Falling Feet First into a Black Hole

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Discussion Overview

The discussion revolves around the visual experience of a person falling feet first into a Schwarzschild black hole, particularly focusing on whether they can see their feet as they cross the event horizon. The scope includes theoretical considerations of general relativity and the implications of tidal forces on perception during this extreme scenario.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • One participant questions whether a person falling feet first can always see their feet, especially after crossing the event horizon, assuming no tidal forces act on them.
  • Another participant references a webpage suggesting that a person would see their feet pass through the event horizon, arguing that this aligns with the equivalence principle and local time considerations.
  • A participant mentions using a spacetime diagram to explain their reasoning, noting that light emitted from the feet moves outward but does not approach the singularity as quickly as the head does.
  • Further clarification is sought regarding the relationship between the feet and the photons emitted from them, particularly after crossing the horizon, suggesting that the observer would see light emitted before crossing the horizon.
  • One participant highlights the availability of additional general relativity resources for further exploration of the topic.

Areas of Agreement / Disagreement

Participants express varying interpretations regarding the visibility of the feet after crossing the event horizon, with some supporting the idea that light emitted before crossing the horizon allows for continued visibility, while others raise questions about the implications of light cone behavior. No consensus is reached on the matter.

Contextual Notes

The discussion involves assumptions about the effects of tidal forces and the nature of light emission in the context of general relativity, which may not be fully resolved within the conversation.

Allday
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this was a kind of interesting HW problem i was working on. handed in the solution already, but don't know if it was right. ill run it by the forum and see what the members think.

what would a person see if they where falling feet first radially into a Swarzschild black hole. The person is looking at their feet the whole time. Are they always able to see their feet? (especially when their feet are inside the event horizon and their head is not). Once they cross the horizon are they still able to see their feet? Assume of course that they are not stretched apart by the tidal forces.
 
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This page says that you could see your feet (which is what I'd have guessed, since otherwise it seems like the equivalence principle would be violated):
One common question is whether a man falling (feet first) through an even horizon of a black hole would see his feet pass through the event horizon below him. As should be apparent from the schematics above, this kind of question is based on a misunderstanding. Everything that falls into a black hole falls in at the same local time, although spatially separated, just as everything in your city is going to enter tomorrow at the same time. We generally have no trouble seeing our feet as we pass through midnight tonight, although it is difficult one minute before midnight trying to look ahead and see your feet one minute after midnight. Of course, for a small black hole you will have to contend with tidal forces that may induce more spatial separation between your head and feet than you'd like, but for a sufficiently large black hole you should be able to maintain reasonable point-to-point co-moving distances between the various parts of your body as you cross the horizon.
If you want more of an explanation though, you'll have ask one of the GR experts on this board...
 
yeah that was my conclusion eventually, thanks for the link. i answered it by referencing the space time diagram with the light cones tilting in as you approach the event horizon. my reasoning was that even thought the light emitted from the feet in the radially "outward" direction is still approaching the singularity they don't do so as fast as the persons head.

gabe
 
Allday said:
yeah that was my conclusion eventually, thanks for the link. i answered it by referencing the space time diagram with the light cones tilting in as you approach the event horizon. my reasoning was that even thought the light emitted from the feet in the radially "outward" direction is still approaching the singularity they don't do so as fast as the persons head.
gabe
Yeah, I think the tilted light cones would be the key to understanding this, that web page also emphasized them in its explanation. But what's the "they" that you're saying doesn't approach the singularity as fast as the head--the feet, or the photons? I figure once your feet cross the horizon but your eyes haven't, you can still see your feet, but you're seeing light that was emitted from your feet before they crossed the horizon. And is it also true that when you see your feet after you've crossed the horizon, you're always seeing light that was emitted from your feet when they were at a greater distance from the singularity than your eyes are currently? From the tilted light-cone diagrams, I think it must be, since the radial dimension basically becomes your time dimension once you've crossed the horizon.
 
I must point out that there are very many interesting GR articles on that site as may be seen by http://www.mathpages.com/rr/rrtoc.htm" .
:smile:
 
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