Which lines a spectrum contains is decided by a symmetry, not by an energy. The gaps say what could be emitted; parity says what actually is.
The states of Β§9.2 are stationary β left alone, an excited hydrogen atom would stay excited forever. Real atoms emit light. This section turns the electromagnetic field on and asks which transitions can happen, then makes one small correction that turns out to have discovered an isotope.
What drives a transition
The most probable radiative transitions are electric dipole electric dipole transition The most probable radiative transition, driven by the interaction βdΒ·E with dipole operator d = βer. Its matrix element vanishes unless the two states have opposite parity, which yields the Ξl = Β±1 selection rule. defined in ch. 9 β open in glossary transitions, driven by the interaction of the field with the electronβnucleus dipole moment :
and the probability of a transition between states and is proportional to
Parity kills most of them
The argument is two lines and needs no integration.
Working through the spherical-harmonic algebra narrows the survivors further β the integral vanishes unless is or exactly:
Labelled by n = nr + l + 1, as in Table 9.1 and Fig. 9.8. Now the aligned levels share a name, and the spectroscopic labels 1s, 2s, 2p, 3d appear. Same diagram, same physics β only the bookkeeping changed, and this is the switch the book makes without announcing it. Energies come from Eq. (9.21), not from the drawing, so the alignment is the formula speaking.
Dotted lines are the allowed electric dipole transitions β every one steps sideways by exactly one column, because Ξl = Β±1. Notice what is missing: nothing connects 2s to 1s, since both have l = 0. That is why the 2s state is metastable.
The spectrum
Transitions can be induced by an external field oscillating at the resonant frequency , absorbing energy when and emitting it otherwise. Spontaneous transitions look uncaused but are not: they are driven by the quantized electromagnetic field, which is present even around a perfectly isolated atom.
Either way the emitted photon carries , giving
The reduced mass effect
One assumption has been quietly load-bearing: that the nucleus stays put. It does not β nucleus and electron both orbit their common centre of mass. Writing the classical energy in that frame turns the two-body problem into a one-body one with the reduced mass reduced mass ΞΌ = mβmβ/(mβ+mβ), the effective mass of a two-body relative motion. It turns a two-particle problem into one particle moving in the separation r; ΞΌ = m_p/2 for two protons. defined in ch. 5 β open in glossary
and the quantum problem transforms the same way. So every result so far holds with replaced by β the length scale becomes , the energy scale , and
Check yourself
0 / 6 answered
1.Why does an electric dipole transition always change the parity of the state?
In the diagram, switch off βobey Ξl = Β±1β.
2.What becomes visible, and what does it tell you about the 2s state?
3.The 2s state lives 0.14 s while 2p lives 1.6 ns. What does βforbiddenβ mean here?
4.Why does this page reuse chapter 1's hydrogen data module instead of recomputing the wavelengths?
5.Deuterium's spectral lines sit 0.18 nm from hydrogen's. Where does that come from?
6.Positronium is an electron bound to a positron. What does its reduced mass do to the spectrum?