Topic 3.3: Light and Atoms

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Vocabulary practice flashcards covering atomic energy levels, atomic emission and absorption spectra, continuous spectra, characteristic X-rays, and the physics of lasers and stimulated emission.

25 Terms

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Continuous Spectrum

An electromagnetic spectrum containing an unbroken range of frequencies radiated by solid, liquid, or dense gaseous objects.

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Incandescence

The process by which hot solids, liquids, or dense gases emit a continuous spectrum of electromagnetic radiation whose frequency distribution and dominant colour depend directly on temperature.

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Black Body Spectrum

The characteristic continuous spectrum of electromagnetic radiation emitted by hot, dense objects across various temperatures.

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Line Emission Spectrum

A spectrum consisting of thin, discrete coloured lines on a dark background, produced when atoms of a pure heated gas or gas connected to a high potential difference emit specific discrete frequencies of light.

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Line Absorption Spectrum

A spectrum consisting of discrete dark lines superimposed on a continuous spectrum, produced when light passes through a cooler gas and specific frequencies are absorbed by atomic electrons.

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Spectral Lines

Specific discrete lines present on an emission or absorption spectrum, each representing a unique wavelength characteristic of the chemical element or compound emitting or absorbing it.

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Ground State

The lowest energy state of an atom (n=1n = 1), representing the state where its electrons possess the minimum possible internal energy.

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Excited State

Any energy state higher than the ground state (n>1n > 1) to which an electron can be promoted when the atom absorbs energy.

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Collisional Excitation

The process by which an electron in an atom is raised from a lower energy state to a higher energy state by absorbing energy from a collision with an incoming particle, such as an accelerated electron.

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<p>Characteristic X-Rays</p>

Characteristic X-Rays

High-intensity discrete peaks in an X-ray spectrum produced when incident high-speed electrons eject inner-shell electrons from target atoms, causing outer-shell electrons to drop down and emit photons with energies equal to the transition gap.

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Ionisation Energy

The minimum amount of energy required to completely remove a valence electron from an atom in its ground state (n=1n = 1).

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Balmer Series

The spectral series of four visible emission lines in hydrogen produced when excited electrons transition from higher energy states down to the n=2n = 2 energy level.

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Lyman Series

The spectral series of emission lines in hydrogen located in the ultraviolet region, produced when excited electrons drop down to the n=1n = 1 ground state.

<p>The spectral series of emission lines in hydrogen located in the ultraviolet region, produced when excited electrons drop down to the $$n = 1$$ ground state.</p>
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Paschen Series

The spectral series of emission lines in hydrogen located in the infrared region, produced when electrons transition from higher energy levels down to the n=3n = 3 level.

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Rydberg Constant (RR)

A fundamental physical constant used in Balmer's empirical formula to calculate the wavelengths of hydrogen spectral transitions, with a value of 1.097ร—107โ€‰mโˆ’11.097 \times 10^7\,\text{m}^{-1}.

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Fraunhofer Lines

The dark absorption lines observed in the Sun's continuous spectrum, caused by the selective absorption of light by cooler elemental gases in the solar atmosphere.

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Fluorescence

The process in which an atom absorbs a high-energy photon to enter an excited state, and then spontaneously transitions back to the ground state via intermediate steps, emitting two or more lower-energy (longer wavelength) photons.

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Spontaneous Emission

The random transition of an electron from an excited state to a lower energy state without external influence, typically occurring after an average lifetime of about 10โˆ’8โ€‰s10^{-8}\,\text{s} and emitting a photon in an arbitrary direction.

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<p>Stimulated Emission</p>

Stimulated Emission

The process where an incident photon of energy ฮ”E=hฮฝ\Delta E = h\nu triggers an excited electron to drop to a lower energy state, releasing a second photon identical in energy, direction, and phase to the incoming photon.

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<p>Population Inversion</p>

Population Inversion

A non-equilibrium condition required for laser operation in which a greater number of atoms occupy a higher energy (metastable) state than a lower energy state.

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Metastable State

An excited atomic state with an unusually long lifetime (approximately 10โˆ’3โ€‰s10^{-3}\,\text{s} compared to the standard 10โˆ’8โ€‰s10^{-8}\,\text{s}), allowing sufficient accumulation of excited atoms to establish a population inversion.

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Laser (Light Amplification by Stimulated Emission of Radiation)

A device that generates a narrow, intense, monochromatic, and coherent beam of light via stimulated emission within an optical resonant cavity.

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<p>Gain Medium</p>

Gain Medium

The active substance in a laser containing atoms or molecules that undergo stimulated emission to amplify light.

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Pump (Laser)

The external energy source (such as an electrical potential difference) that provides the energy required to excite atoms in the gain medium and maintain a population inversion.

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Coherence

A property of laser light in which all emitted photons maintain a constant phase relationship relative to one another over large distances, enabling the beam to remain highly focused and uni-directional.