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It's easy done. I still do it from time to time. To be clear, you correctly calculated ##\gamma=1/\sqrt{1-v^2/c^2}## and correctly calculated ##t-vx/c^2## but then incorrectly combined them as ##(t-vx/c^2)/\gamma## instead of ##\gamma(t-vx/c^2)##. As a general policy I'd recommend trying not to mix expressions containing gammas with expressions containing the square root form because if you do it's easy to substitute the wrong value as you did.mucker said:Ibix thanks Ibex, sorry for being dumb!![]()
You're always at t=0? So your watch always reads the same time? That's odd - I might stay in the same place but my watch always advances.mucker said:because the current frame of reference of an observer is always rooted in t=0, so therefore this event lies 2 seconds in his past
It is indeed the latter, but not for the reason you say. Negative values of ##t## aren’t necessarily in the past, they’re just before whatever moment we decided to call ##t=0##.mucker said:If we were to plot this event on a spacetime diagram from his perspective do we say t=0, x=2ls, or is it actually t=-2, x=2ls? (because the current frame of reference of an observer is always rooted in t=0, so therefore this event lies 2 seconds in his past). I was at first thinking the former but after thinking through it for a while I think you would record it as the latter...
He can record it as either, surely, as long as he records the reception event consistently. The latter might make the maths slightly simpler, but not much. Or am I missing a stated constraint somewhere?Nugatory said:It is indeed the latter, but not for the reason you say. Negative values of ##t## aren’t necessarily in the past, they’re just before whatever moment we decided to call ##t=0##.
What I was getting at is in respect to base observer/inertial frame (as in from what you are going perform your transformations on) - whenever I see spacetime diagrams the worldline of an object always intersects t0 (unless it's been transformed). Another way of looking at it is that say that we plot the wordline of an object at t1x3, t2x4, is that just the same as t0x2, t1x3 if we move the axis's up one second (or wait for one second to pass)? And isn't it essenitally the same thing? What I am saying is that I always see a wordline intercept t=0 so I assumed that is the just the covention we use - as in we can plot a worldline for two events like I just did, and they mean exactly the same thing, but by convention we defer to the t=0 one.Ibix said:You're always at t=0. That's odd - I might stay in the same place but my watch always advances.
I suppose in a rounabout way, that is what I was asking and actually what I concluded. What I was asking then is if you can plot it both ways, is the norm (convention/standard/whatever) to draw based on the wordline intersecting t0?Ibix said:He can record it as either, surely, as long as he records the reception event consistently. The latter might make the maths slightly simpler, but not much. Or am I missing a stated constraint somewhere?
The Lorentz transformations are embedded in the fact that each observer sees the same speed of light with respect to themselves. But, as shown in the diagrams, they disagree about whether the lightning flashes were simultaneous. They do agree that Mr. Green receives the light pulses together and Mr. Blue does not, but they draw different conclusions about what that means.mucker said:in mr greens frame he sees the bolts as expected (hit at the same time) and concludes the exact (and perfect) sequence of events that mr blue will conclude...without any Lorentz transformation.
You pick whatever origin you like. The origin needn't be at any specific time or place, but once you pick that origin you need to be consistent. So if you choose the origin as the event where the green man receives the light flash then receiving the light flash would be at ##(t_r,x_r)=(0,0)## and emitting the light flash would be at ##(t_e,x_e)=(-2,2)##. Of course, if you wanted you could have chosen a different origin, it doesn't matter as long as you are consistent.mucker said:from observer 1 (green man, stationary) a lighning bolt strikes 2ls away (he knows the distance for this example). He becomes aware of it at t2 obviously. If we were to plot this event on a spacetime diagram from his perspective do we say t=0, x=2ls, or is it actually t=-2, x=2ls? (because the current frame of reference of an observer is always rooted in t=0, so therefore this event lies 2 seconds in his past). I was at first thinking the former but after thinking through it for a while I think you would record it as the latter...
Yes, I confirmmucker said:Is this assessment correct and do the numbers look good?
There are too many issues here to address this early in the morning. All I shall say is to repeat my suggestion to read Morin's book.mucker said:I think I've finally figured it out and where I was going wrong. I'd be grateful if someone can verify that my logic is now sound.I had a feeling I [wrongly] concluded that due to the invariant speed of light, if you are moving at relativist speeds to two events of equal distance apart, you would still see them at the same time. Example - we only need one event here to show where my logic was flawed. Say for Ob A event happens 5ls away at t=0 and takes 5 secs to see it, he concludes it happened t=0. At that exact moment for Ob B, the event is still 5ls away (at least in Ob A frame, let’s not complicate this with length contraction and time dilation yet) and even though he is moving towards it, since light speed is invariant, it won't reach him any sooner. I've realized this logic is flawed - even though light always moves at the same speed in all reference frames, it actually has less distance to travel to reach ObB, so it DOES arrive sooner. I was failing to factor in that by the time the light reaches ObB it never traveled 5ls but was in fact less (if moving towards event). I know this may seem obvious to the rest of you or even dumb on my part but what was throwing me off was 2 facts I kept in mind when processing this:
So, I rationalised it as so:
- That light speed is invariant
- That in an inertial frame you are essentially stationary
Therefore, he concludes it happened at t=0 just like ObA.
- At t=0 ObB is 5ls away from event
- ObB is stationary in his frame over 5 seconds
- At t=5 he sees lightning at the end of the train and he already knows this distance is 5ls
Tbh I just think the train example is a terrible example, I came to the above conclusions because of that diagram. For example, the diagram looks like/implies the light travels 5ls from both ends to mr blue in his frame (for same reasons I say above), when in fact it travels 3ls (approx.) for R ray and 7ls for L ray (I am aware from blue’s perspective this not the case).
Using multiple sources may be part of the problem.mucker said:PeroK I am reading. I know you may think I am not, but I am. I am reading on average 4 hours a day, but sometimes it just raises more questions. I am reading from multiple sources too. I have read up on this one subject from about 4 different sources. The latest one I read, which brought me to above conclusions shows that the light has more distance to cover if you are moving relevant to where the events went off.
OK, so can you at least give me some idea of where you think I am not understanding a what a reference frame is?PeroK said:One of the fundamental issues before you can learn SR is to grasp the concept of a reference frame. And, especially being able to switch from one reference frame to another. A common error is to fix a certain reference frame as absolute in a sense and then only half-heartedly switch to another frame.
I've ordered the book!PeroK said:A reference frame (in this context a global inertial reference frame) is a system of coordinates that label each event in spacetime. It's not a snapshot.
An inertial observer has an associated "rest" frame. But, events may be labelled in that frame without explicit reference to any observer.
In many ways, it's better to imagine a reference frame as an infinite grid of equally spaced observers, all at rest relative to each other and all with pre synchronized clocks. Each observer records any local events, and the information from all observers is collated into the full set of observations.
In classical physics, two reference frames are related by the simple Galilean transformation, which preserves time intervals, lengths and simultaneity.
In SR, two reference frames are related by the Lorentz transformation, which preserves none of these this; but does preserve the length of spacetime intervals.
Read Morin!