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- Q5617809 subject Q6509408.
- Q5617809 subject Q7163702.
- Q5617809 subject Q7806727.
- Q5617809 abstract "Gullstrand–Painlevé coordinates are a particular set of coordinates for the Schwarzschild metric – a solution to the Einstein field equations which describes a black hole. The time coordinate follows the proper time of a free-falling observer who starts from far away at zero velocity, and the spatial slices are flat. There is no coordinate singularity at the Schwarzschild radius (event horizon).The solution was proposed independently by Paul Painlevé in 1921 and Allvar Gullstrand in 1922. It was not recognized until 1933 in Lemaître's paper that these solutions were simply coordinate transformations of the usual Schwarzschild solution.".
- Q5617809 wikiPageExternalLink 0411060.
- Q5617809 wikiPageExternalLink hamilton1.
- Q5617809 wikiPageExternalLink index.html.
- Q5617809 wikiPageWikiLink Q1047034.
- Q5617809 wikiPageWikiLink Q14041.
- Q5617809 wikiPageWikiLink Q1478885.
- Q5617809 wikiPageWikiLink Q185243.
- Q5617809 wikiPageWikiLink Q192651.
- Q5617809 wikiPageWikiLink Q2111.
- Q5617809 wikiPageWikiLink Q211728.
- Q5617809 wikiPageWikiLink Q237284.
- Q5617809 wikiPageWikiLink Q271818.
- Q5617809 wikiPageWikiLink Q273711.
- Q5617809 wikiPageWikiLink Q2829907.
- Q5617809 wikiPageWikiLink Q315434.
- Q5617809 wikiPageWikiLink Q321.
- Q5617809 wikiPageWikiLink Q40392.
- Q5617809 wikiPageWikiLink Q4232155.
- Q5617809 wikiPageWikiLink Q5336608.
- Q5617809 wikiPageWikiLink Q601195.
- Q5617809 wikiPageWikiLink Q6086564.
- Q5617809 wikiPageWikiLink Q6509408.
- Q5617809 wikiPageWikiLink Q7163702.
- Q5617809 wikiPageWikiLink Q742969.
- Q5617809 wikiPageWikiLink Q76436.
- Q5617809 wikiPageWikiLink Q7806727.
- Q5617809 comment "Gullstrand–Painlevé coordinates are a particular set of coordinates for the Schwarzschild metric – a solution to the Einstein field equations which describes a black hole. The time coordinate follows the proper time of a free-falling observer who starts from far away at zero velocity, and the spatial slices are flat. There is no coordinate singularity at the Schwarzschild radius (event horizon).The solution was proposed independently by Paul Painlevé in 1921 and Allvar Gullstrand in 1922.".
- Q5617809 label "Gullstrand–Painlevé coordinates".