How do closed timelike curves avoid mass discontinuities in spacetime?

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Discussion Overview

The discussion revolves around the concept of closed timelike curves (CTCs) and how they relate to the conservation of mass in spacetime. Participants explore the implications of mass existing at multiple points in time along a CTC and the potential for mass discontinuities. The conversation touches on theoretical aspects, including the behavior of virtual particle-antiparticle pairs in relation to CTCs.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant questions how mass can exist at multiple moments along a CTC without creating a discontinuity, suggesting that the concept is not purely theoretical.
  • Another participant argues that the conservation law for the stress-energy tensor is satisfied in the context of CTCs, as mass "comes in" and "goes out" of a small region of spacetime, maintaining balance.
  • A different participant challenges the definitions of mass "coming in" or "going out," proposing that interpretations may vary depending on the perspective taken around the formation of particle pairs.
  • In response, a participant explains that the direction of a mass's 4-momentum vector indicates whether mass is entering or exiting a region of spacetime, linking this to the flow of time as measured by a clock carried by the mass.

Areas of Agreement / Disagreement

Participants express differing views on the interpretation of mass behavior in relation to CTCs, particularly regarding the definitions of mass entering or exiting a region of spacetime. The discussion remains unresolved, with multiple competing perspectives presented.

Contextual Notes

The discussion highlights the complexity of applying conservation laws in the context of CTCs and the potential ambiguity in defining mass interactions within small regions of spacetime.

georgir
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[Mentor's note: split from https://www.physicsforums.com/threads/gravity-instantaneous.801033/ ]

If masses can not just appear and disappear, how do solutions with closed timelike curves work? If you have some mass happily looping around such curve, from some other point of view you have some "moments" where that mass exists (twice, even, for both branches of the CTC) and then some later moments where it does not...
I'm having trouble imagining what could be the boundary between those and how it does not form a "discontinuity"...
I guess this is not entirely theoretical question too, as I've read that virtual particle-antiparticle pairs can actually be viewed as a single particle on a CTC.
 
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georgir said:
If you have some mass happily looping around such curve, from some other point of view you have some "moments" where that mass exists (twice, even, for both branches of the CTC) and then some later moments where it does not...

The conservation law for the stress-energy tensor doesn't work with "moments"; it doesn't depend on how you split up spacetime into space and time, and it doesn't say that the total amount of mass in a spacelike slice must be the same for every spacelike slice. It just says that, for any small region of spacetime, the amount of stress-energy "coming in" must equal the amount of stress-energy "going out". If you pick out any small region of spacetime that contains a short segment of the CTC followed by the mass, then the mass "comes in" to that small region and "goes out" of that small region, and it's the same amount of mass both times, so the conservation law is satisfied.
 
This is interesting... but what defines if the mass is "coming in" or is "going out" ?
If you take a small region of spacetime around the formation of the particle pair, you could say that it is just one particle, coming in and going out... or you could say that it is two particles going out, and require having enough energy coming into that region from elsewhere to compensate.
 
georgir said:
what defines if the mass is "coming in" or is "going out" ?

The mass is described by a 4-momentum vector; you just look at where the vector is pointing. On one side of a given small region of spacetime, the vector will be pointing in; on the other side, it will be pointing out. (The direction of the vector corresponds to the direction in which a clock carried by the mass is increasing its elapsed time.)
 

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