ueit said:
Juao Magueijo’s article “Plan B for the cosmos” (Scientific American, Jan. 2001, p.47) reads:
Inflationary theory postulates that the early universe expanded so fast that the range of light was phenomenally large. Seemingly disjointed regions could thus have communicated with one another and reached a common temperature and density. When the inflationary expansion ended, these regions began to fall out of touch.
It does not take much thought to realize that the same thing could have been achieved if light simply had traveled faster in the early universe than it does today. Fast light could have stitched together a patchwork of otherwise disconnected regions. These regions could have homogenized themselves. As the speed of light slowed, those regions would have fallen out of contact
It is clear from the above quote that the early universe was in thermal equilibrium. That means that there was enough time for the EM field of each particle to reach all other particles (it only takes light one second to travel between two opposite points on a sphere with a diameter of 3 x 10^8 m but this time is hardly enough to bring such a sphere of gas at an almost perfect thermal equilibrium). A Laplacian demon “riding on a particle” could infer the position/momentum of every other particle in that early universe by looking at the field around him. This is still true today because of the extrapolation mechanism.
Your logic here is faulty--even if the observable universe had reached thermal equilibrium, that definitely doesn't mean that each particle's past light cone would become identical at some early time. This is easier to see if we consider a situation of a local region reaching equilibrium in SR. Suppose at some time t0 we fill a box many light-years long with an inhomogenous distribution of gas, and immediately seal the box. We pick a particular region which is small compared to the entire box--say, a region 1 light-second wide--and wait just long enough for this region to get very close to thermal equilibrium. The box is much larger than the region so this will not have been long enough for the whole thing to reach equilibrium, so perhaps there will be large-scale gradients in density/pressure/temperature etc., even if any given region 1 light-second wide is very close to homogenous.
So, does this mean that if we take two spacelike-separated events inside the region which happen after it has reached equilibrium, we can predict one by knowing the complete light cone of the other? Of course not--this scenario is based entirely on the flat spacetime of SR, so it's easy to see that for
any spacelike-separated events in SR, there must be events in the past light cone of one which lie outside the past light cone of the other, no matter how far back in time you go. In fact, as measured in the inertial frame where the events are simultaneous, the distance between the two events must be identical to the distance between the edges of the two past light cones at
all earlier times. Also, if we've left enough time for the 1 light-second region to reach equilibrium, this will probably be a lot longer than 1 second, meaning the size of each event's past light cone at t0 will be much larger than the 1 light-second region itself.
The situation is a little more complicated in GR due to curved spacetime distorting the light cones (look at some of the diagrams on
Ned Wright's Cosmology Tutorial, for example), but I'm confident you wouldn't see two light cones smoothly join up and encompass identical regions at earlier times--it seems to me this would imply at at the event of the joining-up, this would mean photons at the same position and moving in the same direction would have more than one possible geodesic path (leading either to the first event or the second event), which isn't supposed to be possible. In any case, your argument didn't depend specifically on any features of GR, it just suggested that if the universe had reached equilibrium this would mean that knowing the past light cone of one event in the region would allow a Laplacian demon to predict the outcome of another spacelike-separated event, but my SR example shows this doesn't make sense.
ueit said:
I also disagree that “the singularity doesn't seem to have a state that could allow you to extrapolate later events by knowing it”. We don’t have a theory to describe the big-bang so I don’t see why we should assume that it was a non-deterministic phenomena rather than a deterministic one. If QM is deterministic after all I don’t see where a stochastic big-bang could come from.
I wasn't saying anything about the big bang being stochastic, just about the initial singularity in GR being fairly "featurless", you can't extrapolate the later state of the universe from some sort of description of the singularity itself--this doesn't really mean GR is non-deterministic, you could just consider the singularity to not be a part of the spacetime manifold, but more like a point-sized "hole" in it. Of course GR's prediction of a "singularity" may be wrong, but in that case the past light cones of different events wouldn't converge on a single point of zero volume in the same way, so as long as we assume the new theory still has a light cone structure, we're back to my old argument about the past light cones of spacelike-separated events never becoming identical.
JesseM said:
I was asking if you were sure about your claim that in the situation where Mars was deflected by a passing body, the Earth would continue to feel a gravitational pull towards Mars' present position rather than its retarded position, throughout the process.
ueit said:
Yes, because this is a case where Newtonian theory applies well (small mass density). I’m not accustomed with GR formalism but I bet that the difference between the predictions of the two theories is very small.
Probably, but that doesn't imply that GR predicts that the Earth will be attracted to Mars' current position, since after all one can ignore Mars altogether in Newtonian gravity and still get a very good prediction of the movement of the Earth. If you really think it's plausible that GR predicts Earth can "extrapolate" the motions of Mars in this situation which obviously departs significantly from spherical/cylindrical symmetry, perhaps we should start a thread on the relativity forum to get confirmation from GR experts over there?
ueit said:
In Newtonian gravity the force is instantaneous. So, yes, in any system for which Newtonian gravity is a good approximation the objects are “pulled towards other object's present positions”.
You're talking as though the only reason Newtonian gravity could fail to be a good approximation is because of the retarded vs. current position issue! But there are all kinds of ways in which GR departs wildly from Newtonian gravity which have nothing to do with this issue, like the prediction that sufficiently massive objects can form black holes, or the prediction of gravitational time dilation. And the fact is that the orbit of a given planet can be approximated well by ignoring the other planets altogether (or only including Jupiter), so obviously the issue of the Earth being attracted to the current vs. retarded position of Mars is going to have little effect on our predictions.
ueit said:
The article you linked from
John Baez’s site claims that uniform accelerated motion is extrapolated by GR as well.
Well, the
wikipedia article says:
In general terms, gravitational waves are radiated by objects whose motion involves acceleration, provided that the motion is not perfectly spherically symmetric (like a spinning, expanding or contracting sphere) or cylindrically symmetric (like a spinning disk).
So either one is wrong or we're misunderstanding what "uniform acceleration" means...is it possible that Baez was only talking about uniform acceleration caused by gravity as opposed to other forces, and that gravity only causes uniform acceleration in an orbit situation which also has spherical/cylindrical symmetry? I don't know the answer, this might be another question to ask on the relativity forum...in any case, I'm pretty sure that the situation you envisioned where Mars is deflected from its orbit by a passing body would not qualify as either "uniform acceleration" or "spherically/cylindrically symmetric".
ueit said:
EM extrapolates uniform motion, GR uniform accelerated motion. I’m not a mathematician so I have no idea if a mechanism able to extrapolate a generic accelerated motion should necessarily be as complex or so difficult to simulate on a computer as you imply. You are, of course, free to express an opinion but at this point I don’t think you’ve put forward a compelling argument.
You're right that I don't have a rigorous argument, but I'm just using the following intuition--if you know the current position of an object moving at constant velocity, how much calculation would it take to predict its future position under the assumption it continued to move at this velocity? How much calculation would it take to predict the future position of an object which we assume is undergoing uniform acceleration? And given a system involving many components with constantly-changing accelerations due to constant interactions with each other, like water molecules in a jar or molecules in a brain, how much calculation would it take to predict the future position of one of these parts given knowledge of the system's state in the past. Obviously the amount of calculation needed in the third situation is many orders of magnitude greater than in the first two.
ueit said:
If what you are saying is true then we should expect Newtonian gravity to miserably fail when dealing with a non-uniform accelerated motion, like a planet in an elliptical orbit, right?
No. If our predictions don't "miserably fail" when we ignore Mars altogether, they aren't going to miserably fail if we predict the Earth is attracted to Mars' current position as opposed to where GR says it should be attracted to, which is not going to be very different anyway since a signal from Mars moving at the speed of light takes a maximum of 22 minutes to reach Earth according to
this page. Again, in the situations where GR and Newtonian gravity give very different predictions, this is not mainly because of the retarded vs. current position issue.