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Oppenheimer and Snyder compute continued gravitational contraction

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J. Robert Oppenheimer and Hartland Snyder published a calculation of a spherically symmetric pressureless cloud collapsing under its own gravity, showing that it contracts indefinitely and that a distant observer sees the collapse freeze at the Schwarzschild radius while an observer riding the surface passes through in finite time. It is the first description of what would later be called a black hole. Its influence was limited for two decades, partly because the idealised assumptions invited dismissal and partly because the physics community was about to be redirected by the war.

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Assembled from 28 blocks · 1 evidence · 25 related

  1. Story
  2. J. Robert Oppenheimer and Hartland Snyder published a calculation of a spherically symmetric pressureless cloud collapsing under its own gravity, showing that it contracts indefinitely and that a distant observer sees the collapse freeze at the Schwarzschild radius while an observer riding the surface passes through in finite time. It is the first description of what would later be called a black hole. Its influence was limited for two decades, partly because the idealised assumptions invited dismissal and partly because the physics community was about to be redirected by the war.
  3. Knowledge
  4. The event horizon
  5. The singularity
  6. Time dilation near a horizon
  7. Oppenheimer and Snyder compute continued gravitational contraction
  8. Connections
  9. The singularity
  10. The event horizon
  11. Time dilation near a horizon
  12. Penrose proves that collapse to a singularity is generic
  13. Oppenheimer and Snyder compute continued gravitational contraction
  14. Penrose proves that collapse to a singularity is generic
  15. The Nobel Prize in Physics recognises black holes twice over
  16. The Kerr solution and black hole spin
  17. Schwarzschild radius
  18. Black hole entropy
  19. Schwarzschild solves the field equations for a point mass
  20. Oppenheimer and Snyder compute continued gravitational contraction
  21. Penrose proves that collapse to a singularity is generic
  22. The term "black hole" enters use
  23. GW150914 - two black holes merge and the signal reaches Earth
  24. Schwarzschild radius
  25. Oppenheimer and Snyder compute continued gravitational contraction
  26. S2 passes pericentre and its light is measurably redshifted
  27. Evidence
  28. The first relativistic description of indefinite gravitational collapse, including the divergence between the infalling and distant descriptions of the crossing. V55 VERIFICATION BASIS: not consulted in session; no research tool was available. Volume and page are from recall of a canonical citation and must be checked.
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