Physics › Quantum phenomena › Energy levels and photon emission

Energy levels and photon emission

A glowing low-pressure gas does not emit a continuous spectrum. It emits a few sharp colours and almost nothing between, and that pattern of lines is direct evidence that the energy inside an atom comes in fixed rungs.

Year 12AQA 3.2.2.3CIE 22.4.1, 22.4.2, 22.4.3OCR A 5.5.2(a), 5.5.2(b), 5.5.2(c), 5.5.2(d), 5.5.2(e), 5.5.2(f)EDEXCEL 96

Builds on Collisions of electrons with atoms.

IN THIS TOPIC

  • Interpret line spectra as evidence for transitions between discrete energy levels.
  • Use hf = E1 − E2 for photon emission, with levels quoted in J or eV.
  • Explain why each element's line spectrum is unique.

COMMON MISCONCEPTION

An atom can emit any colour it likes.

The evidence: lines, not rainbows

Pass the light from a glowing gas, hydrogen in a discharge tube say, through a diffraction grating and no rainbow appears. You get a line spectrum, a handful of sharp bright colours with darkness between them.

A line spectrum: each bright line is one transition's photon energy, so the pattern fingerprints the elementbright lines on darkness, and nothing in betweendiscrete lines mean discrete gaps: the levels are quantised
FIG. 1An emission line spectrum, discrete bright lines with nothing in between. Discrete lines demand discrete energy gaps.

Each line is light of one photon energy, so the atom emits only certain exact energies. One conclusion survives that observation. The electron's possible energies inside the atom are discrete levels, and light comes out only when an electron drops from one level to another.

The transition equation

When an electron falls from a level of energy E1 to a lower level E2, the atom emits one photon carrying exactly the difference.

hf=E1-E2hf = E_{1} - E_{2}ON THE AQA DATA SHEET
A downward transition emits one photon carrying exactly the energy gap: hf equals E1 minus E2-13.6 eV-3.4 eV-1.5 eVone photon,hf = 10.2 eVthe photon's energy is the gap, exactly, every time
FIG. 2A drop from −3.4 eV to −13.6 eV emits one photon of exactly 10.2 eV. The gap sets the frequency; the frequency sets the colour.

Level diagrams quote energies as negative numbers, measured down from zero at ionisation, so a bound electron sits in an energy debt and the ground state is the deepest rung of all. The subtraction in hf = E1 − E2 handles the signs by itself and always delivers a positive photon energy. Questions quote levels in joules or in electronvolts, so the conversion habit from the last lesson stays on duty throughout.

WORKED EXAMPLE

A red line, predicted

In hydrogen an electron falls from the −1.51 eV level to the −3.40 eV level. Find the photon's frequency and wavelength, and place it in the spectrum.

The gap is the photon. ΔE = 3.40 − 1.51 = 1.89 eV = 3.02 × 10−19 J, and the subtraction has to come out positive, which is the check on getting it the right way round.

f = ΔE/h = 3.02 × 10−19/(6.63 × 10−34) = 4.6 × 1014 Hz.

λ = c/f = 660 nm, deep red, and a real line of the hydrogen spectrum. Two numbers off a level diagram have predicted the colour of a glowing gas.

Fingerprints

Every element has its own set of levels, so every element has its own set of gaps, and so every element emits its own set of lines. A spectrum identifies an element as surely as a fingerprint identifies a person. Astronomers read the composition of stars they will never touch by exactly this route, because the starlight arrives carrying the atomic barcodes of everything burning in it.

The same levels absorb as they emit, so the dark lines of an absorption spectrum sit at positions matching emission lines. The match is not a complete mirror: a cool gas absorbs mainly from the levels its electrons actually occupy, the ground state above all, so some emission lines have no absorption twin.

GUIDED PRACTICE

Counting the lines

An atom has exactly three energy levels. How many different spectral lines can it emit? Draw the level diagram in your head and count the downward arrows.

Show the working

Each pair of levels gives one possible drop. Top to middle, top to bottom, middle to bottom, so three transitions, and if the two gaps are different sizes those are three different photon energies: three lines.

Count transitions and count lines separately, because they are not always the same number. Space the three levels equally and the top-to-middle drop releases exactly what the middle-to-bottom drop releases, so those two photons land at the same wavelength: three transitions, two lines. The top-to-bottom photon carries the sum of the other two, so it can never coincide with either.

With four levels there are six transitions, because every extra level adds one for each level below it, and six distinct lines so long as no two gaps happen to match. Counting spectral lines is combinatorics with the physics already done.

INDEPENDENT PRACTICE

The cost of escape

Hydrogen's ground state sits at −13.6 eV. Find the maximum wavelength of a photon that can ionise a ground-state hydrogen atom.

Show the working

Ionisation means lifting the electron from −13.6 eV all the way to zero, so the photon must carry at least 13.6 eV, which is 2.18 × 10−18 J.

Maximum wavelength goes with minimum energy, so λ = hc/E = (6.63 × 10−34 × 3.00 × 108)/(2.18 × 10−18) = 91 nm, deep in the ultraviolet. Anything longer knocks on the door without the fare.

ASSESSMENT FOCUS

  • “Explain how line spectra provide evidence for energy levels” wants the full chain. Sharp lines mean only certain photon energies. Each photon energy equals a level difference. The levels are therefore discrete.
  • One transition makes one photon, carrying exactly the gap. Two small drops make two photons and never one photon of the combined energy.
  • Level energies are negative, and the ground state is the most negative of all. “Lowest level” means deepest in the well, not smallest in magnitude.
  • Put the levels into joules before h gets involved in hf = E1 − E2. Substituting eV straight into that equation is the commonest unit slip in this topic.
  • A bigger gap means a higher frequency, so transitions down to the ground state give the most energetic photons and often land in the ultraviolet.

CHECK YOURSELF

In hydrogen, an electron falls from the −3.4 eV level to the −13.6 eV ground state. Find the frequency of the emitted photon. (h = 6.63 × 10−34 J s.)

Show a hint

Gap first, in eV; then joules; then h.

Show the answer

Take the gap first. E1-E2E_{1} - E_{2} = (−3.4) − (−13.6) = 10.2 eV, and the signs have taken care of themselves.

Convert it. 10.2 × 1.60 × 10−19 = 1.63 × 10−18 J.

Then f=E/hf = E/h = 1.63 × 10−18 / (6.63 × 10−34) = 2.5 × 1015 Hz. That sits in the ultraviolet, as a drop to the ground state usually does.

Discrete lines mean discrete gaps.

Discrete gaps mean discrete levels.

One transition makes exactly one photon.

WORKBOOK

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Answer book

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  • Interpret line spectra as evidence for transitions between discrete energy levels.
  • Use hf = E1 − E2 for photon emission, with levels quoted in J or eV.
  • Explain why each element's line spectrum is unique.

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