6
$\begingroup$

From the perspective inside a black hole: Is information about everything outside a black hole - the rest of the cosmos - represented on the inside of the (event) horizon too? NB. I realize it is the notion of a so called stretched horizon that is being used about the 2d-like sheet that information is scrambled on, but I haven't heard about its view-from-the-inside-analogy, that naively being a horizon hovering just "below" the event horizon; therefore the simplified use of "event horizon" in the question. I also realize that it would be impossible to sample (all) this information as an inside job, which I would suppose could have some bearing on the answer to the question.

$\endgroup$
2
$\begingroup$

I cant speak in the case of full generality, but at least for Schwarzschild and Reissner-Nordstrom (electrically charged) non-rotating black holes, there exists a coordinate system called 'isotropic coordinates'; it turns out that in these coordinate systems the 'interior' and 'exterior' regions are actually isomorphic; this means that representing the solution in these coordinates gives rise to two identical yet causally disconnected regions of space-time. These two space-times share a common boundary, namely the event horizon.

As such, the two regions can be thought of representing the same physics and the answer to your question is then a definite 'yes': the information contained within the 'interior' section also amasses on the horizon.

$\endgroup$
0
$\begingroup$

The Holographic Principle in Black Hole Entropy implies a radical complementarity. From the perspective of an observer outside of the black hole what falls into the black hole is thermalized on the horizon and the information is spread out on the two dimensional area of the event horizon.

From the perspective of person falling through the event horizon Leonard Susskind argues that the person does not notice passing through the point of no return but experiences the universe in 3D inside the black hole. There is a complementarity, where from one perspective an observer sees the scrambled 2D information on the surface are of the event horizon, and from a second perspective inside the black hole there is no destructive thermalization and the observer is in 3 space.

From an external perspective there is a 2D reality, and from the interior perspective there is a 3D reality, and thus we have a type quantum complementarity of exclusive realities depending on the observer.

$\endgroup$
  • $\begingroup$ The question is more like the reverse of what you are answering. It has more to do with a hypothetical 2D representation INSIDE the event horizon of 3D objects located on the outside; is there any sort of symmetry that way. I realize it would be impossible to sample such a "screen" from the inside though, as your probe can't move in the direction of the event horizon/outwards. $\endgroup$ – Andersi2 Jan 6 '14 at 17:47
  • $\begingroup$ My understanding from Susskind's lecture is that inside it is 3D, from the outside the black hole we are looking at a hot 2D event horizon. I think there are some good lectures on line at Perimeter. By the concept of complementarity we only see one geometry or the other, never both simultaneously like wave particle complementarity. $\endgroup$ – sjlanterman Jan 8 '14 at 17:20

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service, privacy policy and cookie policy

Not the answer you're looking for? Browse other questions tagged or ask your own question.