Angular Momenta and Magnetic Dipole Moments — Question 10

Section 40-3 · Physics pages 6630–6631

Question 10 A normal Zeeman triplet follows transition energies rather than upper levels alone Consider an ideal spinless electric-dipole transition from lu = 1 to ll = 0. Its zero-field photon energy is E0. Use orbital shifts mlµBB and allowed ∆ml = 0, ±1. ll = 0 Schematic; labels, not drawing lengths, specify the data. (a) Find the possible emitted photon energies. (b) For E0 = 2.00 eV and B = 1.00 T, estimate the magnitude of the wavelength shift of either outer component using hc = 1240 eV nm and µB = 5.788 × 10−5 eV/T.
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Question 10 - Solution A normal Zeeman triplet follows transition energies rather than upper levels alone ll = 0 (a) Method and calculation mlower l = 0, mupper l = −1, 0, 1. Eγ = E0 −µBB, E0, E0 + µBB . (b) Interpretation and further calculation λ = hc/E ⇒δλ ≃−hc E2 0 δE, λ0 = 620 nm. |δλ| ≃1240(5.788 × 10−5) (2.00)2 = .01794 nm . Physical check Transition energies subtract both upper and lower shifts. Here the lower shift vanishes; the shorter-wavelength component has the larger photon energy.

Question 10

A normal Zeeman triplet follows transition energies rather than upper levels alone

Consider an ideal spinless electric-dipole transition from lu=1l_u=1 to ll=0l_l=0. Its zero-field photon energy is E0E_0. Use orbital shifts mlμBBm_l\mu_BB and allowed Δml=0,±1\Delta m_l=0,\pm1.

Diagram shown in the original SVG worksheet.

  1. Find the possible emitted photon energies.

  2. For E0=2.00eVE_0=2.00\,\mathrm{eV} and B=1.00TB=1.00\,\mathrm T, estimate the magnitude of the wavelength shift of either outer component using hc=1240eVnmhc=1240\,\mathrm{eV\,nm} and μB=5.788×10−5eV/T\mu_B=5.788\times10^{-5}\,\mathrm{eV/T}.

Question 10 - Solution

A normal Zeeman triplet follows transition energies rather than upper levels alone

Diagram shown in the original SVG worksheet.

(a) Method and calculation

mllower=0,mlupper=−1,0,1.m_l^{\mathrm{lower}}=0,\quad m_l^{\mathrm{upper}}=-1,0,1.Eγ=E0−μBB,E0,E0+μBB.\boxed{E_\gamma=E_0-\mu_BB,\ E_0,\ E_0+\mu_BB}.

(b) Interpretation and further calculation

λ=hc/E⇒δλ≃−hcE02δE,λ0=620nm.\lambda=hc/E\Rightarrow\delta\lambda\simeq-\frac{hc}{E_0^2}\delta E,\quad\lambda_0=620\,\mathrm{nm}.|δλ|≃1240(5.788×10−5)(2.00)2=.01794nm.\boxed{|\delta\lambda|\simeq\frac{1240(5.788\times10^{-5})}{(2.00)^2}=.01794\,\mathrm{nm}}.

Physical check

Transition energies subtract both upper and lower shifts. Here the lower shift vanishes; the shorter-wavelength component has the larger photon energy.