pervect said:
While such a frame, if it could be defined, would be interesting, it would not qualify as an absolute frame. An absolute frame is generally understood to imply that no other object is used to construct it. In this case, you are using many objects to construct your frame. So it's just an interesting relative frame.
I'm sure there are all sorts of complications I'm not thinking of, but if the vector sums did remain within a sphere somewhere in the universe, the center of that sphere wouldn't move relative to any observer.
whatta said:
shouldn't the sum be zero. or else it would be like the universe is moving somewhere.
I was thinking that it would be sort of like a brownian plot of a particle. The universe seems clumpy to a certain extent (as evidenced by CMBR pictures) so the vector sums would wander around a bit. It may be smooth enough however that the wandering sums stay within a defined and fairly small sphere (in relation to the total universe).
If you could define the sphere, then the center of that sphere could be said to be stationary relative to every other point in the universe. Any apparent motion of that point across the sky could be interpreted as the observer's motion relative to this point rather than the other way around.
loop quantum gravity said:
vectors of what, of forces acting on them, of their displacements,of their velocities, of what exactly?
Displacements for given time.
HallsofIvy said:
What do you mean by "the vectors" (that's really loop quantum gravity's question). All relevant vectors: force, acceleration, velocity, momentum, are only defined relative to some frame of reference. Starting from a different frame of reference would give different vectors and so a different result for the "sum of all vectors".
I was starting with the premise that at any given time, the universe has a state that exists regardless of our ability to measure it.
For example: If astronomers were lucky enough to record the birth of a sun-like star, the exact instant when it's nuclear fires ignited, and if after performing spectral analysis, they determined that the star was 4 billion light years away, it would be reasonable to assume that the star still exists. The star would actually be 4 billion years old, not days or weeks.
So from this, we could say that the universe has a non-relativistic state. We can't measure that state, but we might be able to come up with a rough extrapolation by projecting known physical laws forward in time from the point of observation.
pervect said:
Some of the technical points regarding vectors in GR are rather,well, technical. I will give a source that points out that you can't add them together in GR the way you do in SR rather than talk about the details myself. See Baez's
http://math.ucr.edu/home/baez/einstein/node2.html"
which also talks a little bit about "relative" vs "absolute" velocities. The following quote is from that URL.
Thanks for the link
pervect said:
It's probably also important to note that standard cosmological models assume the universe is infinite (or very very large, and that we are not near the edge). Of course the part we can actually observe (the observable universe) is finite.
Interesting. I hadn't hread that.
HallsofIvy said:
What do you mean by "the vectors" (that's really loop quantum gravity's question). All relevant vectors: force, acceleration, velocity, momentum, are only defined relative to some frame of reference. Starting from a different frame of reference would give different vectors and so a different result for the "sum of all vectors".
After chewing on that for awhile...
If you define a set of points on a circle with a large radius from your frame (say, 5 billion light years). Select whatever particles are closest to these points to use as the origin. Sum all vectors from these points and due to the fact that some of these origin points are bound to be closer to the "edge" of the universe than others, over time, the sums from each point should display a definite bias.
Points closer to the "edge" of the universe would display a bias in the direction of the geometric center as the shortened vectors from the edge side would be overpowered by the longer vectors from the rest of the universe.
Comparing the bias for each of the origin points should indicate roughly where the geometric center of the universe is and where the edge is. If you could find the center then it could be used as "the mother of all reference frames" for all distance and time measurements.