Rindler coordinates are a coordinate system used in the context of special relativity to describe the hyperbolic acceleration of a uniformly accelerating...
66 KB (7,759 words) - 05:12, 22 June 2024
relativity where he is known for introducing the term "event horizon", Rindler coordinates, and (in collaboration with Roger Penrose) for the use of spinors...
14 KB (1,401 words) - 04:51, 11 July 2024
different in both coordinates. The Rindler spacetime has a horizon, and locally any non-extremal black hole horizon is Rindler. So the Rindler spacetime gives...
22 KB (2,938 words) - 19:48, 21 May 2024
accelerating observers (even linearly accelerating observers; see Rindler coordinates) can employ various distinct but operationally significant notions...
38 KB (6,356 words) - 10:24, 27 May 2024
metric, Isotropic coordinates, Lemaître–Tolman metric, Peres metric, Rindler coordinates, Weyl–Lewis–Papapetrou coordinates, Gödel metric. Some of...
15 KB (2,488 words) - 23:03, 29 December 2023
hyperbolic motion one can use Rindler coordinates, in the case of uniform circular motion one can use Born coordinates. Concerning the historical development...
59 KB (7,810 words) - 04:25, 8 January 2024
Wolfgang Rindler, the author of a standard introductory university-level textbook on relativity, hyperbolic coordinates of spacetime are called Rindler coordinates...
9 KB (1,255 words) - 01:05, 16 February 2023
147R. doi:10.1103/PhysRev.57.147. Biography portal Physics portal Rindler coordinates, for an account of the strange episode of Einstein and Rosen 1937...
14 KB (1,451 words) - 13:28, 22 May 2024
is a boundary beyond which events cannot affect an observer. Wolfgang Rindler coined the term in the 1950s. In 1784, John Michell proposed that gravity...
28 KB (3,545 words) - 16:46, 8 July 2024
acceleration. This Born rigid frame can be described by using Rindler coordinates (Kottler-Møller coordinates) c t = ( x ′ + c 2 α ) sinh α t ′ c , y = y ′ , x...
32 KB (4,442 words) - 17:35, 12 August 2023