Doppler effect in Special relativity -- Solution verification

In summary, during the first part of the trip, rocket A approaches stationary observer B at a velocity of 0.6 c, with a travel time of 6 hours, resulting in a total of 4.8 signals received by B at a doubled frequency. The turnaround time for B to detect A's movement is 0.4 times the travel time. In the second part of the trip, A moves away from B at a velocity of 5/13 c, with a travel time of 12 hours, resulting in a total of 16 signals received (4.8 from the first part and 11.2 from the second part). This assumes that A and B are far enough apart for B to receive signals from
  • #1
romanski007
12
1
Homework Statement
The question was taken from the past exam paper.


Two rockets A and B are moving relative to each other. Rocket A emits a monochromatic signal of wavelength 600 nm every 1 hour ($$f_A$$ = 1 per hour), while rocket B receives them at a wavelength of 300 nm for the first part of the trip which took 6 hours from rocket A perspective.


The second part of the trip took 12 hours from rocket A perspective and rocket B observed a wavelength of 900 nm.

Determine the total number of signals received by rocket B for the entire duration of the trip.

Provided formula for the relative velocity of two rockets was $$v = c \frac{1-(\frac{\lambda_b} {\lambda_a})^2}{1+(\frac{\lambda_b} {\lambda_a})^2} $$
Relevant Equations
$$v = c \frac{1-(\frac{\lambda_b} {\lambda_a})^2}{1+(\frac{\lambda_b} {\lambda_a})^2} $$
I am assuming that B is a stationary observer here.
For the first part of the trip, using the formula, rocket A is approaching B at velocity $$v_A$$ =0.6 c.

The length that A travels is $$L_A = v_A t_1 $$ where $$t_1 = $$ 6 hrs. For the first part of the trip, B is receiving signals at a rate $$2 f_A$$ because the wavelength is halved and thus frequency is doubled.

The time taken for B to detect the turnaround of A is given by $$T_1 = \frac{L_1}{v_1} - \frac {L_1}{c} $$ where the first term is the length and the second term comes from the fact that A is approaching B.

Thus substituting, $$T_1 = 0.4t_1$$ and the total number of signals received $$N_1 = 2 f_A T_1 $$ = 4.8 signals.

For the second part, A is moving away with a velocity $$v_2 = \frac{5}{13} c $$ where the formula was used once again. The frequency is now given by $\frac{2}{3} f_A$ and the time of travel was $$ T_ 2 = \frac{L_2}{v_2} + \frac{L_2}{c}$$ where $$L_2 = v_2 t_2$$ and $$t_2$$ = 12 hours.
Furthermore second term emerges due to A moving away from B.

Thus total number of signals for second part is $$N_2 = \frac{2}{3} f_A T_2 = \frac{144}{13}$$ signals

Thus $$N = N_1 + N_2 = \frac{144}{13} + 4.8 = 16$$ signals
 
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  • #2
There must be some additonal assumptions or information. If A and B are far enough apart, then B will receive no signals from A.
 

FAQ: Doppler effect in Special relativity -- Solution verification

What is the Doppler effect in special relativity?

The Doppler effect in special relativity is a phenomenon where the observed frequency of a wave (such as light or sound) is affected by the relative motion between the source of the wave and the observer. It is a result of the time dilation and length contraction effects predicted by Einstein's theory of special relativity.

How does the Doppler effect in special relativity differ from the classical Doppler effect?

In classical physics, the Doppler effect only takes into account the relative motion between the source of the wave and the observer. However, in special relativity, the Doppler effect also takes into account the time dilation and length contraction effects caused by the relative motion between the source and observer. This means that the observed frequency of the wave can be affected by the relative velocity between the source and observer, as well as the angle of motion.

What is the formula for calculating the Doppler effect in special relativity?

The formula for calculating the Doppler effect in special relativity is given by f_obs = f_src * √((1 + v/c) / (1 - v/c)), where f_obs is the observed frequency, f_src is the source frequency, v is the relative velocity between the source and observer, and c is the speed of light.

Can the Doppler effect in special relativity be observed in everyday life?

Yes, the Doppler effect in special relativity can be observed in everyday life. For example, the colors of stars appear to shift towards the blue end of the spectrum when they are moving towards Earth and towards the red end when they are moving away from Earth. This is due to the Doppler effect in special relativity.

How is the Doppler effect in special relativity used in scientific research?

The Doppler effect in special relativity is used in various fields of science, such as astronomy, cosmology, and particle physics. It allows scientists to measure the relative velocities of objects in space, study the expansion of the universe, and analyze the behavior of particles in high-speed collisions. It also helps in the development of technologies such as radar and GPS systems.

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