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Black Holes

Notes

Black Holes

One-line summary: Regions where gravity bends spacetime so severely that nothing escapes; observable only by their shadow and the brilliantly hot gas trapped around them.

The insight

A black hole forms when a dying star's core collapses into a "bottomless pit of gravity." Per michelle-thaller, we don't know if there's an interior — "all the equations blow up; time and space don't exist in there." What we observe is indirect: the shadow of the event horizon (imaged by the event-horizon-telescope), stars whipping around the galactic-center black hole, and the extremely bright accretion disk and jets. Every major galaxy hosts a central supermassive black hole; the Milky Way's is ~4 million solar masses, with the largest known reaching tens of billions.

The chain

How the giant central black holes formed is an open frontier: the early dense universe may have collapsed huge gas cores directly into black holes (not stars), which then accreted and merged into supermassive holes. Canonical: direct-collapse-to-supermassive-black-holes.

Evidence

Contradictions / tensions

"White holes" (a hypothetical other end of a black hole) had a following in the 1960s–70s but have "fallen out of favor" — the super-bright objects once attributed to them are now understood as hot accretion-disk gas. Whether a new universe forms inside a black hole (or whether our universe is itself inside one) is flagged explicitly as conjecture, not observation.

Open questions

  • Is there an interior to a black hole, and what governs it? (current physics gives up — see neutron-stars for the parallel)
  • what-is-time near an event horizon.

Related

Referenced by
brain — research vault