Sharp peaks on a smooth hump
The spectrum of a molybdenum tube at \(30\,\text{kV}\) has two sharp peaks on its smooth hump. One is at \(0.063\,\text{nm}\) and a taller one at \(0.071\,\text{nm}\). Braking cannot explain them, because braking favours no particular energy. Something inside the molybdenum atom picks out these two energies. They are called characteristic X-rays, because they are characteristic of the target.
The electrons of an atom are arranged in shells. The shell with \(n = 1\) is called the K shell, \(n = 2\) the L shell and \(n = 3\) the M shell. In a heavy atom every inner shell is full. The K shell holds two electrons, deep down near the nucleus.
How deep the K shell is
In hydrogen, the electron on \(n = 1\) is bound by \(13.6\,\text{eV}\). In a heavy atom a K electron is bound far more tightly. It lies inside all the other electrons, so it feels nearly the whole nuclear charge \(Ze\). The Bohr energy grows as \(Z^2\). For molybdenum, \(Z = 42\), a rough estimate is \(13.6 \times 41^2 \approx 22.9\,\text{keV}\).
The measured value for molybdenum is \(20.0\,\text{keV}\), so the rough estimate is close. This binding energy of a K electron is called the K edge. The L and M shells are held much less tightly, \(2.5\) and \(0.2\,\text{keV}\) in molybdenum. On an energy ladder, the K shell sits far below the other two.
An electron from the filament can knock a K electron clean out of the atom. For this, it must bring at least the K edge, \(20.0\,\text{keV}\) for molybdenum. The atom is left with a vacancy in its K shell. A vacancy so deep does not last. Within a tiny fraction of a second, an electron from a higher shell falls into it.
When an electron falls from a higher shell into a vacancy in a lower shell, the atom gives out one photon. Its energy is the difference between the energies of the two shells: \(h\nu = E_{\text{upper}} - E_{\text{lower}}\).
Three lines and their names
The lines are named by the shell that holds the vacancy. A fall into the K shell gives a K line, and a fall into the L shell an L line. The Greek letter says where the electron came from. The letter α means from the next shell up, and β from two shells up.
A molybdenum atom has a vacancy in its K shell. It can be filled by an L electron, giving the Kα line, or by an M electron, giving the Kβ line. Which photon has the shorter wavelength?
Play each chip of the figure above. For Kα an L electron falls into the K vacancy. The photon carries \(20.0 - 2.5 = 17.5\,\text{keV}\), and its wavelength is \(1240/17500 = 0.071\,\text{nm}\). For Kβ an M electron falls in. The photon carries \(20.0 - 0.2 = 19.8\,\text{keV}\), and \(\lambda = 0.063\,\text{nm}\).
The Lα chip starts with a vacancy in the L shell. An M electron falls into it, and the photon carries only \(2.5 - 0.2 = 2.3\,\text{keV}\). Its wavelength is \(0.54\,\text{nm}\), almost eight times that of Kα. L lines are always far softer than K lines, because the L and M shells lie close together near the top of the ladder.
The K, L and M shells of a target atom have energies \(-20.0\), \(-2.6\) and \(-0.5\,\text{keV}\). Find the energy and wavelength of its Kα, Kβ and Lα photons.
Each photon's energy is the difference between two shell energies. The wavelength is \(\lambda = 1.24/E\) nm, with \(E\) in keV.
Kα: \(20.0 - 2.6\). Kβ: \(20.0 - 0.5\). Lα: \(2.6 - 0.5\).
Kα \(17.4\,\text{keV}\), \(\lambda = 0.0713\,\text{nm}\). Kβ \(19.5\,\text{keV}\), \(\lambda = 0.0636\,\text{nm}\). Lα \(2.1\,\text{keV}\), \(\lambda = 0.590\,\text{nm}\).
Kβ is the most energetic and the shortest; Lα the least energetic and the longest. In ångströms the three are \(0.71\), \(0.64\) and \(5.9\,\text{Å}\). Values used: \(hc = 1240\,\text{eV nm}\).
In copper the K shell is bound by \(8.98\,\text{keV}\) and the L shell by \(0.93\,\text{keV}\). Find the wavelength of copper's Kα line, in nm.
Why is the Lα line of an element so much longer in wavelength than its Kα line?
Think of the inner shells as a deep well with a short ladder at the top. The K shell is at the bottom of the well. The L and M shells are two rungs close together near the top. Any fall to the bottom is long, so the K lines are hard and close together. A step between the top rungs is short, so the L lines are soft.
The Kα peak is always taller than the Kβ peak. After a K vacancy forms, an L electron is far more likely to fill it than an M electron. In molybdenum, Kβ is only about a fifth as strong as Kα.
When the peaks appear
The peaks need K vacancies, and a K vacancy needs an incoming electron with at least the K edge. So the K lines of molybdenum appear only when \(eV\) exceeds \(20.0\,\text{keV}\), that is, above \(20.0\,\text{kV}\). They all appear together. At \(18\,\text{kV}\) the tube gives no Kα, even though a Kα photon carries only \(17.5\,\text{keV}\).
Once the peaks appear, a higher voltage makes them taller, as the figure above shows. More electrons now have enough energy to make K vacancies. But the peaks never move. Their wavelengths are fixed by the shell energies of the target atom, and the tube voltage cannot change those. Only a different target moves them.
A molybdenum tube (K edge \(20.0\,\text{keV}\)) runs first at \(40\,\text{kV}\), then at \(15\,\text{kV}\). Find the cut-off wavelength at each voltage. At which voltage does the Kα line at \(0.071\,\text{nm}\) appear?
(a) At \(40\,\text{kV}\): \(\lambda_{min} = 1240/40000 = 0.031\,\text{nm}\). At \(15\,\text{kV}\): \(\lambda_{min} = 1240/15000 = 0.083\,\text{nm}\).
(b) At \(40\,\text{kV}\) the electrons carry \(40\,\text{keV}\), more than the K edge, so they make K vacancies and Kα appears.
(c) At \(15\,\text{kV}\) no electron can make a K vacancy, so there is no Kα. Its continuum starts at \(0.083\,\text{nm}\), longer than \(0.071\,\text{nm}\) anyway.
Values used: \(hc = 1240\,\text{eV nm}\), K edge of molybdenum \(20.0\,\text{keV}\).
A molybdenum tube (K edge \(20.0\,\text{keV}\), Kα \(17.5\,\text{keV}\)) runs at \(18\,\text{kV}\). Does its spectrum show the Kα line?
The molybdenum target of a tube is replaced by copper. The voltage and current stay the same. Which statements are true?
The K edge shows up in absorption too. A metal foil absorbs X-rays weakly just below its K edge, and strongly just above it, where the photons can knock out K electrons.
Mammography, the X-ray examination of the breast, needs soft X-rays that tell one soft tissue from another. Many mammography tubes have a molybdenum target run at about \(28\,\text{kV}\). Most of their useful X-rays are the Kα and Kβ lines of molybdenum, near \(17.5\) and \(19.8\,\text{keV}\). A thin molybdenum filter removes much of the rest, so the beam is nearly one colour of X-ray.
From 1906 Charles Barkla sent X-rays onto different elements and studied the X-rays they gave out in turn. Each element sent out its own kind, one harder group and one softer group. In 1911 he called them the K and L radiations. He started in the middle of the alphabet, in case harder or softer groups turned up later. None harder than K has ever been found. Barkla received the Nobel Prize in Physics in 1917.
- Thinking Kα has the shorter wavelength because α comes first.α is the smaller fall, L to K. The larger fall, M to K, is Kβ, so Kβ is shorter.
- Taking the Kα energy as the least voltage for the K lines.The line needs a K vacancy first, which needs the K edge. For molybdenum that is \(20.0\,\text{kV}\), not \(17.5\,\text{kV}\).
- Expecting the peaks to move when the voltage changes.The peaks are fixed by the target's shells. The voltage makes them taller or makes them vanish, never moves them.
- Using negative shell energies with the wrong sign.The photon energy is always positive: the binding energy of the lower shell minus that of the upper shell.