etotheipi
Okay, well I don't understand. To me it just looks like you wrote the time transformation. But it's quite possible I don't know enough. 
etotheipi said:Okay, well I don't understand. To me it just looks like you wrote the time transformation. But it's quite possible I don't know enough.![]()
What do you mean by "without test particle" vs. "with test particle"? The definition of a frame does not have anything to do with test particles.Sagittarius A-Star said:I think, your formulation in #233 "non-inertial reference frame" could be interpreted as:
A1) non-accelerated frame(with non-Einstein-synchronization) without test particle -> no inertial force
A2) non-accelerated frame (with non-Einstein-synchronization) with test particle -> no inertial force
B1) accelerated frame without test particle -> no inertial force
B2) accelerated frame with test particle -> inertial force.
PeterDonis said:What do you mean by "without test particle" vs. "with test particle"? The definition of a frame does not have anything to do with test particles.
Ah, I see. That concern was about the distinction between the metric and the geodesic equation; the latter is where "inertial forces" (which is really a misnomer) appear. But neither of those things are a frame, and defining a frame automatically gets you both an expression for the metric and an expression for the geodesic equation. There is no such thing as a "frame without test particle" where you only have the metric and no geodesic equation.Sagittarius A-Star said:I added this distinction only because of etotheipi's concern in posting #139.
To my understanding, the geodesic equation follows automatically from the metric, because you can derive the geodesic equation by applying the principle of maximum proper time (which is compatible to the action principle) to a free test particle.PeterDonis said:Ah, I see. That concern was about the distinction between the metric and the geodesic equation; the latter is where "inertial forces" (which is really a misnomer) appear.
Yes, it does. But the two are still conceptually distinct: the metric describes the geometry of spacetime, the geodesic equation describes the curves that freely moving objects (objects that feel no force) follow.Sagittarius A-Star said:To my understanding, the geodesic equation follows automatically from the metric
By the way, as an aside. Do you know of a particularly easy or convenient way to make sure that ##\lambda## is not just any affine parameter but is specifically the proper time (specifically for a timelike worldline). I know that I can take ##\lambda## and go back to the metric to convert it to proper time, but can I do anything to the Lagrangian or the Euler equations to make it happen automatically?vanhees71 said:The dot means derivative with respect to an arbitrary world-line parameter, λ, which is automatically an affine parameter, because H=L=const, because L doesn't depend on λ explicitly.
Any affine parameter along a timelike worldline is proper time. Converting from one affine parameter to another is just rescaling the unit of time and/or picking a new "zero point". There is no one particular one that is "the" proper time; they all are.Dale said:Do you know of a particularly easy or convenient way to make sure that ##\lambda## is not just any affine parameter but is specifically the proper time (specifically for a timelike worldline)
Sorry, I should have been clear. I want the one that is the unit scaling in units where c=1. I.e. so that the affine parameter has the same units as the units of space.PeterDonis said:Any affine parameter along a timelike worldline is proper time. Converting from one affine parameter to another is just rescaling the unit of time and/or picking a new "zero point". There is no one particular one that is "the" proper time; they all are.
Isn't this going to be true automatically? I'm having trouble imagining how you would get into a situation where it wasn't true.Dale said:Sorry, I should have been clear. I want the one that is the unit scaling in units where c=1. I.e. so that the affine parameter has the same units as the units of space.
Then of course you have to set ##H=-1/2##.Dale said:Sorry, I should have been clear. I want the one that is the unit scaling in units where c=1. I.e. so that the affine parameter has the same units as the units of space.
hutchphd said:Have you carefully worked it out in detail? Draw up the two scenarios: incident beam comes in normal to grating and produces both a +1 and -1 diffraction max. The angular location of each will be the same even if the +x speed differs from the -x speed. This will be true because the overall diagonal speed of the diffracted beams +/-1 will also differ. This is a generic result as @Dale says
Check
Of course that's true. But it is only formally the case. You can define the time-coordinate of your coordinate system in such a way, that the start time is formally equal to the arrival time. That's like if you drive for 1 hour and cross the border of a time zone. Then you can start at 10h00 and arrive at 10h00 of the other time zone.DAH said:That's an interesting video thanks.
In the video he say's that light from distant objects such as stars or galaxies could reach us instantaneously and we wouldn't know it. Surely that's not true, is it?
Strictly speaking, you can't push things to this limit, because in this limit, surfaces of constant "time" are not spacelike, they're null. But that means there is no valid notion of "spatial distance" in these coordinates, which means there is also no valid notion of "speed".Sagittarius A-Star said:You can define the time-coordinate of your coordinate system in such a way, that the start time is formally equal to the arrival time.
No. The two time zones are two different coordinate systems with different time coordinates. They are not two parts of a single coordinate system. If you want a single coordinate system with a single time coordinate for the entire Earth, you need to look at something like UTC.Sagittarius A-Star said:That's like if you drive for 1 hour and cross the border of a time zone. Then you can start at 10h00 and arrive at 10h00 of the other time zone.
"Spatial distance" is not changed by this coordinate system, because ##x' = x##. Only light speed is infinite in this direction. Sound speed for example is then still finite.PeterDonis said:Strictly speaking, you can't push things to this limit, because in this limit, surfaces of constant "time" are not spacelike, they're null. But that means there is no valid notion of "spatial distance" in these coordinates, which means there is also no valid notion of "speed".
Yes, but obviously we know that the light from distant objects takes a certain amount of time to reach us. I was reading a paper the other day (don't have a link) about how scientists observed multiple images of a type 1a supernova caused by gravitational lensing, and there was a time delay between each image. They actually predicted when one of the images would appear using GR and the one way speed of light as c, and their calculations were correct. If light from the SN was instantaneous then those multiple images would have appeared at the same time.Sagittarius A-Star said:Of course that's true. But it is only formally the case. You can define the time-coordinate of your coordinate system in such a way, that the start time is formally equal to the arrival time. That's like if you drive for 1 hour and cross the border of a time zone. Then you can start at 10h00 and arrive at 10h00 of the other time zone.
The coordinate system I linked is for SR, not GR.DAH said:Yes, but obviously we know that the light from distant objects takes a certain amount of time to reach us. I was reading a paper the other day (don't have a link) about how scientists observed multiple images of a type 1a supernova caused by gravitational lensing, and there was a time delay between each image. They actually predicted when one of the images would appear using GR and the one way speed of light as c, and their calculations were correct. If light from the SN was instantaneous then those multiple images would have appeared at the same time.
Yes, it is, because, as I said, the surfaces of constant time are null, not spacelike. In other words, the spatial metric changes because of the redefinition of the time coordinate, even though the spatial coordinates do not change.Sagittarius A-Star said:"Spatial distance" is not changed by this coordinate system, because ##x' = x##.
The derivation you cite in that previous post is not valid for the limit case where ##c## becomes infinite in one direction; the equation for ##c' / c## is undefined for ##\theta = 0## (divide by zero error). So, as I said, this limit is not valid and so are any claims made using it.Sagittarius A-Star said:Only light speed is infinite in this direction. Sound speed for example is then still finite.
PeterDonis said:The derivation you cite in that previous post is not valid for the limit case where ##c## becomes infinite in one direction; the equation for ##c' / c## is undefined for ##\theta = 0## (divide by zero error). So, as I said, this limit is not valid and so are any claims made using it.
Source:Mathpages said:Furthermore, this dependence is sufficient to ensure that the average speed of light over any closed loop path is precisely c (for any constant value of k in the range from −1 to +1).
No, the sums still have terms in them with zero in the denominator, so they're still not valid.Sagittarius A-Star said:At mathpages, they allow also the "instantaneously" case at segments for calculating the round-trip-speed of light (k= +/- 1). They add traverse times (partly equal to zero) and avoid so deviding by zero:
More precisely, they are null in whatever direction we choose as the "axis" of the anisotropy. For the coordinate transformation given in the mathpages article, this is the ##x## direction. The metric in the transformed chart is easily found to be (I use capital letters instead of primes for the transformed chart):PeterDonis said:for the case ##k = \pm 1##, surfaces of constant time are null, not spacelike.
With reference to this post, I take it as follows: take a system of N moving objects and starting from their proper time (measured by its own attached clock), proper acceleration and relative radar speed of all other N-1 objects (i.e. ##N(N-1)## total relative radar speeds) write down the resulting system of equations involving coordinate "labels" of an hypotetical inertial reference frame (i.e. assume as metric in those coordinates the standard diagonal SR metric in inertial coordinates). If that system of equations has or has not a solution is a physical result.Dale said:For your question, you take a system of moving objects, each with their own clock, radar, and accelerometers (6 degree of freedom type). You measure the object’s proper time, proper acceleration, and relative distance and speed (radar) to each of the other objects. Then you solve the resulting system of equations to determine if there exists an inertial frame that can describe the object’s motion. It may very well turn out that there is no solution to that system of equations. So the existence of such a solution is not a mere convention but a physical result.