How to Derive the Angle Transformation of a Stationary Rod in Relativity?

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An observer in frame S' sees a stationary rod at an angle φ' with the x' axis, while an observer in frame S sees it at angle φ with the x axis. The relationship between these angles is expressed as tan(φ') = (1/γ) tan(φ), where γ is the Lorentz factor. The discussion highlights the importance of correctly applying the Lorentz transformation to the coordinates of the rod's endpoints to derive the angle transformation. It clarifies that the correct calculation of tan(φ) involves the differences in coordinates (∆y/∆x) rather than simply y/x. The conversation emphasizes the need to consider the effects of relativistic length contraction on the rod's dimensions in different frames.
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An observer in S' sees a stationary rod lying in the x'-y' plane and making an angle \phi' with the x' axis. Show that
\tan{\phi'}=\frac{1}{\gamma} \tan{\phi}

where \phi is the angle the rod makes with the x-axis according to an observer in S.

so far I have \tan{\phi'} = \frac{y'}{x'}=\frac{y}{\gamma(x-vt)}=\frac{1}{\gamma} \frac{y}{x-vt}

if i could just get rid of that vt, i'd be there but i can't seem to get it to go away...
 
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I assume the rod is moving in the x direction. In the S frame, let the length in the x direction be Lx and it's length in the y direction be Ly. In the S' frame, the length in the y direction will be the same i.e. L'y = Ly, and the length in the x direction will be shorter by a factor of √(1 - v²), i.e. L'x = √(1 - v²) Lx. So we get

tan θ = Ly / Lx

tan θ' = L'y / L'x = Ly/Lx√(1 - v²)
 


Your mistake was that you took tan θ to be y/x. If the coordinates of the tips of the rod are (x1, y1) and (x2, y2), then tan θ will be ∆y/∆x where ∆x = x2 - x1 and ∆y = y2 - y1. You should apply the Lorentz transform to both (x1, y1) and (x2, y2) to obtain ∆x' and ∆y'. tan θ' will then be ∆y'/∆x'.
 

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