Non-radial geodesics in Schwarzschild spacetime

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Discussion Overview

The discussion revolves around the behavior of non-radial timelike geodesics in Schwarzschild spacetime, particularly their interaction with the event horizon and singularity. Participants explore whether non-radial geodesics can cross the horizon and how angular momentum influences the proper time to reach the singularity.

Discussion Character

  • Exploratory
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • One participant questions whether non-radial timelike geodesics can cross the event horizon radially or if they can exist inside the horizon.
  • Another participant asserts that angular momentum prevents crossing the horizon radially and clarifies that "radially" refers to temporal direction inside the horizon.
  • A participant speculates that the proper time to reach the singularity may exceed a specific value depending on angular coordinates, asking for a formula to support this.
  • Another participant expresses an intuitive feeling that the proper time to reach the singularity would actually decrease with non-radial trajectories.
  • Some participants reference a previous thread and an exercise in MTW that discusses the longest proper time for a radial geodesic from the horizon to the singularity.
  • There is a debate about whether the MTW exercise restricts itself to radial motion, with some asserting it does not and others suggesting that the conclusion about maximizing geodesics being radial is not an assumption.
  • One participant proposes a heuristic argument regarding the proper time lapse of non-radial geodesics approaching null geodesics inside the event horizon.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between angular momentum and proper time in non-radial geodesics, and there is no consensus on whether the proper time increases or decreases based on trajectory. The discussion remains unresolved regarding the implications of non-radial geodesics inside the horizon.

Contextual Notes

Participants reference specific exercises and discussions from MTW, indicating a reliance on particular definitions and interpretations of geodesics, but the implications of these references are not universally accepted.

timmdeeg
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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.
 
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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.
 
PAllen said:
MTW exercise 31.4 does not restrict itself to radial motion.

Ah, ok. I'll check it out when I have a chance to dig out my copy of MTW.
 
PeterDonis said:
Ah, ok. I'll check it out when I have a chance to dig out my copy of MTW.
I thought all copies of MTW had collapsed to black holes by now ... if so you might have difficulties getting the information out ... :wink:
 
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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.
 
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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:
 
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  • #12
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?
 

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