, H., "Zur Gravitationstheorie," Ann. der Physik 54 (1917), 117–145.
  2. T. Lewis, "Some special solutions of the equations of axially symmetric gravitational fields," Roy. Soc., Proc. 136, 176–92 (May 2, 1932).
  3. A. Papapetrou, "A static solution of the equations of the gravitatinal field for an arbitrary charge-distribution," Proc. R. Irish Acad. A 52, 11 (1948).
  4. Jiří Bičák; O. Semerák; Jiří Podolský; Martin Žofka (2002). Gravitation, Following the Prague Inspiration: A Volume in Celebration of the 60th Birthday of Jiří Bičák. World Scientific. p. 122. ISBN 981-238-093-0.

Further reading

Selected papers

Selected books


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