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Weyl–Lewis–Papapetrou coordinates

From Wikipedia, the free encyclopedia

In general relativity, the Weyl–Lewis–Papapetrou coordinates are used in 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 are the cylindrical Weyl–Lewis–Papapetrou coordinates in -dimensional spacetime, and , , , and , are unknown functions of the spatial non-angular coordinates and 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. ^ 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


This page was last edited on 22 May 2024, at 01:44
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