Does General Relativity Allow for Swimming in Space-Time?

In summary, the author thinks that the idea of moving around in curved space without violating conservation laws is far-fetched and unlikely.
  • #1
Jonathan Scott
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"Swimming" in space-time

On the main forums page, there is a link in the "Scientific American" section to an article http://www.scientificamerican.com/article.cfm?id=surprises-from-general-relativity".

I've had a look at the article and I don't even begin to believe it.

Even if you forgive the illustrative device of macroscopically-curved space, the idea that one could wriggle around in a way which escapes conservation laws seems extremely far-fetched. Even his simplified example of "swimming" on an ordinary sphere seems to be in obvious violation of conservation laws.

I checked the article date and it's not April 1.

Does anyone think this could REALLY be correct?

(I'd go so far as to say that if GR really did work like that, I'd count it as evidence of a problem in GR).
 
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  • #2
Jonathan Scott said:
Even if you forgive the illustrative device of macroscopically-curved space, the idea that one could wriggle around in a way which escapes conservation laws seems extremely far-fetched. Even his simplified example of "swimming" on an ordinary sphere seems to be in obvious violation of conservation laws.

Hi Jonathan! :smile:

I think the clue is in the example Guéron gives of swimming on a sphere (http://www.scientificamerican.com/article.cfm?id=surprises-from-general-relativity&page=2") …

I'll change it slightly …

Suppose you have two bodies, of masses m and 2m, stationary at O.

Stage 1: Let them push each other apart, a distance 3r. Since the c.o.m. will still be at O, that means the m mass is now twice as far from O as the 2m mass, and in the opposite direction.

Stage 2: Let the 2m mass split into two equal parts (each therefore of mass m, the same as the other mass), which push each other apart, perpendicular to the original direction, until the three masses form an equilateral triangle.

Stage 3: Join the three masses to C, the centre of the equilateral triangle, and let them pull each other in, obviously coming together at C.

In flat space, C is at a distance r, say, from each vertex of the equilateral triangle, and a distance r.sin30º, = r/2, from each side of the equilateral triangle, and so C and O are the same point, so the whole mass of 3m is back where it started.

But on the surface of a sphere, C is at a distance r from each vertex of the equilateral triangle, and a distance r.sinθ, which is slightly more than r/2, from each side of the equilateral triangle (where θ 60º and 90º are the angles of the obvious smaller triangle), and so C and O are not the same point, so the whole mass of 3m has moved slightly.

And the same applies in any curved space, whether positively or negatively curved …
Basically, in curved space, the "average position" of three bodies is not well-defined, since it depends on the order in which you do the averaging.

In other words, the c.o.m. of three bodies is not well-defined, so there is no conservation law relating to the c.o.m., and so there is no paradox in the c.o.m. moving. :smile:
 
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  • #3
The on-line version of the article does not seem to include references, but the version in the August 2009 edition of Scientific American does give references. The paper that started this is

http://www.sciencemag.org/cgi/content/abstract/sci;299/5614/1865?maxtoshow=&HITS=10&hits=10&RESULTFORMAT=&author1=wisdom&andorexacttitle=or&andorexacttitleabs=or&andorexactfulltext=or&searchid=1&FIRSTINDEX=0&sortspec=relevance&fdate=7/1/1880&tdate=7/31/2009&resourcetype=HWCIT,HWELTR,

and the papers by the author of the Scientific American article are

http://arxiv.org/abs/gr-qc/0510054

http://arxiv.org/abs/gr-qc/0612131.
 
  • #4


I read that but I'm still having difficulty in believing it.

I'm assuming his "swimming on a sphere" case is like literally being a 2D object on a frictionless sphere (with the usual 3D laws of physics) and trying to move around. That can in theory work, in that it's certainly possible to rearrange things. If for example you split a mass at the equator into two parts which are pushed apart until they land up at the poles, then you can pull them back together to any other point on the equator. This doesn't violate any conservation laws because this will apply some force perpendicularly to the surface of the sphere which will shift the sphere itself a tiny bit.

However, I don't see how the curvature of GR could be like applying a force in a perpendicular direction to space, and in any case I find it hard to believe that one could be in a frame of reference where space alone is curved without that being associated with major acceleration or non-zero mass density. I think I'd need some convincing on that too.

I'd agree that in a local bit of curved space in geometry (not GR) such oddities could perhaps be achieved, but in GR the masses affect the space as well as the space affecting the masses and conservation of momentum and energy still hold on a scale large enough to approximate flatness even if there are regions of significant curvature locally.

Still, you're welcome to try to convince me that the "swimming" effect can work in GR.
 
  • #5
Jonathan Scott said:
… This doesn't violate any conservation laws because this will apply some force perpendicularly to the surface of the sphere which will shift the sphere itself a tiny bit.

No, Guéron's and my examples treat the sphere as fixed: the masses start in the same position, and finish in the same position, but have moved relative to the sphere, but without violating conservation.
However, I don't see how the curvature of GR could be like applying a force in a perpendicular direction to space

And the force is not perpendicular to the sphere, or to space: it is along the surface of the sphere, or within space.
 
  • #6


Jonathan Scott said:
I read that but I'm still having difficulty in believing it.

I think he hasn't factored in the modification to the local geodesic caused by the mass of the weights on the end of his arms together with a modification caused by the acceleration and deceleration of these weights which will also modify the geodesic.

I think what will happen as he swims towards his rocket is that his small amount of movement, if any, towards the rocket will move the rocket an equal amount away from him.
 
  • #7
Nickelodeon said:
I think what will happen as he swims towards his rocket is that his small amount of movement, if any, towards the rocket will move the rocket an equal amount away from him.

You mean he can move both himself and the rocket in the same direction, and without even touching the rocket? :confused:
 
  • #8


tiny-tim said:
You mean he can move both himself and the rocket in the same direction, and without even touching the rocket? :confused:


Strange I know but yes. Taking an extreme example, if you have a satellite moving around the Earth in orbit and you give the Earth a nudge it will effect the motion of the satellite.

In this case, he slightly moves the Earth towards him which in turn moves the rocket
 
  • #9


Similar effects exist even in Newtonian gravity. I disagree with the author of that article that the relativistic versions are fundamentally different. They do allow for a wider array of phenomena, but I think it's a very similar mechanism.

In either case, there are no conservation laws violated. The point is that an extended object in an inhomogenous gravitational field can "push" or "pull" off of those inhomogeneities. In Newtonian gravity, these are the forces that couple to the quadrupole and higher moments of an extended mass. The same interpretations also arise in GR, although the relevant formalism is too complicated to be taught in most textbooks.
 
  • #10
Hi Stingray! :smile:
Stingray said:
Similar effects exist even in Newtonian gravity.

The point is that an extended object in an inhomogenous gravitational field can "push" or "pull" off of those inhomogeneities. In Newtonian gravity, these are the forces that couple to the quadrupole and higher moments of an extended mass. The same interpretations also arise in GR, although the relevant formalism is too complicated to be taught in most textbooks.

No … those inhomogeneities are the difference … see http://www.scientificamerican.com/article.cfm?id=surprises-from-general-relativity&page=3" of Guéron's article …
Some effects in Newtonian gravitation may seem similar to spacetime swimming at first glance. For instance, an astronaut orbiting Earth could alter his orbit by stretching tall and curling into a ball at different stages. But these Newtonian effects are distinct from spacetime swimming—they occur because the gravitational field varies from place to place. The astronaut must time his actions, like a person on a swing does to swing faster. He cannot change his Newtonian orbit by rapidly repeating very small motions, but he can swim through curved spacetime that way.

The Newtonian method works only because Earth's gravitational field is inhomogeneous, but Wisdom's method (in Guéron's article) works even in a completely homogeneous gravitational field.

And the Newtonian method uses the "springiness" of Earth's gravitational field, and must be timed to "harmonise" with it, but Wisdom's method can be timed quite randomly and still work. :smile:
 
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  • #11


But if you can move between two points when they happen to be at the same gravitational potential, then you should be able to move up an infinitesimal gravitational gradient using the same method, and thus up any gravitational potential using the same method.
 
  • #12


I disagree. In their papers, Wisdom and Gueron both consider motion in Schwarzschild fields. These are inhomogeneous. Furthermore, a "uniform gravitational field" is flat spacetime. I don't think it's controversial to say that there are no swimming effects in that case.

To generalize slightly, no curvature inhomogeneities implies either Minkowski or de Sitter spacetime. In both cases, there are a full set of 10 conservation laws associated with the background Killing fields. This implies that no amount of internal deformation can affect the center-of-mass motion (ignoring beamed radiation or anything like that). The only way out of this is if the body is so large that it fills almost the entire universe. This is the only case where I'd agree with Gueron that centers-of-mass are intrinsically hopeless to define.

It is possible to get motion through internal deformation in (cosmological) spacetimes that are homogeneous only in spatial directions. I actually wrote a paper about this. Intuitively, components of the fluid moving with respect to the cosmological rest frame no longer see spatially homogeneity. They can push and pull off of the "timelike curvature." This is essentially the Newtonian effect with allowances for Lorentz boosts.

I need to think more about the timing argument.
 

1. What is meant by "swimming in space-time"?

"Swimming in space-time" refers to the concept of moving through the four dimensions of space and time, similar to how a swimmer moves through water. It is a way to visualize the motion of objects and events in the universe.

2. How does swimming in space-time relate to Einstein's theory of relativity?

Einstein's theory of relativity explains that space and time are interconnected and can be warped by the presence of massive objects. Swimming in space-time takes this concept further by imagining the movement of objects through this warped space-time fabric.

3. Can objects actually swim in space-time?

No, objects cannot literally swim in space-time. This is simply a conceptual tool to help understand the complex nature of the universe and how objects move through it.

4. What are some practical applications of understanding swimming in space-time?

Understanding swimming in space-time can help with navigation and predicting the motion of objects in the universe. It also has implications for space travel and understanding the effects of gravity on objects.

5. How can we visualize swimming in space-time?

There are various visual representations of swimming in space-time, including 3D animations and mathematical models. Some people also use the analogy of a trampoline to explain how massive objects warp space-time.

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