Chapter 12 Quantum Mechanics and Atomic Theory

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Flashcards covering key vocabulary terms, quantum numbers, equations, and principles from Chapter 12: Quantum Mechanics and Atomic Theory.

Last updated 7:08 PM on 8/24/26
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32 Terms

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Wavelength (λ\lambda)

The distance between adjacent crests of a wave, expressed in meters (m\text{m}).

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Frequency (ν\nu)

The number of wave crests passing through a given point per second, measured in Hertz (Hz\text{Hz}) or s1\text{s}^{-1}.

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Speed of Light (cc)

The constant speed at which a wave crest travels in a vacuum, independent of its frequency, given by c=λνc = \lambda \nu.

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Amplitude

The maximum height of a wave measured above its center line.

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Constructive Interference

Wave interference occurring when a crest of one wave meets a crest of another wave, resulting in the addition of their amplitudes.

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Destructive Interference

Wave interference occurring when a crest of one wave meets a trough of another wave, causing the two waves to cancel each other out.

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Black-body Radiation

The electromagnetic radiation emitted by all non-reflective objects (black bodies), peaking at a characteristic frequency that shifts to shorter wavelengths with increasing temperature.

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Ultraviolet Catastrophe

The false prediction of classical electromagnetic theory that the intensity of black-body radiation would increase indefinitely with decreasing wavelength.

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Photon

A stream of quantized light particles postulated by Max Planck, each carrying energy given by Planck's equation E=hν=hcλE = h\nu = \frac{hc}{\lambda}.

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Atomic Absorption Lines

Discontinuous absorption spectra produced when matter absorbs photons matching the energy difference between its final and initial states (Ephoton=EfEiE_{photon} = E_f - E_i).

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Atomic Emission Lines

Discontinuous emission spectra produced when excited atoms emit energy as photons to relax to lower energy levels (Ephoton=EiEfE_{photon} = E_i - E_f).

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Hydrogen-like Species

The hydrogen atom and single-electron ions, such as H\text{H}, He+\text{He}^+, Li2+\text{Li}^{2+}, and Be3+\text{Be}^{3+}.

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Bohr Model

A model for hydrogen-like species in which an electron revolves around the nucleus in allowed circular orbits of specified radii determined by quantum number nn.

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Balmer Series

A set of hydrogen emission lines produced when an electron relaxes from a higher level to the n=2n = 2 level.

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Lyman Series

A set of hydrogen emission lines produced when an electron relaxes from a higher level to the n=1n = 1 level.

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Ionization Energy of Hydrogen

The energy required to absorb a photon that completely removes an electron from its ground state (n=1n = 1) to an isolated stationary state (n=n = \infty), given by E=RHE = R_H.

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De Broglie Wave-Particle Duality

The concept that material particles display wave-like properties with a wavelength inversely proportional to momentum, given by λ=hp=hmu\lambda = \frac{h}{p} = \frac{h}{m u}.

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Electron Diffraction

The creation of a wave interference diffraction pattern when electrons are scattered by a thin metal foil.

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Heisenberg's Uncertainty Principle

The fundamental limit on simultaneously measuring a particle's position (xx) and momentum (pp) with absolute precision, expressed as ΔxΔph4π\Delta x \Delta p \ge \frac{h}{4\pi}.

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Wave Function (ψ\psi)

A function obtained by solving the Schrödinger equation that describes a particle exhibiting quantum wave-like properties.

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Probability Density (ψ2\psi^2)

The value ψ2(x)\psi^2(x) representing the probability of finding a quantum particle at a specific position xx.

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Radial Node

A spherical surface on which the probability density ψ2\psi^2 is zero, occurring where the radial wave function R(r)=0R(r) = 0.

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Angular Node

A non-spherical node occurring at angles satisfying Y(θ,ϕ)=0Y(\theta, \phi) = 0.

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Principal Quantum Number (nn)

The quantum number (n=1,2,3,,n = 1, 2, 3, \dots, \infty) determining orbital size and the overall shell energy in single-electron species.

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Angular Momentum Quantum Number (ll)

The quantum number (l=0,1,2,,n1l = 0, 1, 2, \dots, n-1) defining the subshell and geometric shape of an atomic orbital.

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Magnetic Quantum Number (mlm_l)

The quantum number (ml=l,,0,,+lm_l = -l, \dots, 0, \dots, +l) designating the three-dimensional orientation of an orbital in space.

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Electron Spin Quantum Number (msm_s)

The fourth quantum number (ms=+12m_s = +\frac{1}{2} or ms=12m_s = -\frac{1}{2}) indicating an electron's intrinsic magnetic spin direction.

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Shielding Effect

The reduction in magnetic and electrostatic attraction between outer electrons and the nucleus caused by inner electrons repelling the outer electrons.

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Pauli Exclusion Principle

The quantum rule stating that no two electrons in an atom can have the exact same set of all four quantum numbers.

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Hund's Rule

The principle stating that electrons occupy degenerate orbitals singly with parallel spins before pairing up to maximize unpaired electrons.

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Aufbau Process

The hypothetical process of building up an electron configuration by progressively adding protons and electrons into available orbitals of lowest energy.

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n + l Rule

The rule stating that electronic subshells with lower n+ln + l values are filled before higher ones, and if two subshells have equal n+ln + l, the lower nn subshell fills first.