Answer: What is the angle \alpha in B's frame with relativistic kinematics?

In summary, the velocity of B w.r.t A is 0.6c and the attempt at a solution is to lengthen AC and BC in B's frame so that: AC'=\frac{1}{\sqrt{1-(v_{x}/c)^{2}}} \cdot 12 = \frac{60 \sqrt{82}}{41} and BC'=\frac{1}{\sqrt{1-(v_{y}/c)^{2}}} \cdot 12 = \frac{60 \sqrt{82}}{41}.
  • #1
PhMichael
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Homework Statement


The velocity of B w.r.t A is:

[tex]\vec{v}=0.6c\left ( \frac{\hat{x}-\hat{y}}{\sqrt{2}} \right )[/tex].

what is [tex]\alpha[/tex] (the 90 degrees of the triangle in A's frame) in B's frame?


2. The attempt at a solution

AC and BC will each be lengthened in B's frame, so that:

[tex] AC' = \frac{1}{\sqrt{1-(v_{x}/c)^{2}}} \cdot 12 = \frac{60 \sqrt{82}}{41} [/tex]

[tex] BC' = \frac{1}{\sqrt{1-(v_{y}/c)^{2}}} \cdot 12 = \frac{60 \sqrt{82}}{41} [/tex]

where,

[tex]v_{x}=v_{y}=\frac{0.6c}{\sqrt{2}} [/tex]

But here I'm stuck and can't proceed ... any guidance will be appreciated :)
 
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  • #2
In B's frame, the two legs of the triangle will be length contracted, not lengthened. Moreover, it's not a simple scaling of the entire length of each segment since only lengths in the direction of motion are contracted.
 
  • #3
vela said:
In B's frame, the two legs of the triangle will be length contracted, not lengthened. Moreover, it's not a simple scaling of the entire length of each segment since only lengths in the direction of motion are contracted.

umm, from Lorentz tranf. i get that they're lengthened and i did use the fact that the only legs who are seen "deformed" (+/-) are the ones in the direction of motion, that's why I used the x component of the velocity for AC and the y component for BC.

By lorentz I get:

[tex] \Delta x' = \gamma_{x} \Delta x [/tex] , where, [tex]\Delta x'=AC' [/tex]
[tex] \Delta y' = \gamma_{y} \Delta y [/tex] , where, [tex]\Delta y'=BC' [/tex]

As: [tex]\Delta t = 0 [/tex]

NO?
 
  • #4
Oh, OK, I see what you were doing. By treating the components of the velocity separately, you're essentially looking at a Lorentz boost in the x-direction combined with a separate boost in the y-direction. That combination, however, doesn't yield the same result as a single boost in the direction of B's velocity. You can see this by considering what happens to AB. In the case of a single boost, its length remains unchanged because it's perpendicular to B's velocity. But when you have two separate boosts, both boosts will cause its length to decrease because it's not perpendicular to either component of the velocity.

The other point of confusion comes from applying the Lorentz transformation to find the length of the segments measured by B. You're calculating the spatial distance between two spacetime events when Δt=0, but from B's point of view, those two events occur at different times. You want to calculate the spatial distance when Δt'=0.
 
  • #5
OK, let me see if I've got you correctly:

[tex] v=|\vec{v}|=0.6c \to \gamma = 1.25 [/tex]

[tex]AB'=AB=12 \sqrt{2} [/tex]

[tex]AC'=BC'=\frac{12}{\gamma}=\frac{12}{1.25}=9.6 [/tex]

and by the law of cosines, we obtain [tex]\alpha[/tex] :

[tex] (12 \sqrt{2} )^{2} = 2(9.6)^{2} - 2(9.6)^{2}cos \alpha [/tex]

[tex] \alpha = 124.23^{o} [/tex]

Is this correct?
 
  • #6
No. The segments AC and BC don't contract by the factor of γ because they have a component perpendicular to v. Only the component parallel to v becomes shorter.
 
  • #7
Wow, what a messy question ... So I gusee i'll need to describe each leg in the directions parallel and perpindicular to the velocity direction:

[tex] AB'=AB=12 \sqrt{2} [/tex]

-----------------

[tex]AC_{\parallel}=6 \sqrt{2} \to AC_{\perp}=6 \sqrt{2}[/tex]

[tex] AC'_{\parallel}=\frac{AC_{\parallel}}{\gamma}=6.788 [/tex] , [tex]AC'_{\perp}=AC_{\perp}=6 \sqrt{2} [/tex]

[tex] AC' = \sqrt{(AC'_{\parallel})^{2}+(AC_{\perp})^{2}}=10.866 [/tex]

-----------------

[tex]BC_{\parallel}=6 \sqrt{2} \to BC_{\perp}=6 \sqrt{2}[/tex]

[tex] BC'_{\parallel}=\frac{BC_{\parallel}}{\gamma}=6.788 [/tex] , [tex]BC'_{\perp}=BC_{\perp}=6 \sqrt{2} [/tex]

[tex] BC' = \sqrt{(BC'_{\parallel})^{2}+(BC_{\perp})^{2}}=10.866[/tex]

------------------

and then by using the law of cosines, i get:

[tex]\alpha = 102.68 [/tex] Is it now right?!
 
Last edited:
  • #8
How'd you get 9.6 for the parallel components of AC' and BC'? I don't get that number.

As a sanity check, do you expect the angle α to be bigger or smaller as observed by B given how you expect the triangle to change shape?
 
  • #9
I got it by dividing 12 over [tex]\gamma = 1.25 [/tex].

I think it should be larger than 90 degrees so there must be something messed up.
 
  • #10
I've screwed up ... i should've divided that parallel component by gamma!
 
  • #11
I've just edited the calculations ... can you please go over them quickly and let me know if they now seem OK ? :smile:
 
  • #12
Looks good!
 
  • #13
thanks pal! :wink:
 

1. What is relativistic kinematics?

Relativistic kinematics is a branch of physics that studies the motion of objects at speeds close to the speed of light, taking into account the principles of special relativity.

2. How does relativistic kinematics differ from classical kinematics?

Relativistic kinematics takes into account the effects of time dilation and length contraction, which are not present in classical kinematics. It also uses the concept of four-vectors and Lorentz transformations to describe the motion of objects at high speeds.

3. What is the importance of relativistic kinematics in modern physics?

Relativistic kinematics is essential in understanding the behavior of particles at high energies, such as those in particle accelerators. It is also used in fields such as astrophysics and cosmology to describe the motion of objects at extreme speeds.

4. What is the equation for relativistic velocity?

The equation for relativistic velocity is v = c * tanh(c/b), where c is the speed of light and b is the velocity of the object relative to the observer.

5. Can relativistic kinematics be applied to everyday situations?

Yes, relativistic kinematics can be applied to everyday situations, although the effects may be very small and difficult to observe. For example, GPS satellites must take into account the principles of special relativity in order to accurately calculate positions on Earth.

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