Seeing the Unseen: Visualizing a Rotating Black Hole

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Discussion Overview

The discussion revolves around the visualization of black holes, specifically focusing on the shape of the event horizon and how it appears to observers from different positions. The scope includes theoretical aspects of black hole geometry and the effects of rotation on their appearance.

Discussion Character

  • Exploratory, Technical explanation, Conceptual clarification

Main Points Raised

  • One participant notes that non-rotating black holes are spherical, while rotating black holes are ellipsoidal.
  • Another participant inquires if the term "rotating black hole" refers specifically to a Kerr black hole.
  • A participant introduces the concept of a boosted black hole, suggesting that its event horizon could appear Lorentz contracted, resulting in a "pancaked" shape perpendicular to the direction of motion.
  • Further discussion includes the effects of gravitational lensing on the appearance of a rotating black hole, assuming no accretion disk obscures the view.

Areas of Agreement / Disagreement

Participants present multiple views regarding the shape of black holes and their visual representation, indicating that the discussion remains unresolved with competing perspectives on the topic.

Contextual Notes

There are assumptions regarding the definitions of black hole types and the conditions under which their shapes are described, which may not be fully explored in the discussion.

Kevin_Axion
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Of course one would suspect the title is quite odd because Black Holes don't allow anything with the velocity from 0 to c to escape once they pass the Event Horizon, excluding Bekenstein-Hawking Radiation but that is a concept that is irrelevant in this context. The trouble I'm having in visualizing a Black Hole is the apparent shape of the Event Horizon or the Black Hole itself, is it spherical as though it would appear similar from any observer dependent on their position around the Black Hole or is it a two dimensional circle then so from a front observer and opposite observer it would look "identical" but not to a side observer.

Thanks, Kevin
 
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A non-rotating black hole is spherical; rotating one is ellipsoidal.
 
Thanks, concise and the answer I was looking for. By a rotating black hole do you just mean a Kerr Black?
 
Last edited:
Also, for a boosted black hole, you can imagine the event horizon simply appearing lorentz contracted, so that it pancakes perpendicular to the line of motion.
 
Kevin_Axion said:
Thanks, concise and the answer I was looking for. By a rotating black hole do you just mean a Kerr Black?

Yep, it would be a Kerr black hole. In that scenario Nabeshin's point would be pretty impressive too. Beyond the structure of the hole itself, you'd also have the effects of gravitational lensing of starlight behind and around the event horizon, warped and "squashed" into the ellipse of its rotation. This assumes no accretion disk to obscure the view.
 

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