OCR · A-Level · Physics
Course version: H556 · Version from Sept 2015
(d) the equations ΔE = hf and ΔE = hc/λ
Full specification wording
Electromagnetic radiation from stars: (d) the equations ΔE = hf and ΔE = hc/λ
These two equations convert between the energy gap of a transition and the electromagnetic radiation produced or absorbed. ΔE = hf gives the photon energy from its frequency, where h is the Planck…
Checked against the OCR H556 specification (opens in a new tab) on .
- Point 4 of 11
- 4 key terms
Study notes
From the checked teaching notes for this specification point.
The idea
These two equations convert between the energy gap of a transition and the electromagnetic radiation produced or absorbed. ΔE = hf gives the photon energy from its frequency, where h is the Planck constant, about 6.63 × 10⁻³⁴ J s. Because for light in a vacuum c = fλ, substituting f = c/λ gives ΔE = hc/λ, which is useful when a wavelength is known.
For example: A photon of wavelength 656 nm has energy hc/λ = (6.63 × 10⁻³⁴ × 3.00 × 10⁸) ÷ (656 × 10⁻⁹), which is about 3.03 × 10⁻¹⁹ J. Convert nanometres to metres before substituting, and remember that ΔE is the difference between two energy levels, so it is positive for an emitted photon.
What earns the marks
- States ΔE = hf, identifying ΔE as the photon energy and f as its frequency.
- States ΔE = hc/λ, identifying λ as the wavelength in metres and c as the speed of light in a vacuum.
- Uses c = fλ to show how the two forms are equivalent.
- Substitutes values with consistent SI units, converting nm to m by multiplying by 10⁻⁹.
- Calculates photon energy accurately, for example about 3.03 × 10⁻¹⁹ J for 656 nm.
- Relates the calculated ΔE to the difference between two discrete energy levels.
Common mistakes and how to put them right
Substituting a wavelength in nanometres directly into hc/λ.
Put it right: Convert to metres first, since 656 nm is 656 × 10⁻⁹ m.
Using the frequency of the light as the frequency of the electron or vice versa.
Put it right: f in ΔE = hf is the photon frequency.
Treating ΔE as always the full ionisation energy.
Put it right: ΔE is the difference between the two levels involved in that particular transition.
Mixing up h and c values or their powers of ten.
Put it right: Write both constants with units before substituting to catch slips.
Exam tips
- Write the equation, then substitute numbers with units, then evaluate, so unit conversions are visible to the examiner.
- If the answer is needed in eV, divide the joule value by 1.60 × 10⁻¹⁹ J eV⁻¹.
- Check the order of magnitude: visible photons have energies of a few times 10⁻¹⁹ J, so a wildly different value signals a conversion error.
Try the lesson
The start of the Electromagnetic radiation from stars: (d) the equations ΔE = hf and ΔE = hc/λ lesson, made from checked teaching notes for this specification point.
Listen
These two equations convert between the energy gap of a transition and the electromagnetic radiation produced or absorbed. ΔE = hf gives the photon energy from its frequency, where h is the Planck constant, about 6.63 × 10⁻³⁴ J s. Because for light in a vacuum c = fλ, substituting f = c/λ gives ΔE = hc/λ, which is useful when a wavelength is known. For example, a photon of wavelength 656 nm has energy hc/λ = (6.63 × 10⁻³⁴ × 3.00 × 10⁸) ÷ (656 × 10⁻⁹), which is about 3.03 × 10⁻¹⁹ J. Convert nanometres to metres before substituting, and remember that ΔE is the difference between two energy levels, so it is positive for an emitted photon. A strong answer earns marks for these points. States ΔE = hf, identifying ΔE as the photon energy and f as its frequency. States ΔE = hc/λ, identifying λ as the wavelength in metres and c as the speed of light in a vacuum. Uses c = fλ to show how the two forms are equivalent. Substitutes values with consistent SI units, converting nm to m by multiplying by 10⁻⁹. Exam tip: Write the equation, then substitute numbers with units, then evaluate, so unit conversions are visible to the examiner.
See it
Key words
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Photon energy and the Planck constant
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Wave-particle relationship for electromagnetic radiation
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Unit conversion in spectroscopy calculations
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Energy conservation in atomic transitions
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See every definition
- Photon energy and the Planck constant
- ΔE = hf gives the photon energy from its frequency, where h is the Planck constant, about 6.63 × 10⁻³⁴ J s.
- Wave-particle relationship for electromagnetic radiation
- Because for light in a vacuum c = fλ, substituting f = c/λ gives ΔE = hc/λ, which is useful when a wavelength is known.
- Unit conversion in spectroscopy calculations
- Convert nanometres to metres before substituting, multiplying by 10⁻⁹.
- Energy conservation in atomic transitions
- ΔE is the difference between two energy levels, so it is positive for an emitted photon.
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