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

    A flowchart running from top to bottom. The first box reads 'Energy gap between two levels, ΔE' and points to a box reading 'ΔE = hf', which points to 'Photon frequency f'. A separate box 'c = fλ' points to 'Substitute f = c/λ', and the 'ΔE = hf' box also points to 'Substitute f = c/λ'. That box points to 'ΔE = hc/λ', which points to 'Wavelength λ in metres', then to 'Convert nm to m: multiply by 10⁻⁹', then to 'Substitute h, c and λ', and finally to 'Photon energy ΔE'.
    Shows how ΔE = hf and ΔE = hc/λ are linked through c = fλ, and the steps to calculate photon energy from a wavelength.

    Key words

    Say what each word means before you turn the card.

    Photon energy and the Planck constant

    Try answering aloud or in your head before turning the card.

    Wave-particle relationship for electromagnetic radiation

    Try answering aloud or in your head before turning the card.

    Unit conversion in spectroscopy calculations

    Try answering aloud or in your head before turning the card.

    Energy conservation in atomic transitions

    Try answering aloud or in your head before turning the card.

    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.

    Label the diagram

    Some boxes have lost their names. Pick the right name for each number.

    The diagram again, with 3 boxes numbered instead of named. A flowchart running from top to bottom. The first box reads 'Energy gap between two levels, ΔE' and points to a box reading 'ΔE = hf', which points to 'Photon frequency f'. A separate box 'c = fλ' points to 'Substitute f = c/λ', and the 'ΔE = hf' box also points to 'Substitute f = c/λ'. That box points to 'ΔE = hc/λ', which points to 'Wavelength λ in metres', then to 'Convert nm to m: multiply by 10⁻⁹', then to 'Substitute h, c and λ', and finally to 'Photon energy ΔE'.
    • 1Box 1

    • 2Box 2

    • 3Box 3

    0 of 3 labelled

    There is more to this lesson

    The full lesson goes on to check your understanding and help you earn the marks. Create a free account to carry on, with your progress saved.

    Carry on with the full lesson

    A week of Premium from your first lesson · Then the free plan continues · No card, no charge

    Test your understanding of Electromagnetic radiation from stars: (d) the equations ΔE = hf and ΔE = hc/λ

    Active recall beats re-reading. Take an instant quiz now to test what you’ve learned and lock it into long-term memory.

    Take topic quiz

    A week of Premium from your first lesson · Then the free plan continues · No card, no charge