Special Relativity Question (Lorentz)

In summary: one is to use v = d/time ==> time = d/v and t' = \frac{1} {sqrt{1-\frac{v^2} {c^2}}} ...but that's not what is written here.
  • #1
RJLiberator
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Homework Statement


Synchronized clocks A and B are at rest in our frame of reference a distance 2 light minutes apart. Clock C passes A at a speed of c*4/5 bound for B, when both A and C read t =0 in our frame.

a) What time does C read when it reaches B?

b) How far apart are A and B in C's frame?

c) In C's frame, when A passes C, what time does B read?

Homework Equations



Lorentz equations

[tex] x' = x\sqrt{1-\frac{v^2} {c^2}} [/tex]
[tex] t' = t\sqrt{1-\frac{v^2} {c^2}} [/tex]

The Attempt at a Solution

a) I don't believe we have to use lorentz equations for this.
[tex] t = \frac{distance} {speed} = \frac{2c*mins} {0.8*c} = \frac{5} {2} mins [/tex]

b) This is where we use Lorentz contraction so

[tex] x^c = 2c*mins\sqrt{1-\frac{16}{25}} = 1.2c*mins[/tex]

c) This is the tougher one for me.

So, in C's frame, B is coming towards us at 4*c/5. We are at t=0.

Does time B read 1.2 minutes?

Thanks for your time / looking over my work.
 
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  • #2
Yes Lorentz is needed for (a). The question is what does the moving clock of C read, not what do clocks A and B read. Doing a calculation that divides the distance by the speed - both of which are given in the units of the frame A and B - will tell us what clocks A and B read, not what C reads. Also the arithmetic is incorrect: ##2\div 0.8## is not equal to ##4/5##.

First do a correct calculation of the elapsed time on clock A. Then use Lorentz to convert that to an elapsed time on clock C.
 
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  • #3
Whoops! I fixed the arithmetic error.

Let me analyze more deeply what we have:

In "our" frame of reference:
A, B are at rest
velocity of clock c = (4/5)c
d = 2 light minutes

We need to find t in C's frame of reference as it reaches B
so t in c we denote t' = t*sqrt(1-16/25)

The problem is in finding what t is equal to?
If I say x' = 2 light minutes (1-16/25) = 1.2 c minutes as I determined in b, then

x' = 1.2 c*minutes

Now I could use v = d/time ==> time = d/v

[tex] t' = \frac {d} {v} = \frac {1.2c*mins} {\frac{4c} {5}} = \frac{3} {2} mins [/tex]
And so, the answer for a would be 1.5 minutes, b would be 1.2 c minutes.

Is this so far correct?
 
  • #4
Yes, that looks correct to me.

For (c) I don't think the equations you have written are enough, as they are simplifications of the full Lorentz equations. The simplified equations only cover scaling and tell us nothing about simultaneity.

Question (c) asks for the frame-AB time coordinate of the spacetime point P that is the intersection of the worldline of B and the line of simultaneity in frame C that passes through the spacetime point Q at which C passes A.

The full equations, that enable calculation for (c) are here.
 
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  • #5
Nice!

Hm, I see.

[tex] t' = \gamma(t-\frac{vx} {c^2}) [/tex] Should be the one we are looking for.

t' = B's reading when A passes C.

[tex] \gamma = \frac{1} {sqrt{1-\frac{v^2} {c^2}}} [/tex]

Well, we know x should be 1.2 c minutes apart part b
I suppose t = 3/2 minutes now from part a
v = c*4/5These are all in C's frame.

So what we get is the following

[tex] t' = \frac{1.5-\frac{4*1.2c^2} {5c^2}} {\sqrt{1-\frac{16c^2} {25c^2}}} [/tex]

And this equals 0.9 minutes.

Although, I'm not really sure why using these values for t, v, x all work out for the initial time that it reads.
This seems fishy, but, the answer appears to be OK (or at least make sense).
 
  • #6
Can anyone confirm my reasoning for the last post?

My answer of 0.9 minutes seems reasonable. Q: In C's frame, when A passes C, what time does B read?
When A passes C, the time on B reads 0.9 minutes.

My only concern is that I used the information for C over an elapsed time period, not the initial settings (as there I'm lost on how I'd go about that...).

Why does this work ? (permitting this is the correct answer 0.9 minutes).
 
  • #7
RJLiberator said:
Can anyone confirm my reasoning for the last post?

My answer of 0.9 minutes seems reasonable. Q: In C's frame, when A passes C, what time does B read?
When A passes C, the time on B reads 0.9 minutes.

My only concern is that I used the information for C over an elapsed time period, not the initial settings (as there I'm lost on how I'd go about that...).

Why does this work ? (permitting this is the correct answer 0.9 minutes).

It's not 0.9 minutes. That's something else that is relevant here but not the answer to c).

(It's really confusing calling those the "Lorentz" equations. Those are the time dilation and length contraction equations, not to be confused with the Lorentz Transformation. Where does that terminology come from?)

There are several ways to do part c). You could ask the following questions:

1) In the A-B frame, what do both clocks read when C passes B?

2) In C's frame, what how much does B's clock advance between C passing A and B?

3) Can you use these two calculations to get the answer to c)?
 
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  • #8
1) In the A-B frame, what do both clocks read when C passes B?
Well, we know that 1.5 minutes is the time elapsed when C reaches B in C's frame.

[tex] 1.5mins = t\sqrt{1-\frac {16} {25}} => t = 2.5 minutes [/tex]

That makes sense as the velocity = 4c/5 so you would expect it to be an elapsed time greater than the 2 minutes it takes speed to travel the distance.
2) In C's frame, what how much does B's clock advance between C passing A and B?

B's clock advances from 0 to 1.5 minutes in C's frame. B's clock advances 1.5 minutes.

3) Can you use these two calculations to get the answer to c)?
So, in c's frame, when A passes C that must been that B reads 1.0 minutes.

A = 0 minutes when C see's A passing it (in c's frame).
B = 1 minute when C see's A passing it (in c's frame)

That way, when 1.5 minutes elapses (time elapsed) we get 2.5 total minutes.
(It's really confusing calling those the "Lorentz" equations. Those are the time dilation and length contraction equations, not to be confused with the Lorentz Transformation. Where does that terminology come from?)

noted!
 
  • #9
That's not right. The best approach is to analyse the problem entirely from the A-B frame first. In the A-B frame:

C passes A at ##t = 0##

C passes B at ##t = 2c.mins/0.8c = 2.5 mins##

Therefore, when C passes B, both A and B's clocks must read 2.5 minutes in the A-B frame. And C's clock reads something else. I think you've worked this out, it's 1.5 minutes.

Now, an important point. B's clock reads 2.5 minutes when C passes B full stop! And C's clock reads 1.5mins full stop. All other observers will agree on this: when that event took place (C passed B): the time in B's frame (at point B) was 2.5 minutes and the time in C's frame (at point C)was 1.5 minutes full stop.

Now, can you analyse the problem from C's frame, starting when C is at A (##t = t' = 0##) until B reaches C?

Hint: at ##t' = 0## you have an unknown time on B's clock: call it ##t_0## say. And work from there.
 
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  • #10
Okay, so with the hint from earlier to use the Lorentz transformations for part c, and with your help, here is what I have thus far.

[tex] t = \gamma(t'+\frac {vx'} {c^2}) [/tex]

Filling in with t' = 0, x' = 1.2 light minutes, and v = 4c/5

we get the answer of 1.6 minutes.I see how I used t' = 0. That makes sense, and we are trying to find t_0 in C's frame. I'm using the correct distance and the correct velocity.

I think the final answer is 1.6 minutes is what B reads.

But, not sure how this makes sense, if at t=0 in A, t=1.6 minutes in B, in c's frame. I would think the answer would be closer to 0.
 
  • #11
RJLiberator said:
Okay, so with the hint from earlier to use the Lorentz transformations for part c, and with your help, here is what I have thus far.

[tex] t = \gamma(t'+\frac {vx'} {c^2}) [/tex]

Filling in with t' = 0, x' = 1.2 light minutes, and v = 4c/5

we get the answer of 1.6 minutes.I see how I used t' = 0. That makes sense, and we are trying to find t_0 in C's frame. I'm using the correct distance and the correct velocity.

I think the final answer is 1.6 minutes is what B reads.

But, not sure how this makes sense, if at t=0 in A, t=1.6 minutes in B, in c's frame. I would think the answer would be closer to 0.

To answer your last question, you should go through the scenario in C's frame. You have used the Lorentz Transformation above to solve the problem directly. But, if you start with unknown ##t_0## on B's clock and calculate the time that elapses on B's clock during its motion towards C, then you should be able to confirm the answer you got and perhaps shed some light on why ##t_0 \ne 0##.
 
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  • #12
RJLiberator said:
But, not sure how this makes sense, if at t=0 in A, t=1.6 minutes in B, in c's frame. I would think the answer would be closer to 0.
A spacetime diagram is really helpful to see what's going on as well. C's "now" when t'=0 corresponds to the x'-axis. You can see in the diagram, this axis intersects B's world line when t=1.6 min.
 

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The diagram does help out a lot. I imagine we are on the verge of learning how to develop those graphs.
 

FAQ: Special Relativity Question (Lorentz)

1. What is the theory of special relativity?

The theory of special relativity, also known as the Lorentz transformation, is a fundamental theory in physics that explains how time and space are perceived differently by observers moving at different speeds. It was proposed by Albert Einstein in 1905 and has been extensively tested and confirmed through various experiments.

2. How is special relativity different from general relativity?

Special relativity deals with the behavior of objects and observers in an inertial reference frame, while general relativity includes the effects of gravity and acceleration. Special relativity applies to all objects in the absence of gravity, while general relativity applies to objects in the presence of gravity and non-inertial reference frames.

3. What is the Lorentz factor in special relativity?

The Lorentz factor, denoted by the symbol γ, is a quantity that describes the relationship between an object's velocity and its observed time and length. It is given by the equation γ = 1/√(1-(v^2/c^2)), where v is the velocity of the object and c is the speed of light. This factor becomes significant at high velocities and explains phenomena such as time dilation and length contraction.

4. Can special relativity be applied to everyday situations?

Yes, special relativity has many practical applications in everyday life. For example, GPS satellites use special relativity to accurately calculate the positions of objects on Earth. It also helps to understand the behavior of particles at high speeds in particle accelerators, and is essential in the development of technologies such as nuclear power and nuclear weapons.

5. Is special relativity still relevant today?

Absolutely. Special relativity is still a fundamental part of modern physics and has been confirmed by countless experiments and observations. It is used in various fields such as astrophysics, cosmology, and particle physics, and has led to groundbreaking discoveries and advancements in our understanding of the universe.

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