Special relativity - transformation of angle

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SUMMARY

This discussion focuses on the transformation of angles in special relativity, specifically addressing the use of Lorentz transformations and the gamma factor. The key equations involved include the gamma factor, $$\gamma = \frac{1}{\sqrt{1-\beta^2}}$$, and the Lorentz contraction formula, $$l'=\frac{l}{\gamma}$$. A common mistake identified is the failure to apply the Lorentz transformation correctly, leading to issues with simultaneity. The correct approach involves using the Earth's frame to analyze light emission and its trajectory, ultimately leading to the angle transformation formula $$\tan \theta' = \frac{y}{\gamma(x-vr/c)}$$.

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  • Understanding of special relativity concepts, including Lorentz transformations
  • Familiarity with the gamma factor in special relativity
  • Basic knowledge of trigonometry, particularly tangent functions
  • Ability to manipulate algebraic expressions involving relativistic equations
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Toby_phys
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Homework Statement


Capture.jpg


Homework Equations


Gamma factor:
$$\gamma = \frac{1}{\sqrt{1-\beta^2}} $$
Lorentz contraction
$$l'=\frac{l}{\gamma}$$
Trig:
$$ cos\theta = \frac{adjacent}{hypotenuse}$$

The Attempt at a Solution


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I have all the quantities but the algebra doesn't seem to work out.

Thank you in advance for any help
 
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You've probably approached it the wrong way. Think about energy-momentum transformations for light instead.
 
wow, that was soo easy. Thank you.

However what was wrong with my method? I understand why your way works, but why didn't mine?
 
Toby_phys said:
wow, that was soo easy. Thank you.

However what was wrong with my method? I understand why your way works, but why didn't mine?

There's a relativity of simultaneity issue that you missed. You need to use a Lorentz Transformation on the x-coordiate, not simply a length contraction.
 
Oh ok, thank you
 
I found my notes on this. If we do things in the Earth's frame first, with light emitted at ##t=0## with the star at ##(0,0)## and the Earth at ##(x,y)##, then ##\tan \theta = \frac{y}{x}##

Note that the light reaches Earth at ##t = \frac{r}{c}## where ##r^2 = x^2 + y^2##

In the star's frame, the light is emitted from ##(0,0)## at ##t'=0## and reaches the Earth at ##(x', y') = (\gamma(x-vt), y)## at some time ##t'## that isn't important.

So, ##\tan \theta' = \frac{y'}{x'} = \frac{y}{\gamma(x-vt)} = \frac{y}{\gamma(x-vr/c)}##

If you work through that and do a bit of trig manipulation, you should get the same answer.
 

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