Special Relativity: Angles in different Inertial Systems

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Homework Help Overview

The discussion revolves around a problem in special relativity concerning the emission of light from a moving source. The original poster presents a scenario where a light source at rest in an inertial frame emits light at a specific angle, and the task involves transforming this angle into another inertial frame moving relative to the first. The problem includes multiple parts, focusing on the relationship between angles and velocities in different reference frames.

Discussion Character

  • Exploratory, Conceptual clarification, Mathematical reasoning

Approaches and Questions Raised

  • The original poster attempts to solve parts a) and b) of the problem, indicating that they have successfully applied trigonometric relationships and the constancy of the speed of light. However, they express uncertainty regarding part c), questioning the specific angle to find and the implications of the speed being close to the speed of light. Some participants clarify that part c) involves finding the angle related to the previous part and suggest focusing on the relationship between the angle and the Lorentz factor.

Discussion Status

Participants are actively engaging with the problem, with some providing clarifications on the requirements of part c). There is a recognition that understanding the angle to focus on was a significant hurdle. The discussion is productive, with participants guiding each other towards a clearer understanding of the problem's requirements.

Contextual Notes

The original poster notes ambiguity in the problem text regarding the angle to be found and the context of speeds close to the speed of light. This uncertainty is acknowledged by other participants, who emphasize the importance of correctly interpreting the problem's requirements.

Guybrush
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Homework Statement


a) A light-source at rest in an inertial system S' is emitting light with angle θ' relative to the x'-axis. The System S' is moving at speed v (along the x-axis) relative to the laboratory system S. Show that the emitted light is making an angle θ with the x-axis of:

\cos \theta = \frac{c \cos \theta' + v}{c + v\cos \theta'}

b) Now assume that the light-source is emitting its light isotropically in its own reference system. Show, that the part of the light being emitted into the forward-going hemisphere is located within a cone with half angle:

\cos \theta = v/c

c) Show that this angle, for speeds close to c, can be approximated with \gamma^{-1}, where \gamma = \frac{1}{\sqrt{1 - v^2/c^2}}

(Tip given in the text: \sin^2 x + \cos^2 x = 1, and \sin x \approx 1, x << 1)

Homework Equations


The relevant equations are the equations for transforming speeds in different inertial systems
u_x = \frac{u'_x + v}{1 + u'_xv/c^2}
u_{y,z} = \frac{u'_{y,z}}{\gamma (1 + u'_xv/c^2)}

The Attempt at a Solution


Parts a), and b) I have solved with no problem. In part a) you just realize that the speed of light is constant in all reference frames so that u = u' = c. Using standard trigonometry you get that u'_x = c \cos \theta'. You get u_x by inserting in the equation above. Then \cos \theta = u_x/u, which reduces to the correct answer.

In part b) you just use the limiting case where θ' = 90°, which reduces to the correct equation.

In part c) I am not sure what to do. In large part because the problem text seems very ambiguous (what angle am I supposed to find? What speed is close to the speed of light, is it the relative speed between the inertial systems or have we ceased looking at light, and instead some other particle emitting at speeds close to the speed of light?). I have tried taylor expanding the above result in v/c around 1, but the math gets so convoluted, that I doubt this is the right approach.

I have translated the problem text above from another language into english, but I hope it is still understandable. Any help would be much appreciated.
 
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hi, nice work so far. uh, for part c) you are meant to find the angle from part b), i.e. you are meant to find the angle theta in this equation: ##\cos(\theta)=v/c## And you are meant to assume v is close to c. So you are still considering a source which emits light, except now they are saying the source itself is going at close to the speed of light. It is not too difficult from here, as long as you start in the right place. You have two equations:
##\gamma=\frac{1}{1-v^2/c^2}##
##\cos(\theta)=v/c##
And you are told to get an equation which relates some function of ##\theta## to ##\gamma## (i.e. no ##v## involved). What is the simplest way to do this?
 
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Ah, yes. I see now. You just insert \cos^2 \theta in place of v^2/c^2 in the Gamma function, and reduce for the angle, while using the trigonometric identities given in the problem. A large part of my problem was that I did not even realize what angle to look for. Thanks a bunch!
 
ah yeah, no problem. yes, I agree the hardest bit of part c) was seeing what it is they wanted. (which can often be the hardest bit of a lot of physics problems!)
 

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