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- hence the name of the chart. Isotropic charts are most often applied to static spherically symmetric spacetimes in metric theories of gravitation such...7 KB (1,179 words) - 00:26, 24 November 2022
- equations of general relativity. The metric describes a homogeneous, isotropic, expanding (or otherwise, contracting) universe that is path-connected...28 KB (4,171 words) - 16:09, 1 June 2024
- Tolman–Oppenheimer–Volkoff equation (metric and pressure equations of a static and spherically symmetric body of isotropic material) Planck length Luminet...37 KB (5,027 words) - 17:28, 23 May 2024
- invariant under rotations and taking the mirror image. A static spacetime is one in which all metric components are independent of the time coordinate t {\displaystyle...16 KB (3,672 words) - 00:52, 13 June 2024
- parameter H ( t ) = H 0 {\displaystyle H(t)=H_{0}} . In isotropic coordinates, the McVittie metric is given by d s 2 = − ( 1 − G M 2 c 2 a ( t ) r K 1 /...9 KB (1,687 words) - 13:24, 22 November 2023
- constrains the structure of a spherically symmetric body of isotropic material which is in static gravitational equilibrium, as modeled by general relativity...12 KB (2,080 words) - 05:37, 24 January 2024
- In Einstein's theory of general relativity, the interior Schwarzschild metric (also interior Schwarzschild solution or Schwarzschild fluid solution) is...12 KB (1,919 words) - 00:34, 17 October 2023
- The Gödel metric, also known as the Gödel solution or Gödel universe, is an exact solution, found in 1949 by Kurt Gödel, of the Einstein field equations...24 KB (3,800 words) - 16:35, 1 February 2024
- }}\right)\approx 0} and that the metric and its derivatives are approximately static and that the squares of deviations from the Minkowski metric are negligible. Applying...34 KB (5,096 words) - 09:51, 5 June 2024
- Unsolved problem in physics: Is the universe homogeneous and isotropic at large enough scales, as claimed by the cosmological principle and assumed by...32 KB (3,744 words) - 00:22, 9 June 2024
- charts have many applications in metric theories of gravitation such as general relativity. They are most often used in static spherically symmetric spacetimes...21 KB (4,089 words) - 06:20, 17 June 2024
- object, such as a star. In most textbooks one finds the metric tensor written in terms of a static polar spherical chart, as follows: d s 2 = − ( 1 − 2 m...27 KB (4,996 words) - 22:40, 6 December 2023
- equipped with suitable tensor fields which models a static round ball of a fluid with isotropic pressure. Such solutions are often used as idealized...8 KB (923 words) - 17:52, 29 January 2024
- Gullstrand–Painlevé coordinates (redirect from Gullstrand-Painlevé Metric)stuck to a full quadratic (static) form but instead, allowed a cross time-space product making the metric form no longer static but stationary and no longer...21 KB (3,655 words) - 17:32, 23 May 2024
- , to write the metric (the line element). Several coordinate charts are possible; these include: Schwarzschild coordinates Isotropic coordinates, in...10 KB (1,784 words) - 15:04, 26 October 2021
- constant spatial coordinate values to observers who perceive the universe as isotropic. Such observers are called "comoving" observers because they move along...18 KB (2,447 words) - 19:26, 7 June 2024
- Nordström's theory of gravitation (section The static spherically symmetric asymptotically flat vacuum solution)general theory of relativity. The static vacuum solutions in Nordström's theory are the Lorentzian manifolds with metrics of the form d s 2 = exp ( 2 ψ...38 KB (6,686 words) - 07:18, 5 April 2024
- Born coordinates (redirect from Langevin-Landau-Lifschitz metric)its immediate vicinity clocks are synchronized and light propagates isotropically in space. But the experience when the observers try to synchronize their...38 KB (6,356 words) - 10:24, 27 May 2024
- of static spherically symmetric perfect fluids. Static spacetime Static spherically symmetric perfect fluids Schwarzschild coordinates Isotropic coordinates...3 KB (365 words) - 14:08, 19 July 2022
- cosmological principle – that the universe is roughly homogeneous and isotropic in space though not necessarily in time, and the Copernican principle –...34 KB (4,543 words) - 01:49, 4 May 2024
- the transmitted power is 50 kilowatts. If the power is distributed isotropically over an area of 5.64 x 10^20 square meters (the area subtended by the
- that it formally became static, that is, included a term F ( t ) {\displaystyle F(t)} referring to the time parameter. The metric, giving the distance in
- is another important property of the isotropic model — the existence of a time singularity in the spacetime metric. In other words, the existence of such