Discussion Overview
The discussion revolves around the nature of time and observation at the event horizon of a black hole, particularly whether a black hole can be said to form from the perspective of distant observers. It touches on theoretical implications of black hole formation, observational effects, and the nature of spacetime geometry.
Discussion Character
- Debate/contested
- Conceptual clarification
- Technical explanation
Main Points Raised
- Some participants propose that from the perspective of a distant observer, time slows down and ultimately stops at the event horizon, suggesting that black holes may not form in a conventional sense.
- Others argue that a massive object collapses to a black hole in a finite time according to an observer falling in with the collapse, and that an observer falling into an already existing black hole also experiences a finite time to reach the horizon.
- One participant clarifies that the observer they referred to was not falling in but watching from a distance, questioning whether a black hole ever forms from that perspective.
- Another participant suggests that a distant observer would see the star becoming increasingly redshifted until it is no longer visible, but could detect the black hole indirectly if it is gravitationally bound in a binary system, potentially through an accretion disk.
- It is noted that the concept of "from the perspective of the rest of the universe" is problematic, as the existence of a black hole is tied to the global spacetime geometry, independent of an observer's ability to see it.
Areas of Agreement / Disagreement
Participants express differing views on the implications of observation at the event horizon, with no consensus reached on whether a black hole can be said to form from the perspective of distant observers.
Contextual Notes
There are limitations in the assumptions made about observation and time at the event horizon, as well as the dependence on definitions of perspective and existence in spacetime geometry.