Non-radial geodesics in Schwarzschild spacetime

Join the discussion
Ask a follow-up here, or get your own question answered by working scientists, mathematicians and engineers — people, not an autocomplete.
Real named experts · corrections over time · the nuance an AI answer skips
11 replies · 2K views
timmdeeg
Gold Member
Messages
1,592
Reaction score
376
Consider a non-radial timelike geodesic outside the event horizon. Will it nevertheless cross the horizon radially or are non-radial geodesics also possible inside? I couldn't find any reference regarding a possible angle dependence in this respect.
 
Physics news on Phys.org
The angular momentum will prevent it from crossing the event horizon "radially". Inside the horizon you have to realize that "radially" as in "in the direction of the r coordinate" is not a spatial direction, but a temporal one. However, to answer your question, there will naturally be geodesics where the angular coordinats ##\theta## and ##\varphi## are not fixed.
 
Orodruin said:
The angular momentum will prevent it from crossing the event horizon "radially". Inside the horizon you have to realize that "radially" as in "in the direction of the r coordinate" is not a spatial direction, but a temporal one. However, to answer your question, there will naturally be geodesics where the angular coordinats ##\theta## and ##\varphi## are not fixed.
Thanks. Does it mean that the proper time to reach the singularity will exceed ##\tau={\pi}GM/c^3## (for the radial trajectory) depending on the angular coordinates? And if yes, is there an upper bound? It would be great if you could show the respective formula.
 
timmdeeg said:
Thanks. Does it mean that the proper time to reach the singularity will exceed ##\tau={\pi}GM/c^3## (for the radial trajectory) depending on the angular coordinates? And if yes, is there an upper bound? It would be great if you could show the respective formula.
To be honest, I have not thought much about it, but I would not think so. My intuitive feeling is that it would actually decrease the proper time to reach the singularity.
 
We had a recent thread touching on this. The longest possible proper time for any timelike worldline from horizon to singularity is attained by a radial geodesic corresponding to a drop from just outside the horizon. There is an exercise in MTW establishing this.
 
PAllen said:
The longest possible proper time for any timelike worldline from horizon to singularity is attained by a radial geodesic corresponding to a drop from just outside the horizon.

IIRC the discussion in that other thread, the paper linked to there, and the MTW exercise, only considered radial motion.
 
PeterDonis said:
IIRC the discussion in that other thread, the paper linked to there, and the MTW exercise, only considered radial motion.
No, MTW exercise 31.4 does not restrict itself to radial motion. That the maximizing geodesic is radial is something to conclude, not assume.
 
Orodruin said:
I thought all copies of MTW had collapsed to black holes by now ... if so you might have difficulties getting the information out ... :wink:
I thought MTW disproved the principle of equivalence - it falls faster than everything else.
 
  • Like
Likes   Reactions: Orodruin and PeterDonis
PAllen said:
I thought MTW disproved the principle of equivalence - it falls faster than everything else.

Hmm...maybe I'll dig up my copy of Wald as well as MTW and run the experiment. I'll need a vacuum chamber, though, to be sure I've eliminated possible confounding factors. :wink:
 
  • Like
Likes   Reactions: Orodruin
PAllen said:
No, MTW exercise 31.4 does not restrict itself to radial motion. That the maximizing geodesic is radial is something to conclude, not assume.
Thanks for mentioning that. In exercise 31.4 MTW note the hint: ... show that the geodesic of longest proper time lapse between ##r=2M## and ##r=0## is the radial geodesic, ...

Could one argue heuristically (having the light cone inside the event horizon in mind) that the proper time lapse of timelike non-radial geodesics decrease and approach ##0## as their trajectory approaches the null geodesics?