About: Karl Schwarzschild's Pocket Watch   Sponge Permalink

An Entity of Type : dbkwik:resource/TGVw_48bfxR4O_s_eW_eZQ==, within Data Space : 134.155.108.49:8890 associated with source dataset(s)

This pocket-watch was originally owned by the Germain physicist, Karl Schwarzschild and was imbued with time altering abilities. He provided the first exact solution to the Einstein field equations of general relativity, for the limited case of a single spherical non-rotating mass, which he accomplished in 1915, the same year that Einstein first introduced general relativity. The Schwarzschild solution, which makes use of Schwarzschild coordinates and the Schwarzschild metric, leads to a derivation of the Schwarzschild radius, which is the size of the event horizon of a non-rotating black hole.

AttributesValues
rdf:type
rdfs:label
  • Karl Schwarzschild's Pocket Watch
rdfs:comment
  • This pocket-watch was originally owned by the Germain physicist, Karl Schwarzschild and was imbued with time altering abilities. He provided the first exact solution to the Einstein field equations of general relativity, for the limited case of a single spherical non-rotating mass, which he accomplished in 1915, the same year that Einstein first introduced general relativity. The Schwarzschild solution, which makes use of Schwarzschild coordinates and the Schwarzschild metric, leads to a derivation of the Schwarzschild radius, which is the size of the event horizon of a non-rotating black hole.
dcterms:subject
dbkwik:warehouse13...iPageUsesTemplate
Type
  • Pocket-watch
imagewidth
  • 150(xsd:integer)
Danger
  • Mild
Effects
  • Time related.
Source
  • Karl Schwarzschild
activate
  • Unknown
abstract
  • This pocket-watch was originally owned by the Germain physicist, Karl Schwarzschild and was imbued with time altering abilities. He provided the first exact solution to the Einstein field equations of general relativity, for the limited case of a single spherical non-rotating mass, which he accomplished in 1915, the same year that Einstein first introduced general relativity. The Schwarzschild solution, which makes use of Schwarzschild coordinates and the Schwarzschild metric, leads to a derivation of the Schwarzschild radius, which is the size of the event horizon of a non-rotating black hole.
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