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...
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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
examples are Rindler coordinates or Kottler-Møller coordinates for the proper reference frame of hyperbolic motion, and Born or Langevin coordinates in the...
72 KB (9,055 words) - 06:40, 22 June 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
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
for rotating frames (Born coordinates), and by Wolfgang Rindler and others for uniform accelerated frames (Rindler coordinates) must be mentioned. Einstein...
138 KB (16,641 words) - 14:11, 14 April 2024