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Why You'll Never See Anything Enter a Black Hole - Adam Brown

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Why You'll Never See Anything Enter a Black Hole - Adam Brown

Transcript

32 segments

0:00

So, suppose one learns all these

0:01

equations, but then finds himself in the

0:02

unfortunate position of falling into a

0:04

black hole. What would they see?

0:06

>> Great question. There's actually two

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different perspectives you could take.

0:09

One is the perspective of me watching

0:11

you falling into the black hole. The

0:12

other is the perspective of you falling

0:15

into the black hole. What I see, first

0:17

you'll go faster and faster and faster

0:18

towards the black hole [music] as you

0:20

fall down the gravitational potential.

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But then something strange will happen,

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which is you'll stop going faster and

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you'll start going slower. And the

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reason you're going slower is that as I

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watch you, you start to get

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gravitational time dilation as you fall

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down here. And I start to see you

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[music] running slow, your clock running

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slow. As I watch you, and presumably

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using light to watch you, that light

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gets more and more red shifted. The

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wavelength gets longer and longer. The

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longer the wavelength of light, the

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harder it is even to really see you. And

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eventually [music] I just stop seeing

0:45

you entirely. There's a final photon

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that I see that that you emit, and then

0:49

you just fade to [music] black. I never

0:51

see you cross the event horizon.

Interactive Summary

The transcript explains the relativistic effects observed when someone falls into a black hole, contrasting the experience of an outside observer with the perspective of the person falling in, focusing specifically on gravitational time dilation and redshift from the observer's viewpoint.

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