From Wikipedia, the free encyclopedia

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, Thomas Lewis, and Achilles Papapetrou. [1] [2] [3]

Details

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

where (tρϕz) are the cylindrical Weyl–Lewis–Papapetrou coordinates in 3 + 1 spacetime, and λ, Îœ, 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. (1917). "Zur Gravitationstheorie". Annalen der Physik. 54 (18): 117–145. Bibcode: 1917AnP...359..117W. doi: 10.1002/andp.19173591804.
  2. ^ Lewis, T. (1932). "Some special solutions of the equations of axially symmetric gravitational fields". Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character. 136 (829): 176–92. Bibcode: 1932RSPSA.136..176L. doi: 10.1098/rspa.1932.0073.
  3. ^ Papapetrou, A. (1948). "A static solution of the equations of the gravitatinal field for an arbitrary charge-distribution". Proceedings of the Royal Irish Academy. Section A: Mathematical and Physical Sciences. 52: 191–204. JSTOR  20488481.
  4. ^ Jiƙí Bičák; O. SemerĂĄk; Jiƙí PodolskĂœ; Martin Ćœofka (2002). Gravitation, Following the Prague Inspiration: A Volume in Celebration of the 60th Birthday of Jiƙí Bičák. World Scientific. p. 122. ISBN  981-238-093-0.

Further reading

Selected papers

Selected books


From Wikipedia, the free encyclopedia

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, Thomas Lewis, and Achilles Papapetrou. [1] [2] [3]

Details

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

where (tρϕz) are the cylindrical Weyl–Lewis–Papapetrou coordinates in 3 + 1 spacetime, and λ, Îœ, 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. (1917). "Zur Gravitationstheorie". Annalen der Physik. 54 (18): 117–145. Bibcode: 1917AnP...359..117W. doi: 10.1002/andp.19173591804.
  2. ^ Lewis, T. (1932). "Some special solutions of the equations of axially symmetric gravitational fields". Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character. 136 (829): 176–92. Bibcode: 1932RSPSA.136..176L. doi: 10.1098/rspa.1932.0073.
  3. ^ Papapetrou, A. (1948). "A static solution of the equations of the gravitatinal field for an arbitrary charge-distribution". Proceedings of the Royal Irish Academy. Section A: Mathematical and Physical Sciences. 52: 191–204. JSTOR  20488481.
  4. ^ Jiƙí Bičák; O. SemerĂĄk; Jiƙí PodolskĂœ; Martin Ćœofka (2002). Gravitation, Following the Prague Inspiration: A Volume in Celebration of the 60th Birthday of Jiƙí Bičák. World Scientific. p. 122. ISBN  981-238-093-0.

Further reading

Selected papers

Selected books



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