Doppler Effect for Light — Question 1

Section 37-9 · Physics pages 6192–6193

Question 1 A wavelength ratio gives an exact recession speed A spectral line has source-rest wavelength λ0 = 400 nm and is received at λ = 600 nm. Assume purely longitudinal recession in flat spacetime, with no other shift. x D S light v Schematic; labels, not drawing lengths, specify the data. (a) Invert λ/λ0 = √ (1 + β)/(1 −β) for the signed recession speed. (b) Find the corresponding frequency ratio and compare with the low-speed estimate β ≃z, where z = (λ −λ0)/λ0.
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Question 1 - Solution A wavelength ratio gives an exact recession speed x D S light v (a) Method and calculation R = λ/λ0 = 3/2, R2(1 −β) = 1 + β. β = R2 −1 R2 + 1 = 5/13 ≃0.384615 . (b) Interpretation and further calculation f/f0 = 1/R = 2/3 . z = 0.500, β̸ = z at this shift. Physical check The longer wavelength indicates recession; a cosmological or gravitational shift would require a different physical model.

Question 1

A wavelength ratio gives an exact recession speed

A spectral line has source-rest wavelength λ0=400nm\lambda_0=400\,\mathrm{nm} and is received at λ=600nm\lambda=600\,\mathrm{nm}. Assume purely longitudinal recession in flat spacetime, with no other shift.

Diagram shown in the original SVG worksheet.

  1. Invert λ/λ0=(1+β)/(1−β)\lambda/\lambda_0=\sqrt{(1+\beta)/(1-\beta)} for the signed recession speed.

  2. Find the corresponding frequency ratio and compare with the low-speed estimate β≃z\beta\simeq z, where z=(λ−λ0)/λ0z=(\lambda-\lambda_0)/\lambda_0.

Question 1 - Solution

A wavelength ratio gives an exact recession speed

Diagram shown in the original SVG worksheet.

(a) Method and calculation

R=λ/λ0=3/2,R2(1−β)=1+β.R=\lambda/\lambda_0=3/2,\quad R^2(1-\beta)=1+\beta.β=R2−1R2+1=5/13≃0.384615.\boxed{\beta=\frac{R^2-1}{R^2+1}=5/13\simeq0.384615}.

(b) Interpretation and further calculation

f/f0=1/R=2/3.\boxed{f/f_0=1/R=2/3}.z=0.500,β≠zat this shift.z=0.500,\qquad\beta\ne z\quad\text{at this shift}.

Physical check

The longer wavelength indicates recession; a cosmological or gravitational shift would require a different physical model.