How can a black hole absorb matter?

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SUMMARY

The discussion centers on the mechanics of black holes and their ability to absorb matter, specifically addressing misconceptions surrounding time dilation and event horizons as described by the General Theory of Relativity. Participants clarify that while time appears to slow down for external observers, infalling objects experience finite time as they cross the event horizon. The conversation emphasizes the importance of using appropriate coordinate systems, such as Lemaitre coordinates, instead of Schwarzschild coordinates, which do not adequately describe dynamic black hole growth. Ultimately, the participants assert that black holes can indeed form and grow as they attract surrounding matter.

PREREQUISITES
  • General Theory of Relativity
  • Schwarzschild and Lemaitre coordinate systems
  • Concept of event horizons and null surfaces
  • Understanding of time dilation in curved spacetime
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  • Study the implications of the Schwarzschild solution on black hole dynamics
  • Explore the Lemaitre coordinates and their application in general relativity
  • Investigate the Oppenheimer-Snyder model for black hole formation
  • Learn about the concept of light cones and their relevance to black hole physics
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Astronomers, physicists, and students of general relativity seeking to deepen their understanding of black hole mechanics and the complexities of spacetime interactions.

  • #31
JimWhoKnew said:
I want the correcting arguments to be good and valid.
Another simple correcting argument is here:

PeterDonis said:
False. The proper phrasing in daily language is "the observer never sees light signals from the horizon formation". But it is a simple-minded logical error for that observer to conclude that because he didn't see something, it never happened.
 
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  • #32
Dale said:
Why? The existence of any finite ##\Delta \tau## is sufficient. @Ibix argument doesn’t rely on there being an upper bound.
Following @Ibix's clarification in #28, it seems that I misinterpreted his meaning.
 
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