Quantum Model, Electron Configurations, Light, Spectroscopy, Coffee Lab, and PES

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Vocabulary practice flashcards covering quantum mechanics, atomic structure, electron configurations, light principles, spectroscopic techniques, standard curves, and photoelectron spectroscopy.

Last updated 7:50 PM on 9/13/26
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37 Terms

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Bohr Model

An atomic model that places electrons in defined circular orbits with specific quantized energies around the nucleus.

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Quantum Mechanical Model

An atomic model that describes regions of high probability for finding an electron, known as orbitals, rather than exact physical paths.

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Blackbody Radiation

A physical phenomenon demonstrating that energy is emitted in discrete amounts rather than any arbitrary continuous amount.

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Photoelectric Effect

The ejection of electrons from a material when light with a frequency above a specific threshold strikes it.

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Atomic Emission Spectra

Characteristic patterns of specific light wavelengths emitted by atoms, revealing discrete electron energy states.

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Orbital

A region of space where there is a high probability of finding an electron, holding a maximum of two electrons with opposite spins.

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Sublevel

A group of equal-energy orbitals of the same type (ss, pp, dd, or ff) within a principal energy level.

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Principal Energy Level

A major electron energy shell represented by the principal quantum number n=1,2,3...n = 1, 2, 3\text{...}, with higher levels generally farther from the nucleus and higher in energy.

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ss Sublevel

A spherical sublevel consisting of 1 orbital that holds a maximum of 2 electrons.

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pp Sublevel

A dumbbell-shaped sublevel consisting of 3 orbitals that holds a maximum of 6 electrons.

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dd Sublevel

A complex-shaped sublevel consisting of 5 orbitals that holds a maximum of 10 electrons.

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ff Sublevel

A complex-shaped sublevel consisting of 7 orbitals that holds a maximum of 14 electrons.

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Noble-Gas Configuration

A shorthand electron configuration that replaces the inner completed electron shell with the bracketed symbol of the preceding noble gas.

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Hund's Rule

The rule stating that electrons occupy equal-energy orbitals singly with parallel spins before any orbital receives a second electron.

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Aufbau Principle

The rule stating that electrons occupy the available orbitals of lowest energy first before filling higher-energy orbitals.

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Principal Quantum Number (nn)

The quantum number that indicates the principal energy level or major electron shell (n=1,2,3...n = 1, 2, 3\text{...}).

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Angular Momentum Quantum Number (ll)

The quantum number that identifies the sublevel type, defined as s=0s=0, p=1p=1, d=2d=2, and f=3f=3.

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Magnetic Quantum Number (mlm_l)

The quantum number that designates a specific orbital within a sublevel, ranging from l-l through +l+l.

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Electron Spin Quantum Number (msm_s)

The quantum number that describes the spin orientation of an electron, taking values of +12+\frac{1}{2} or 12-\frac{1}{2}.

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Heisenberg Uncertainty Principle

The fundamental limit stating that it is impossible to simultaneously measure both the exact position and exact momentum of an electron.

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Wave-Particle Theory of Light

The model stating that light exhibits both wave characteristics (wavelength, frequency) and particle characteristics (photons).

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Amplitude

The height of a wave measured from its equilibrium position, which corresponds to the wave's intensity.

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Frequency ($ u$)

The number of wave cycles that pass a given point per second, measured in hertz (Hz\text{Hz} or s1\text{s}^{-1}).

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Wavelength ($ rac{}{} ext{lambda}$ or $ u$)

The distance between equivalent points on consecutive waves, typically expressed in meters (m\text{m}).

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Speed of Light (cc)

The physical constant representing the speed of light in a vacuum, equal to 3.00×108 m/s3.00 \times 10^8\text{ m/s}.

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Planck's Constant (hh)

The proportionality constant relating photon energy to frequency, equal to 6.626×1034 Js6.626 \times 10^{-34}\text{ J}\text{s}.

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Electromagnetic Spectrum

The full range of electromagnetic radiation ordered from longest wavelength to shortest: radio, microwave, infrared, visible, ultraviolet, X-ray, and gamma ray.

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Photon

A discrete packet or particle of electromagnetic radiation carrying energy equal to E=h×frequencyE = h \times \text{frequency}.

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Quantum

The minimum discrete amount or packet of energy that can be absorbed or emitted by an atom.

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Valence Electron

An electron located in the outermost occupied principal energy level of an atom that participates in chemical bonding.

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Octet Rule

The tendency of main-group atoms to gain, lose, or share electrons to achieve a full outer shell of 8 valence electrons.

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Continuous Spectrum

A spectrum that displays an uninterrupted continuum of all wavelengths across a given range.

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Emission Spectrum

A spectrum composed of discrete bright lines at specific wavelengths emitted when excited electrons transition to lower energy levels.

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Absorption Spectrum

A continuous spectrum containing dark lines caused by the absorption of specific light wavelengths as electrons transition to higher energy levels.

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Standard Curve

A reference graph plotting known concentrations against measured responses used to calculate unknown sample concentrations using x=ybmx = \frac{y - b}{m}.

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Photoelectron Spectroscopy (PES)

An experimental technique that utilizes the photoelectric effect to determine electron binding energies and deduce electron configurations.

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Binding Energy Peak

A peak in a photoelectron spectrum whose position indicates electron binding energy and whose area corresponds to the relative number of electrons in that sublevel.