Atomic Energy Levels and Transitions
Line spectra make sense only after one idea is secure: an electron in an isolated atom can occupy only particular energies.
Electrons in isolated atoms have discrete energies
An isolated atom is considered on its own, without neighbouring atoms changing its electron energies.
An electron in an isolated atom can occupy only particular energy levels. It cannot have an energy between two allowed levels.
Definition
1 markWhat is meant by the ground state?
Model answer: The ground state is the lowest energy state of an atom.
Any allowed state above the ground state is an excited state. An atom is excited when one of its electrons has moved to a higher allowed energy level.
Some energy-level diagrams define 0 eV as a free electron at rest far from the atom. Bound states then have negative energies. A level at −2 eV is higher than a level at −5 eV because it is closer to zero.
Reaching 0 eV removes the electron from the atom. This is ionisation, not another bound energy level.
A transition transfers one energy gap
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A downward transition releases one photon. An upward transition can occur when the atom absorbs a photon whose energy exactly matches the gap. A collision can also transfer energy and excite the atom.
Symbols
- = Planck constant (J s)
- = frequency of the photon (Hz)
- = higher electron energy level (J or eV)
- = lower electron energy level (J or eV)
Key idea
A larger energy gap produces a higher-frequency photon and a shorter wavelength. A smaller gap produces a longer wavelength.
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| Transition | Energy transfer | Spectrum |
|---|---|---|
| Electron moves down | one photon is emitted with energy equal to the gap | emission line |
| Electron moves up after absorbing light | one photon with exactly the gap energy is absorbed | absorption line |
Common mistake
Two downward transitions have energy gaps of 2.0 eV and 4.0 eV. Which transition emits the shorter-wavelength photon?
Show worked answer
The 4.0 eV transition. A larger energy gap gives a higher photon frequency and therefore a shorter wavelength.
