Geodesics Around Black Holes: Do They Form Closed Loops?

In summary: But if you send the photon in at the right trajectory, it will enter an unstable orbit - unstable because any perturbation (e.g. the emission of a new photon) will cause the orbit to change and the photon to either spiral inward or escape the black hole.So, in summary, the photon can orbit a black hole, but only if it's precisely on the unstable orbit. Any perturbation will change its path and either cause it to escape or to fall into the singularity. In summary, we discussed the concept of light being unable to escape from black holes due to their immense gravity. A question was raised about the possibility of light traveling in closed loops around black holes, to which it was explained that this is not generally
  • #1
ObsessiveMathsFreak
406
8
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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  • #2
Originally posted by ObsessiveMathsFreak
But Since light has the same speed everywhere does that mean that the space/time geodesics in and around black holes are closed loops?

Not generally (although there is one location at which light can (unstably) orbit a black hole in a closed loop.) Why should the constancy of the local speed of light imply that light should travel in closed loops, around a black hole or anywhere else?
 
  • #3
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.
 
  • #4
well the light should just fall into the singularity, but then again i may be confused on the actual scenario.
 
  • #5
At a distance of

[tex]\frac{3 G M}{c^2}[/tex]

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

- Warren
 
  • #6
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?
 
  • #7
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
 
  • #8
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?
 
  • #9
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,"

[tex]r_s = \frac{2 GM}{c^2}[/tex]

- Warren
 
  • #10
oh, ok.
 
  • #11
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
 
  • #12
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.
 
  • #13
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.
 

What are geodesics around black holes?

Geodesics are the paths that objects follow in a curved spacetime, such as around a black hole. They are the shortest possible paths between two points and are determined by the geometry of the spacetime.

Do geodesics around black holes form closed loops?

Yes, geodesics around black holes can form closed loops. This occurs when an object is orbiting around the black hole and its trajectory is curved enough to return to its starting point. However, this is only possible for objects that are within a certain distance from the black hole, known as the photon sphere.

What determines the shape of geodesics around black holes?

The shape of geodesics around black holes is determined by the mass and spin of the black hole, as well as the velocity and trajectory of the object following the geodesic. The closer the object is to the black hole, the more extreme the curvature of the spacetime and the more dramatic the shape of the geodesic.

Can geodesics around black holes be predicted or calculated?

Yes, the geodesics around black holes can be predicted and calculated using the equations of general relativity. These equations take into account the properties of the black hole and the object following the geodesic, allowing for the prediction of the path that the object will follow.

How do geodesics around black holes affect the behavior of light?

Geodesics around black holes have a significant impact on the behavior of light. Light follows geodesics, so it can be bent and distorted by the strong gravitational pull of a black hole. This can result in phenomena such as gravitational lensing, where the light from distant objects is bent and distorted as it passes near a black hole.

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