Derivation of Relativisitic Doppler effect with angle

In summary: First, you realize they're talking about light waves, right? I mean, couldn't be sound waves at relativistic speeds.In summary, the relativistic Doppler effect occurs when the frequency of light emitted from a source changes due to the relative motion of the source and receiver. The effect is strongest when the angle between the source and receiver is the smallest.
  • #1
Arman777
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Homework Statement


Derive the formula for the Doppler effect for a receiver traveling at an angle theta away from a planar source

Homework Equations

The Attempt at a Solution


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I thought that we can assume that the wavelength has two components ##λ_x## and ##λ_y## where

##λ_x = ct+vtcosθ## and I am not sure about ##λ_y##. Maybe ##λ_y = \sqrt {(ct)^2+ (vtsinθ)^2)}##

I am not sure how to start or approach please help.

Note : I cannot use wave equation.
 
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  • #2
Are you going to model light as a wave or as massless particles, with energy and momentum?
 
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  • #3
PeroK said:
Are you going to model light as a wave or as massless particles, with energy and momentum?
I am not sure actually. Why its important ?. We can't use four vectors or etc.. we didnt learn them.. We can use basic stuff like lorentz transformation only actually.
 
  • #4
Arman777 said:
I am not sure actually. Why its important ?. We can't use four vectors or etc.. we didnt learn them.. We can use basic stuff like lorentz transformation only actually.

Okay, so you can't use the energy-momentum transformation. What about expressing light as a plane wave?
 
  • #5
I suggest the following:
  • Write down the phase function of the wave. You can assume a plane wave moving in the ##x##-direction for this purpose.
  • Write down an expression for the world line of the observer.
  • For a small change in ##t##, determine the change ##d\phi## in the phase function along the world line of the observer.
  • Determine the proper time ##ds## passed for the observer in the same small time difference.
  • The frequency observed by the observer is ##d\phi/ds##.
  • You can find the original frequency by doing the same for the emitter.
 
  • #6
Orodruin said:
I suggest the following:
  • Write down the phase function of the wave. You can assume a plane wave moving in the ##x##-direction for this purpose.
  • Write down an expression for the world line of the observer.
  • For a small change in ##t##, determine the change ##d\phi## in the phase function along the world line of the observer.
  • Determine the proper time ##ds## passed for the observer in the same small time difference.
  • The frequency observed by the observer is ##d\phi/ds##.
  • You can find the original frequency by doing the same for the emitter.
Thats kind of hard for me to do. I can try step by step tho but I am not sure I can find it. Is there a simpler way ? Or is there a way without writing plane-wave equation ? . I find a online derviation and it uses planes waves and lorentz transformation. Probably this is what you are trying to describe.

I
 
  • #7
The wording of the problem would seem to allow starting with the expression for the relativistic Doppler shift head-on. Then just figure out the effect of theta.
 
  • #8
rude man said:
The wording of the problem would seem to allow starting with the expression for the relativistic Doppler shift head-on. Then just figure out the effect of theta.
How..
 
  • #9
Arman777 said:
How..
First, you realize they're talking about light waves, right? I mean, couldn't be sound waves at relativistic speeds.

So how about using the relativistic expression for straight-back light travel (not at an angle to the source-receiver line), then considering how the effective rate of travel as seen by the receiver is impacted by an angle other than zero? Looks like plain old trig to me - but that's just me. :rolleyes:
 

1. What is the Relativistic Doppler effect?

The Relativistic Doppler effect is a phenomenon in which the perceived frequency of a wave (such as light or sound) changes due to the relative motion between the source of the wave and the observer. It takes into account the effects of special relativity, including time dilation and length contraction.

2. How does the Relativistic Doppler effect differ from the classical Doppler effect?

The classical Doppler effect only takes into account the relative motion between the source and observer, while the Relativistic Doppler effect also considers the effects of special relativity. This means that the perceived frequency shift is greater in the relativistic case, especially at high speeds.

3. What is the equation for the Relativistic Doppler effect with angle?

The equation is: fo = fs * √((1 + v/c) / (1 - v/c)) * (1 - (v/c) * cosθ) where fo is the observed frequency, fs is the source frequency, v is the relative velocity between the source and observer, c is the speed of light, and θ is the angle between the direction of motion and the direction of observation.

4. How is the Relativistic Doppler effect with angle used in real-world applications?

The Relativistic Doppler effect with angle is used in various fields such as astronomy, where it helps astronomers determine the relative motion of celestial objects. It is also used in radar and sonar systems to accurately measure the speed and direction of moving objects.

5. What are the limitations of the Relativistic Doppler effect with angle?

One limitation is that it only applies to objects moving at speeds close to the speed of light. It also assumes a constant relative velocity and does not take into account other factors like gravitational effects. Additionally, it only applies to waves traveling in a straight line and does not account for reflections or diffractions.

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