Geodesics Around Black Holes: Do They Form Closed Loops?

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Discussion Overview

The discussion revolves around the nature of geodesics in and around black holes, particularly whether they can form closed loops. Participants explore concepts related to light behavior near black holes, including unstable orbits and the implications of general relativity.

Discussion Character

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

Main Points Raised

  • Some participants propose that light can orbit a black hole at a specific distance, known as the photon sphere, but express uncertainty about the stability of such orbits.
  • Others argue that light should ultimately fall into the singularity, raising questions about the conditions under which light can maintain an orbit.
  • A participant mentions that light can orbit at a distance of 1.5 times the event horizon radius, clarifying that the event horizon itself is not the point of stable orbit.
  • Another participant introduces the concept of closed null curves within the Kerr solution, suggesting these may be unphysical and represent mathematical artifacts rather than physical reality.
  • There is a discussion about the necessity of being outside the event horizon for light to orbit, as any photon within the event horizon cannot escape.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the behavior of light near black holes, particularly concerning the stability of orbits and the nature of closed geodesics. The discussion remains unresolved with no consensus reached.

Contextual Notes

Participants note limitations in understanding the exact conditions under which light can orbit a black hole, including the dependence on specific trajectories and distances from the black hole.

ObsessiveMathsFreak
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Light cannot escape from black holes, hence their name.

But Since light has the same speed everywhere does that mean that the space/time geodesics in and around black holes are closed loops?
 
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My understanding of black holes is that photons travellining in the right trajectory would be caught by the massive gravity of the black hole and orbit the black hole perpetually. This is known as a photon sphere, but I'm sure is just theory.
 
well the light should just fall into the singularity, but then again i may be confused on the actual scenario.
 
At a distance of

\frac{3 G M}{c^2}

light can orbit a black hole, though unstably, as Ambi said.

- Warren
 
unstably because if its distance changes at all, then the force of gravity changes with it and the orbit either becomes a fall or an escape?
 
Originally posted by franznietzsche
unstably because if its distance changes at all, then the force of gravity changes with it and the orbit either becomes a fall or an escape?
You got it. You'd have to have pretty good aim with your laser! :smile:

- Warren
 
Originally posted by chroot
You got it. You'd have to have pretty good aim with your laser! :smile:

- Warren

lol

edit: just realized something, the point at which it orbits exactly is in fact the event horizon is it not?
 
Originally posted by franznietzsche
edit: just realized something, the point at which it orbits exactly is in fact the event horizon is it not?
No, light can orbit at exactly 1.5 times the event horizon radius.

The event horizon exists at the "Schwarzschild radius,"

r_s = \frac{2 GM}{c^2}

- Warren
 
oh, ok.
 
  • #10
Closed null curves and two reference books

Hi, OMF,

ObsessiveMathsFreak said:
Since light has the same speed everywhere does that mean that the space/time geodesics in and around black holes are closed loops?

I'd add to what the others told you a possibly confusing and distracting comment: deep inside the Kerr solution, well hidden from outside viewers by the event horizon, lie closed null curves. These are generally thought to be unphysical and to represent a mathematical artifact of the symmetry of the Kerr vacuum (while the exterior field on the other hand is thought to be in some sense the "preferred state" of the exterior; according to gtr, an isolated black hole will radiate away any deviations from the Kerr geometry in the form of gravitational radiation).

These CNCs are truly closed curves; don't confuse them with the "unstable circular orbits" in the exterior region, which are spiral-shaped null geodesics.

Two excellent books which offer extensive discussions of geodesics in the Kerr solution are The Geometry of Kerr Holes, by Barrett O'Neill, and The Mathematical Theory of Black Holes by Subrahmanyan Chandrasekhar.

Chris Hillman
 
  • #11
edit: just realized something, the point at which it orbits exactly is in fact the event horizon is it not?
There's an easy heuristic reason, I think: if you inserted a mirror into the orbit, then the light could be deflected, and thus escape the black hole. So, the orbit has to be outside of the event horizon.
 
  • #12
franznietzsche said:
well the light should just fall into the singularity, but then again i may be confused on the actual scenario.

Sort of - it depends on whether your photon gets within the event horizon or not.

According to general relativity, massive objects cause space-time to warp in such a way that other objects (including photons) are pulled towards them, so a photon passing close to a black hole will always have its path deflected towards the hole. If you send a photon past with just the right trajectory at just the right distance from the hole, then its path should curve around the black hole and into an orbit (just like getting a satellite to orbit the earth, except that with a satellite we have the advantage of being able to use boosters to continuously fine-tune its position and keep it in orbit).

Inside the event horizon of a black hole the curvature is so strong that the escape velocity is higher than the speed of light and therefore any photon caught in there will spiral inwards towards the singularity.
 

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