• In general relativity, the WeylLewisPapapetrou coordinates are used in solutions to the vacuum region surrounding an axisymmetric distribution of mass–energy...
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  • known for the Mathisson–Papapetrou–Dixon equations, the Majumdar–Papapetrou solution, and the WeylLewisPapapetrou coordinates of gravity theory. He worked...
    12 KB (1,324 words) - 08:31, 30 October 2024
  • transform Weyl transformation Weyl vector of a compact Lie group Weyl–Brauer matrices WeylLewisPapapetrou coordinates Weyl–Schouten theorem Weyl–von Neumann...
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  • metric, Isotropic coordinates, Lemaître–Tolman metric, Peres metric, Rindler coordinates, WeylLewisPapapetrou coordinates, Gödel metric. Some of...
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  • In physics, specifically general relativity, the Mathisson–Papapetrou–Dixon equations describe the motion of a massive spinning body moving in a gravitational...
    8 KB (1,266 words) - 13:56, 30 October 2024
  • corresponding to Newtonian gravitational potential) which appears the WeylPapapetrou chart for the Ernst family of all stationary axisymmetric vacuum solutions...
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  • Thumbnail for Friedmann–Lemaître–Robertson–Walker metric
    symmetric. Rewriting the metric in spherical coordinates reduces four coordinates to three coordinates. The radial coordinate is written as a product...
    26 KB (3,652 words) - 09:48, 14 May 2025
  • Schwarzschild coordinates Kruskal–Szekeres coordinates Eddington–Finkelstein coordinates Gullstrand–Painlevé coordinates Lemaître coordinates (Schwarzschild...
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  • {\displaystyle M\geq {\sqrt {Q^{2}+P^{2}}},} with equality for the Majumdar–Papapetrou extremal black hole solutions. An initial data set consists of a Riemannian...
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  • radiation, and a massless spinor exhibiting axial symmetry. In the Weyl-Lewis-Papapetrou spacetime, there exists a complete set of exact solutions for both...
    23 KB (3,411 words) - 19:15, 18 April 2025
  • Lemaître coordinates are a particular set of coordinates for the Schwarzschild metric—a spherically symmetric solution to the Einstein field equations...
    7 KB (1,195 words) - 19:51, 12 February 2024
  • Thumbnail for Black hole
    Eddington showed that the singularity disappeared after a change of coordinates. In 1933, Georges Lemaître realised that this meant the singularity at...
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  • within the event horizon.: 25–36  Alternatively, using a set of infalling coordinates in general relativity, one can conceptualize the event horizon as the...
    46 KB (5,968 words) - 02:33, 23 May 2025
  • Thumbnail for Wormhole
    1928, German mathematician, philosopher and theoretical physicist Hermann Weyl proposed a wormhole hypothesis of matter in connection with mass analysis...
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  • upon what coordinates or coordinate conditions are selected. Two forms are given below: Boyer–Lindquist coordinates, and Kerr–Schild coordinates. The gravitational...
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  • Thumbnail for Stress–energy tensor
    Tensor index notation and Einstein summation notation). If Cartesian coordinates in SI units are used, then the components of the position four-vector...
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  • of the propagation of radiation in curved spacetime. The Weyl scalars, derived from the Weyl tensor, are often used. In particular, it can be shown that...
    32 KB (6,548 words) - 19:00, 30 January 2025
  • 1921 by Hans Reissner, Hermann Weyl, Gunnar Nordström and George Barker Jeffery independently. In spherical coordinates ⁠ ( t , r , θ , φ ) {\displaystyle...
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  • account the cosmological constant Λ {\displaystyle \Lambda } . In those coordinates the local clocks and rulers are at constant r {\displaystyle {\rm {r}}}...
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  • longitudinal–longitudinal, transverse–longitudinal, and transverse–transverse by Hermann Weyl. However, the nature of Einstein's approximations led many (including Einstein...
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  • of concepts such as vectors, tensors, pseudotensors and curvilinear coordinates. For an introduction based on the example of particles following circular...
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  • universe Introduction to the mathematics of general relativity Normal coordinates Systolic geometry Riemann–Cartan geometry in Einstein–Cartan theory (motivation)...
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  • d y , d z {\displaystyle dx,dy,dz} are small increments in the three coordinates x , y , z {\displaystyle x,y,z} of the clock's position, − G M i r i...
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  • event can be labeled by four numbers: a time coordinate and three space coordinates; thus spacetime is a four-dimensional space. The mathematical term for...
    25 KB (3,525 words) - 06:44, 25 May 2025
  • Thumbnail for White hole
    from the event horizon. For an observer outside using Schwarzschild coordinates, infalling particles take an infinite time to reach the black hole horizon...
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  • Stockum dust WeylLewisPapapetrou Hartle–Thorne Scientists Einstein Lorentz Hilbert Poincaré Schwarzschild de Sitter Reissner Nordström Weyl Eddington Friedmann...
    19 KB (2,934 words) - 18:43, 20 December 2024
  • makes space locally Minkowskian (that is, in suitable locally inertial coordinates, the metric is Minkowskian, and its first partial derivatives and the...
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  • Thumbnail for Introduction to general relativity
    surface can be described by two coordinates: the geographic latitude and longitude. Unlike the Cartesian coordinates of the plane, coordinate differences...
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  • particle. The Christoffel symbols are functions of the four spacetime coordinates and so are independent of the velocity or acceleration or other characteristics...
    28 KB (6,157 words) - 20:01, 21 November 2024
  • space any point can be specified by n real numbers. These are called the coordinates of the point. An n-dimensional differentiable manifold is a generalisation...
    9 KB (1,174 words) - 23:45, 10 April 2025