Chapter 4: Atoms and Light

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Comprehensive practice flashcards reviewing atomic structure, wave-particle duality, quantum numbers, orbital shapes, spectroscopy, and atmospheric photochemistry from Chapter 4.

75 Terms

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Dalton's Atomic Theory (First Postulate)

The foundational postulate stating that elements are composed of extremely small, indivisible particles called atoms.

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Dalton's Atomic Theory (Second Postulate)

The principle stating that all atoms of a given element are identical in size, mass, and chemical properties, while atoms of different elements have different properties.

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Dalton's Atomic Theory (Third Postulate)

The principle stating that chemical compounds are composed of atoms of more than one element combined in simple integer or fractional ratios.

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Dalton's Atomic Theory (Fourth Postulate)

The principle stating that chemical reactions involve only the separation, combination, or rearrangement of atoms, without resulting in their creation or destruction.

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<p>Law of Multiple Proportions (Carbon Oxides)</p>

Law of Multiple Proportions (Carbon Oxides)

The demonstration of Dalton's atomic theory showing that the ratio of oxygen atoms combined with one carbon atom in carbon monoxide (CO\text{CO}) compared to carbon dioxide (CO2\text{CO}_2) is exactly 1:21:2.

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<p>Dalton's Model of Compound Formation</p>

Dalton's Model of Compound Formation

A visual representation showing that discrete, individual atoms of element XX combine with atoms of element YY in a fixed integer ratio (2:12:1) to form molecules of a distinct compound.

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<p>Cathode-Ray Tube Experiment</p>

Cathode-Ray Tube Experiment

An experimental apparatus where a high voltage accelerates a beam of electrons from a cathode past an anode toward a fluorescent screen, deflected by applied electric and magnetic fields.

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J.J. Thomson's Discovery (1906 Nobel Prize)

The experimental determination of the mass-to-charge ratio (m/em/e) of the electron using deflected beams in cathode-ray tube experiments.

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<p>Thomson's Plum Pudding Model</p>

Thomson's Plum Pudding Model

An early atomic model proposing that an atom consists of a uniform spherical cloud of positive electric charge with negatively charged electrons embedded throughout.

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<p>Rutherford's Gold Foil Experiment</p>

Rutherford's Gold Foil Experiment

An experiment bombarding a thin gold foil with α\alpha-particles, proving through large-angle deflections that an atom's positive charge is concentrated in a tiny central nucleus.

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Proton

A subatomic particle residing in the nucleus possessing a positive (++) charge equal in magnitude to an electron's charge and a mass approximately 18401840 times that of an electron.

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<p>Nuclear vs. Atomic Dimensions</p>

Nuclear vs. Atomic Dimensions

The relative dimensional comparison demonstrating that an overall atom spans approximately 10−10 m10^{-10}\,\text{m}, whereas its central atomic nucleus spans only about 10−15 m10^{-15}\,\text{m}.

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Fundamental Characteristics of Atoms

The core properties of atoms: they possess mass, contain positive nuclei, contain electrons, occupy volume, attract one another, and combine to form molecules.

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Electromagnetic Radiation

A form of radiant energy exhibiting wave-like behavior; considered the most powerful experimental tool for investigating the internal electronic structure of atoms.

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Wavelength (λ\lambda)

The spatial distance between identical points on successive waves, such as crest-to-crest or trough-to-trough.

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Amplitude

The vertical height of a wave measured from its central axis of propagation to the peak crest or trough.

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Frequency (ν\nu)

The number of complete wave cycles that pass a given stationary point in 1 second1\,\text{second}, expressed in units of Hertz (Hz=1 s−1\text{Hz} = 1\,\text{s}^{-1}).

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<p>Wave Frequency-Wavelength Relationship</p>

Wave Frequency-Wavelength Relationship

The graphical demonstration showing that as wave frequency doubles from 4 s−14\,\text{s}^{-1} to 8 s−18\,\text{s}^{-1} and quadruples to 16 s−116\,\text{s}^{-1}, the wavelength (λ\lambda) shrinks proportionally.

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Speed of Light (cc)

The constant propagation velocity of light in a vacuum, quantified as c=2.998×108 m/sc = 2.998 \times 10^8\,\text{m/s}, relating frequency and wavelength via c=νλc = \nu\lambda.

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<p>Light Amplitude and Intensity</p>

Light Amplitude and Intensity

The principle that a brighter light has greater intensity and a larger wave amplitude than a dimmer light of identical wavelength.

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<p>Electromagnetic Spectrum</p>

Electromagnetic Spectrum

The full range of electromagnetic radiation arranged by frequency and wavelength: gamma rays, X-rays, ultraviolet, visible light (400–700 nm400\text{--}700\,\text{nm}), infrared, microwaves, radar, and radio waves.

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Heated Solids Problem

A historical physics dilemma where classical wave theory could not explain the broad distribution of wavelengths emitted by solids as temperature increases.

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Quantum

The smallest discrete quantity of electromagnetic energy that can be emitted or absorbed by matter, introduced by Max Planck in 1900.

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Planck's Constant (hh)

The fundamental physical constant of proportionality linking radiant energy to frequency, valued at h=6.626×10−34 J⋅sh = 6.626 \times 10^{-34}\,\text{J}\cdot\text{s}.

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Planck's Energy Equation

The formula E=hνE = h\nu, establishing that the energy of a quantum of radiation is directly proportional to its frequency.

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Energy-Wavelength Proportionality

The relationship expressed by E=hcλE = \frac{hc}{\lambda}, showing that the energy of a photon is inversely proportional to its wavelength.

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Photoelectric Effect

The phenomenon in which electrons are ejected from the surface of a metal when exposed to light of frequency at or above a critical threshold.

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Photon

A localized particle or packet of light energy carrying an energy of E=hνE = h\nu, proposed by Albert Einstein in 1905.

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<p>Photoelectric Effect Apparatus</p>

Photoelectric Effect Apparatus

A vacuum tube setup featuring a target metal plate, an electron detector anode, a voltage source, and a current meter to detect ejected photoelectrons.

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Work Function (WW)

The minimum binding energy required to release an electron from the surface of a given metal (W=hν0W = h\nu_0).

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Einstein's Photoelectric Equation

The conservation-of-energy equation for photoemission: hν=KE+Wh\nu = \text{KE} + W or KE=hν−W\text{KE} = h\nu - W, where KE\text{KE} is the maximum kinetic energy of the ejected electron.

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Threshold Frequency (ν0\nu_0)

The absolute minimum frequency of incident light required to eject electrons from a metal surface with zero excess kinetic energy.

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<p>Threshold Frequency Graph</p>

Threshold Frequency Graph

A linear plot of photoelectron kinetic energy versus incident radiation frequency displaying a horizontal-axis intercept at ν0\nu_0, below which no emission occurs.

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Effect of Light Intensity on Photoemission

The experimental outcome showing that increasing light intensity increases the rate (number) of ejected electrons, but does not alter their individual kinetic energies.

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<p>Electron Energy Reference Convention</p>

Electron Energy Reference Convention

The energetic definition where an unbound, stationary electron separated to infinity from a nucleus is assigned E=0E = 0, meaning bound electrons have negative energies (E<0E < 0).

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Bound Electron Energy State

An electron electrostatically confined within an atom, whose potential and total energy is strictly negative (E<0E < 0).

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Ground State

The lowest, thermodynamically most stable electronic energy level available to an atom.

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Excited State

An unstable, elevated electronic state achieved when an atom absorbs energy (such as a photon) and an electron moves to a higher energy level.

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<p>Atomic Energy Level Transitions</p>

Atomic Energy Level Transitions

A diagram illustrating the upward absorption of a photon to reach excited states and subsequent downward relaxation via photon emission or heat loss.

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Atomic Absorption Spectrum

A spectrum featuring dark absorption lines produced when continuous white light passes through a vapor sample and atoms absorb specific resonant frequencies.

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Atomic Emission Spectrum

A spectrum displaying discrete, colored bright lines against a dark background, produced by photons emitted as excited atoms drop to lower energy states.

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<p>Absorption Spectroscopy Apparatus</p>

Absorption Spectroscopy Apparatus

A configuration where white light from a lamp traverses a cold gas tube, a slit, and a dispersing prism to display absorption lines on a screen.

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<p>Hydrogen Emission Line Setup</p>

Hydrogen Emission Line Setup

A high-voltage discharge tube exciting hydrogen gas, directing emitted light through a narrow slit and prism to create four characteristic visible lines on a photographic plate.

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Balmer Equation (1885)

The mathematical formula ν=3.29×1015 s−1(122−1n2)\nu = 3.29 \times 10^{15}\,\text{s}^{-1}\left(\frac{1}{2^2} - \frac{1}{n^2}\right), which mathematically predicted the frequencies of lines in the visible hydrogen spectrum.

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<p>Bright-Line Spectra of Elements</p>

Bright-Line Spectra of Elements

A comparative collection of line emission spectra showing that each element (alkali metals, alkaline earths, and noble gases) possesses a distinct spectral signature.

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<p>Bohr Model of the Hydrogen Atom (1913)</p>

Bohr Model of the Hydrogen Atom (1913)

A model stating that electrons travel only in discrete circular orbits of quantized energy and emit light only when jumping from an outer to an inner orbit.

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Rydberg Constant for Hydrogen (RHR_H)

The fundamental constant equal to 2.18×10−18 J2.18 \times 10^{-18}\,\text{J} used in calculating energy levels and transition frequencies of single-electron systems.

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Bohr Energy Equation

The formula En=−RH(1n2)=−2.18×10−18 Jn2E_n = -R_H \left(\frac{1}{n^2}\right) = -\frac{2.18 \times 10^{-18}\,\text{J}}{n^2}, giving the exact quantized energy of an electron at principal level nn.

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<p>Staircase Analogy of Energy Quantization</p>

Staircase Analogy of Energy Quantization

A mechanical analogy comparing atomic energy levels to steps on a staircase: an electron or ball can rest on discrete steps (1,2,31, 2, 3) but cannot exist between them.

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<p>Hydrogen Emission Transitions Diagram</p>

Hydrogen Emission Transitions Diagram

A transition scheme illustrating Lyman transitions to n=1n=1 (ultraviolet), Balmer transitions to n=2n=2 (656656, 486486, 434434, and 410 nm410\,\text{nm}), and Paschen transitions to n=3n=3 (infrared).

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De Broglie Hypothesis

The postulate stating that matter in motion exhibits wave properties, meaning that all moving particles have an associated wavelength.

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De Broglie Wavelength Equation

The relationship λ=hmv\lambda = \frac{h}{mv}, which computes the wavelength (λ\lambda) of a particle from Planck's constant, mass (mm), and velocity (vv).

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<p>Photon and Electron Property Equations</p>

Photon and Electron Property Equations

A reference table comparing photon mechanics (E=hνE = h\nu, λ=hcE\lambda = \frac{hc}{E}, c=3×108 m/sc = 3 \times 10^8\,\text{m/s}) with electron mechanics (Ek=12mv2E_k = \frac{1}{2}mv^2, λ=hmv\lambda = \frac{h}{mv}, v=2Ekmv = \sqrt{\frac{2E_k}{m}}).

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Heisenberg Uncertainty Principle

The physical principle establishing that the more precisely the position of a subatomic particle is known, the less precisely its momentum can be known, and vice versa.

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Mathematical Formulation of Uncertainty

The inequality Δx⋅Δp≥h4π\Delta x \cdot \Delta p \ge \frac{h}{4\pi}, which defines the fundamental quantum limitation on simultaneous measurements of position and momentum.

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Schrödinger Wave Equation

A fundamental differential wave equation developed by Erwin Schrödinger to mathematically describe the wave behavior of electrons in atoms.

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Wave Function (ψ\psi)

A mathematical solution to the Schrödinger equation that completely specifies the spatial amplitude and phase of an electron matter wave inside an atom.

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<p>Max Born Orbital Probability Interpretation</p>

Max Born Orbital Probability Interpretation

The proposal that the square of the wave function (ψ2\psi^2) represents probability density, analogous to the distribution of perfume mist droplets on a target surface.

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Atomic Orbital

A three-dimensional region of space surrounding a nucleus within which there is a high probability of finding an electron.

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Pauli Exclusion Principle

The quantum rule dictating that no two electrons in an atom can have identical values for all four quantum numbers (nn, ll, mlm_l, msm_s).

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Principal Quantum Number (nn)

A positive integer (n=1,2,3,…n = 1, 2, 3, \dots) defining the relative size and principal energy level of an atomic orbital.

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Azimuthal Quantum Number (ll)

An integer ranging from 00 to n−1n-1 that designates the geometric shape of an orbital (l=0,1,2,3l = 0, 1, 2, 3 corresponding to s,p,d,fs, p, d, f).

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Magnetic Quantum Number (mlm_l)

An integer taking values from −l-l to +l+l that specifies the three-dimensional orientation of an orbital in space.

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Spin Quantum Number (msm_s)

A quantum parameter describing the intrinsic spin orientation of an electron, restricted to either +12+\frac{1}{2} or −12-\frac{1}{2}.

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<p>Orbital Quantum Numbers (First Four Shells)</p>

Orbital Quantum Numbers (First Four Shells)

A structured table displaying permitted values of nn, ll, and mlm_l, illustrating that total orbitals per shell equal n2n^2 (1,4,9,161, 4, 9, 16).

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Electron Shell, Subshell, and Orbital Hierarchy

The organizational hierarchy of electrons: shells group states with identical nn; subshells group identical nn and ll; orbitals group identical nn, ll, and mlm_l.

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<p>s Orbitals and Radial Distribution</p>

s Orbitals and Radial Distribution

Spherically symmetrical orbitals (l=0l=0) whose radial electron probability density curves (4πr2ψ24\pi r^2\psi^2) exhibit spherical nodes and expand outward as nn increases from 1s1s to 3s3s.

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<p>p Orbitals</p>

p Orbitals

Three dumbbell-shaped atomic orbitals (l=1l=1) oriented along orthogonal cartesian axes, designated pxp_x, pyp_y, and pzp_z (ml=−1,0,+1m_l = -1, 0, +1).

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<p>d Orbitals</p>

d Orbitals

Five atomic orbitals (l=2l=2) consisting of four cloverleaf shapes (dxy,dyz,dxz,dx2−y2d_{xy}, d_{yz}, d_{xz}, d_{x^2-y^2}) and one dumbbell with a central torus (dz2d_{z^2}).

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<p>f Orbitals</p>

f Orbitals

Seven complex multi-lobed atomic orbitals (l=3l=3) with magnetic quantum numbers ml=−3,−2,−1,0,+1,+2,+3m_l = -3, -2, -1, 0, +1, +2, +3.

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Maximum Subshell Electron Capacity

The maximum number of electrons accommodated per subshell: ss holds 22, pp holds 66, dd holds 1010, and ff holds 1414.

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<p>Periodic Table Orbital Blocks</p>

Periodic Table Orbital Blocks

The organization of the periodic table reflecting subshell filling into ss-block (Groups 1-2, He), pp-block (Groups 13-18), dd-block (transition metals), and ff-block (lanthanides/actinides).

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<p>Earth's Atmospheric Layers</p>

Earth's Atmospheric Layers

The atmospheric stratification characterized by altitude and pressure: Troposphere (0–10 km0\text{--}10\,\text{km}), Stratosphere (10–50 km10\text{--}50\,\text{km}), Mesosphere (50–85 km50\text{--}85\,\text{km}), and Thermosphere (>85 km>85\,\text{km}).

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Thermospheric Reactions

Photochemical reactions above 85 km85\,\text{km} where N2N_2 and O2O_2 absorb solar X-rays to produce ionized and dissociated species (N2+hν→N2++e−N_2 + h\nu \rightarrow N_2^+ + e^-, O2+hν→O+OO_2 + h\nu \rightarrow O + O), shielding lower layers.

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<p>Greenhouse Effect Mechanism</p>

Greenhouse Effect Mechanism

The process where tropospheric gases (CO2\text{CO}_2, H2O\text{H}_2\text{O}, CH4\text{CH}_4) transmit incoming visible sunlight but absorb and re-emit outgoing infrared radiation emitted by Earth.