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9702 · 22.4

Energy levels in atoms and line spectra flashcards

Revision flashcards for Cambridge 9702 Energy levels in atoms and line spectra (syllabus 22.4). Flip, recall, then mark a real past-paper question.

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    What does 'quantisation of energy levels' mean?

    Electrons in an atom can only occupy specific, discrete energy values, not any value in between.

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    Define the 'ground state' of an electron.

    The lowest and most stable energy level an electron can occupy within an atom.

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    How does an electron become 'excited'?

    It absorbs a photon (or gains energy from a collision) whose energy is sufficient to move it to a higher, unoccupied energy level.

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    What happens when an excited electron 'de-excites'?

    It transitions to a lower, more stable energy level, emitting a photon with energy precisely equal to the energy difference between the two levels.

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    State the formula for photon energy during an electron transition.

    $E_{photon} = hf = E_{initial} - E_{final}$ (where $E_{initial} > E_{final}$ for emission).

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    What is Planck's constant ($h$)?

    A fundamental constant linking the energy of a photon to its frequency: $h = 6.63 \times 10^{-34} \text{ Js}$.

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    What is an electronvolt (eV) and its conversion to Joules?

    An electronvolt is the kinetic energy gained by an electron accelerated through a potential difference of 1 volt. $1 \text{ eV} = 1.60 \times 10^{-19} \text{ J}$.

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    Describe an emission spectrum.

    A spectrum showing discrete bright lines against a dark background, formed by photons emitted during electron de-excitation in excited atoms.

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    Describe an absorption spectrum.

    A spectrum showing dark lines at specific wavelengths against a continuous background, formed when atoms absorb photons, causing electrons to excite.

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    Why is a line spectrum considered an atomic 'fingerprint'?

    Each element has a unique set of discrete energy levels, leading to a distinct pattern of photon energies that can be absorbed or emitted, identifying the element.

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    Why are energy levels in an atom represented by negative values?

    They represent the energy required to remove an electron from the atom (ionisation). The zero energy level corresponds to a free electron (at infinity), so bound electrons have negative potential energy relative to this state.

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    What is a de-excitation cascade?

    When an excited electron returns to a lower state via a series of intermediate energy levels, emitting multiple photons of different energies, rather than in a single jump.

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    What are the two main mechanisms for atomic excitation?

    1. Photon absorption, which requires a photon with energy exactly matching an energy level difference. 2. Collisional excitation, where a particle transfers at least the required excitation energy to an atomic electron.

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    What is the relationship between the speed of light (c), frequency (f), and wavelength (λ)?

    The wave equation: $c = fλ$. This is used to convert between a photon's frequency and wavelength.

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    How is a continuous spectrum produced?

    By a hot, dense object (solid, liquid, or high-pressure gas) that emits radiation at all wavelengths due to strong interactions between atoms.

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    What is the key difference in the conditions required for photon absorption vs. collisional excitation?

    Photon absorption requires the photon's energy to be *exactly* equal to the energy gap. Collisional excitation only requires the colliding particle's kinetic energy to be *at least* the energy gap.