38.5.1 Energy-Level Diagrams

An energy-level diagram, such as the one shown in FIGURE 38.15 , is a useful pictorial representation of the stationary-state energies. An energy-level diagram is less a graph than it is a picture. The vertical axis represents energy, but the horizontal axis is not a scale. Think of this as a picture of a ladder in which the energies are the rungs of the ladder. The lowest rung, with energy E1, is the ground state. Higher rungs are labeled by their quantum numbers, n=2, 3, 4,….

FIGURE 38.15 An energy-level diagram.

The figure illustrates an energy level diagram.
FIGURE 38.15 Full Alternative Text

Energy-level diagrams are especially useful for showing transitions, or quantum jumps, in which a photon of light is emitted or absorbed. As examples, Figure 38.15 shows upward transitions in which a photon is absorbed by a ground-state atom (n=1) and downward transitions in which a photon is emitted from an n=4 excited state.

EXAMPLE 38.10 Emission and absorption

An atom has stationary states E1=0.00 eV, E2=3.00 eV, and E3=5.00 eV. What wavelengths are observed in the absorption spectrum and in the emission spectrum of this atom?

MODEL Photons are emitted when an atom undergoes a transition from a higher energy level to a lower energy level. Photons are absorbed in a transition from a lower energy level to a higher energy level. But most of the atoms are in the n=1 ground state, so the only transitions seen in the absorption spectrum start from the n=1 state.

VISUALIZE FIGURE 38.16 shows an energy-level diagram for the atom.

FIGURE 38.16 The atom’s energy-level diagram.

The figure illustrates the energy level diagram of an atom at various states.

SOLVE This atom will absorb photons on the 1→2 and 1→3 transitions, with ΔE1→2=3.00 eV and ΔE1→3=5.00 eV. From f=ΔEatom/h and λ=c/f, we find that the wavelengths in the absorption spectrum are

1→2f=3.00 eV/h=7.25×1014 Hzλ=414 nm (blue)1→3f=5.00 eV/h=1.21 ×1015 Hzλ=248 nm (ultraviolet)

The emission spectrum will also have the 414 nm and 248 nm wavelengths due to the 2→1 and 3→1 transitions from excited states 2 and 3 to the ground state. In addition, the emission spectrum will contain the 3→2 transition with ΔE3→2=−2.00 eV that is not seen in absorption because there are too few atoms in the n=2 state to absorb. We found in Example 38.9 that a 2.00 eV transition corresponds to a wavelength of 621 nm. Thus the emission wavelengths are

2→1λ=414 nm (blue) 3→1λ=248 nm (ultraviolet)3→2λ=621 nm (orange)