LBoy said:
Thank you for your answer. Lots to think about :)
1. First comment about simultaneity of flashes. Original idea,the starting thought-experiment describes situation in and out of the train. For the observer in the train flashes at the front (B) and at the back (A) are not simultaneous so in his reference frame he will not see them both as simultaneous (contrary to what Hans says).
Hans: "So both observers see two flashes at the same time." They don't. The point where the two flashes meet is outside OT's head towards the back of the train.
I read the explanation as that there is an observer in the train who visually sees the flashes arrive at the same time, this observation in the train is effectively colocated in space and time with the ground observer seeing the flashes arrive at the same time. However, the train observer
models that the emission events are not simultaneous, while the ground observer models them as simultaneous. Neither of these statements about simultaneity represent anything that can be observed.
LBoy said:
2. Relativistic beaming. As far as I know this effect amount of energy "perceived" (measured) by the observer so in this case my use of word "intensity" is wrong, thanks for pointing that out, however I don't quite get how the observer will measure changes of size of the object. If there is an orthogonal rod along y-axis at length of 1 meter we still see 1 meter, not less nor more in the train. So no "bigger" nor "smaller" flashes unless we define big and small in terms not size but intensity/amount of energy measured in time. I have just realized that Hans might use this colloquialism, however in our case this double meaning is very misleading.
Relativistic beaming is the effect that if you are moving towards an EM source at near the speed of light, then, compared to a colocated observer at rest with respect to the source, you measure an intensity (power per sq. centimeter, for example) on the order of ## \gamma ^3 ## times greater. The causes of the are a combination of aberration reducing the angular diameter of the object, and the Lorentz transform of amplitute of a wave (which implies energy). In the classical treatment, there is no coupling between wave amplitude and wave frequency. It happens that they both transform in the same way, so the Doppler factor applies to both. But classically, these are independently derived facts, which happen to be coupled in a quantum theory. Thus, looking at photons, you might think there is just Doppler and aberration. However, classically, Doppler has nothing to do with energy - that is determined by amplitude transformation.
LBoy said:
3. Penrose-Teller rotation. In Minkowski space we have only three types of object that can be parametrized as simultaneous: a line in 2 dimensions, a plane in 3 d spacetime and finally a 3-d space when spacetime is 4 dimensional. All defined as orthogonal to the versor of time.
Now, however I see that Hans might use the term in 3-d space not in 4-d, and in this context "sphere of simultaneity" to an observer may mean a wavefront of e-m wave traveling from him in 3-d space, in vacuum this will indeed form a sphere in his rest frame and an ellipsoid in Minkowski space. I think there is a way of using this idea to explain events here, however in my opinion, this is a bit too much as it may complicate the picture in this quite difficult thought experiment. If I have time today I will re-read Hans explanations however I don't think 'spherical simultaneity" will add clarity to the picture, but of course I can be wrong.
Thank you again for your comments.
I don't understand what your are getting at here. One traditional analysis of the case of a moving sphere is to consider that light always travels at c in some chosen frame, but that no relativistic effects are present (relativity of simultaneity, length contraction, or time dilation). Then, you find that due to which light rays (simplifying to a geometric optics approximation) arrive at the same time, the sphere is elongated to an ellipse. However, then assuming that what was a sphere in its rest frame must be considered as a squashed in a frame in which it is moving (due to length contraction), then, redoing the arrival time analysis, you find an exact sphere is what will be observed. Member
@A.T., I believe, has links to nice visualizations of all this.
Penrose-Terrell rotation is a completely general phenomenon in special relativity which can be most elegantly approached in terms of aberration, because then you need not consider arrival times or simultaneity, and can immediately see that it applies to objects of any shape. The analysis, in brief, is as follows.
First, what is aberration? In SR, it is simply the way the angle of a light ray transforms in SR under a Lorentz transform. Conceptually, this has nothing in common with the Bradley derivation, which requires a corpuscular model of light as well as the false assumption that light speed depends on the motion of the source (even though the two
different formulas are currently indistinguishable due to observational precision limitations). The general rule is simple. Consider two colocated observers, A and B. Suppose B is moving in the +x direction relative to A. Suppose A observes a light ray (using geometric optics approximation, rather than plane waves) arriving at some ##\theta## relative to the x axis. Then B will observe this light ray arriving at an angle closer to the +x axis. The amount depends on speed, and in the limit of near c, even a ray A perceives as arriving from near the direction of the -x axis, B will observe as coming from near the +x axis.
Consider an arbitrary object moving relative relative to observer B as described above, but at rest relative to A. In the rest frame of A, you can analyze the image without considering simultaneity or arrival times. The situation is completely static. But then, in B rest frame, the set of rays arriving cannot be different. Their angles can be different, as can the frequency and energy. Thus, if you want to know the image B sees when the object looks orthogonal to x, per B, you compute the image per A when the object is back towards -x by the appropriate amount. For an object not too large in angular size, aberration then simply rotates this image towards +x, so it appears to come orthogonal to x per B. This means B sees an image of the object as if it is rotated towards B. In particular, even for a ruler with markings, the image looks just like the ruler was simply turned towards B, and this 'explains' the decrease in angular size (length contraction). Especially, if you imagine B able to image the object continuously despite high speed, it would look like the object, of whatever shape, is rotating as it moves, without any first order change in size or shape.