X-rays — the Continuous Spectrum, Characteristic Lines and Moseley's Law
Characteristic Lines
If an incoming electron ejects a K-shell (n = 1) electron of a target atom, an electron from a higher shell drops into the vacancy and emits a photon equal to the energy difference. L → K gives the Kα line, M → K the Kβ line; vacancies in the L shell give the L series. Because M is farther from K than L is, Kβ has more energy and a shorter wavelength than Kα. These lines appear only once eV exceeds the K-shell binding energy, but once they appear their wavelengths do not move when V is raised further — they belong to the atom.
| Feature | Continuous spectrum | Characteristic lines |
|---|---|---|
| Origin | Deceleration of electrons near nuclei | Electron transitions into inner-shell vacancies |
| Set by | Accelerating voltage (λ_min = hc/eV) | Atomic number of the target |
| Raise V | λ_min shifts to shorter wavelength | Wavelengths unchanged (lines may brighten) |
| Raise filament current | More intense, same λ_min | More intense, same wavelengths |
Moseley's Law — Counting Protons with X-rays
Moseley measured the Kα frequency for element after element and found √ν = a(Z − b): the square root of the frequency is a straight-line function of the atomic number Z. For Kα the screening constant is b ≈ 1 — the one remaining K electron shields one unit of nuclear charge from the L electron that falls in — and a Bohr-type estimate gives ν(Kα) ≈ (3/4) R c (Z − 1)², or an energy of about 13.6 × (3/4)(Z − 1)² eV. For copper, Z = 29, that is 13.6 × 0.75 × 784 ≈ 8.0 keV, close to the measured value.
Key takeaways
- The continuous spectrum comes from braking electrons and ends sharply at λ_min = hc/(eV) = 1240/V nm, set by the accelerating voltage alone.
- Characteristic lines come from inner-shell vacancies and are fixed by the target; raising V does not move them.
- Kβ (M → K) has more energy and a shorter wavelength than Kα (L → K).
- Filament current changes intensity only; voltage changes λ_min; target changes the lines.
- Moseley: √ν = a(Z − b), with b ≈ 1 for Kα, so E(Kα) ≈ 10.2 (Z − 1)² eV and wavelengths scale as 1/(Z − 1)².
Practice questions (8)
Attempt each one before opening the answer. Every explanation names the tempting wrong option as well as the right one, because that is where marks are lost.
The cut-off (minimum) wavelength of the continuous X-ray spectrum from a Coolidge tube depends on:
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Answer: B — The accelerating voltage only
The shortest-wavelength photon takes an electron's entire kinetic energy eV, so λ_min = hc/(eV) depends only on the accelerating voltage. The target decides the characteristic lines, and the filament current decides how many electrons arrive, hence the intensity — neither moves the cut-off.Electrons accelerated through 20 kV strike a target. Taking hc = 1240 eV nm, the cut-off wavelength of the X-rays produced is:
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Answer: A — 62 pm
λ_min = 1240/20 000 nm = 0.062 nm = 62 pm. The other options are the same digits with the power of ten slipped — 62 nm would be ultraviolet, far too long for 20 keV photons, which is a useful sense-check.The accelerating voltage of an X-ray tube is doubled while the target is unchanged. Then:
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Answer: C — λ_min halves and the Kα wavelength is unchanged
λ_min ∝ 1/V, so doubling V halves it. The Kα line is an energy difference inside the target atom and does not depend on how hard the atom was struck, so its wavelength stays put. Halving both treats the characteristic line as if it were the spectrum's edge.According to Moseley's law, a straight line is obtained when one plots, against atomic number Z:
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Answer: C — The square root of the Kα frequency, √ν
Moseley's law is √ν = a(Z − b), linear in Z for the square root of the frequency. ν itself grows as (Z − 1)², a parabola, and λ falls as 1/(Z − 1)². Plotting ν against Z is the usual slip.Using Moseley's law with screening constant 1 for the Kα line, the ratio of the Kα wavelength of an element with Z = 11 to that of an element with Z = 21 is:
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Answer: A — 4
λ ∝ 1/(Z − 1)², so λ(11)/λ(21) = (21 − 1)²/(11 − 1)² = 400/100 = 4: the lighter element has the longer wavelength. 1/4 inverts the ratio, 2 forgets the square, and (21/11)² drops the screening constant.Estimating with E(Kα) ≈ 13.6 × (3/4)(Z − 1)² eV, the Kα photon energy of copper (Z = 29) is about:
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Answer: D — 8.0 keV
13.6 × 0.75 × 28² = 13.6 × 0.75 × 784 ≈ 7997 eV ≈ 8.0 keV. Using Z² = 841 gives about 8.6 keV, and dropping the 3/4 (treating the transition as from infinity to n = 1) gives about 10.7 keV.For the same target, how does the Kβ line compare with the Kα line?
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Answer: A — Kβ has higher photon energy and shorter wavelength
Kβ is an M → K transition and Kα an L → K one. The M shell lies higher than L, so the drop to K is larger: Kβ carries more energy and a shorter wavelength. L → K is Kα, so calling it the source of Kβ mixes up the two lines; Greek-letter order follows increasing energy within a series.The filament current of an X-ray tube is increased while the accelerating voltage is kept fixed. The effect on the X-ray spectrum is:
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Answer: C — The intensity increases at every wavelength, with λ_min and the lines unchanged
More filament current means more electrons per second, each with the same energy eV. So more photons are produced at every wavelength, but λ_min = hc/(eV) and the characteristic wavelengths are unchanged. Expecting λ_min to fall confuses the number of electrons with their energy, the same distinction as intensity versus frequency in the photoelectric effect.