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Wave Model of Light
Light is a type of electromagnetic radiation, a form of energy that travels through space as a wave.
Wavelength (λ)
Shortest distance between equivalent points on a continuous wave (e.g., crest to crest). Measured in meters (m), nanometers (nm), etc.
Frequency (ν)
Number of waves passing a point per second. Measured in hertz (Hz), which is equivalent to 1/s.
Amplitude
Height of a wave from the origin to the crest or trough.
Speed of Light (c)
All electromagnetic waves travel at a constant speed in a vacuum.
Wave Equation
Wavelength and frequency are inversely proportional: as one increases, the other decreases.
Electromagnetic Spectrum
Includes all forms of electromagnetic radiation (radio waves, microwaves, infrared, visible light, ultraviolet, X-rays, gamma rays).
Energy and Frequency Relationship
Energy increases with increasing frequency.
Visible Spectrum
Small portion of the spectrum visible to the human eye (red → violet).
Red Light
Long wavelength, low frequency, low energy.
Violet Light
Short wavelength, high frequency, high energy.
Quantized Energy
Max Planck proposed that matter gains/loses energy in specific amounts called quanta.
Energy of a Quantum
Energy is directly proportional to frequency.
Photoelectric Effect
Observed when light of a specific frequency ejects electrons from a metal surface.
Key Findings of Photoelectric Effect
Light below a certain frequency does not eject electrons, regardless of intensity.
Photon
Massless particle carrying a quantum of energy.
Continuous Spectrum
White light produces a full, unbroken spectrum of colors.
Atomic Emission Spectrum
Each element emits specific frequencies of light, forming a unique spectrum (individual lines of color).
Applications of Atomic Emission Spectrum
Identifying elements and analyzing star compositions.
Electromagnetic Radiation
Energy that travels as waves through space.
Planck's Constant (h)
A fundamental constant used in quantum mechanics.
Emission Spectrum
Continuous spectrum includes all wavelengths; emission spectra show only specific wavelengths unique to each element.
Quantum Energy
Matter absorbs/emits energy in whole-number multiples of .
Einstein and Quantum Theory
Used Planck's concept to explain that photons eject electrons only if their energy exceeds a threshold.
Bohr's Model
Electrons move in fixed circular orbits.
Bohr's Model
Orbits correspond to specific energy levels.
Bohr's Model
Only explains hydrogen's atomic emission spectrum accurately.
Quantum Mechanical Model
Electrons treated as waves.
Quantum Mechanical Model
Does not define exact paths (no circular orbits).
Quantum Mechanical Model
Predicts probabilities of electron locations in three-dimensional regions called atomic orbitals.
De Broglie's Wave-Particle Duality
Electrons exhibit wave-like behavior, meaning only certain wavelengths and energies are possible.
Heisenberg Uncertainty Principle
It's impossible to know both an electron's position and velocity simultaneously, leading to the idea of probability clouds instead of fixed paths.
Energy Levels
Energy levels are numbered (n = 1, 2, 3, etc.) and determine the size and energy of orbitals.
Sublevels
Each energy level has sublevels (s, p, d, f), with increasing complexity as n increases.
Atomic Orbitals
Regions where electrons are most likely to be found.
Ground State
The lowest energy state of an atom.
Quantum Number (n)
Describes the size, energy, and shape of atomic orbitals.
de Broglie Equation
Relates a particle's wavelength to its mass and velocity.
Heisenberg Uncertainty Principle
States that the position and velocity of an electron cannot be known simultaneously.
Quantum Mechanical Model
Describes electrons as wave-like entities in probabilistic regions around the nucleus.
Atomic Orbital
A 3D region around the nucleus indicating the probable location of an electron.
Principal Quantum Number
Specifies the energy level of an electron.
Principal Energy Level
Major energy levels in an atom.
Energy Sublevel
Divisions within a principal energy level (s, p, d, f).
Energy States of Hydrogen
Electrons exist in specific energy levels (orbits).
Ground State (n = 1)
The lowest energy level.
Excited State
When energy is added, electrons jump to higher orbits.
Photon Emission
Electrons drop back to lower energy levels by emitting photons, producing specific wavelengths of light.
Hydrogen's Line Spectrum
Electrons transition between energy levels.
Balmer Series
Visible light corresponds to transitions to the second energy level.
Lyman Series
Ultraviolet (drops to n = 1).
Paschen series
Infrared (drops to n = 3).
Limitations of Bohr's model
Explained hydrogen well but failed for multi-electron atoms.
Quantum Mechanical Model
Based on the wave-particle duality of electrons.
Schrödinger
Introduced the quantum mechanical model in 1926.
Electrons as waves
Electrons are treated as waves.
Atomic orbitals
Regions with a high probability of finding an electron.
Energy levels
Quantized, similar to Bohr's model.
de Broglie's Wave-Particle Duality
Proposed that electrons have wave-like properties.
Quantized energy levels
Only specific wavelengths fit within an orbital.
Heisenberg Uncertainty Principle
States that the act of observing an electron changes its position or velocity.
Key implications of the Uncertainty Principle
Impossible to determine an electron's exact location and speed simultaneously.
Schrödinger Wave Equation
Treated electrons as waves, leading to the quantum mechanical model.
Wave Functions
Mathematical solutions describe the probability of finding an electron.
High-density regions
Indicate higher probabilities (electron clouds).
Principal Quantum Number (n)
Indicates energy level and size of orbitals.
Higher n values
Mean larger orbitals and higher energy levels.
Energy Sublevels
Each principal energy level contains sublevels.
Sublevel shapes
s: Spherical, p: Dumbbell-shaped, d and f: More complex shapes.
Electrons in ground and excited states
Figure 10: Electrons in ground and excited states.
Electron transitions and photon emission
Figure 11: Electron transitions and photon emission.
Uneven spacing of hydrogen's energy levels
Figure 12: Uneven spacing of hydrogen's energy levels.
Wave properties of electrons
Figure 13: Wave properties of electrons.
Heisenberg uncertainty principle illustration
Figure 14: Illustration of the Heisenberg uncertainty principle.
Probability cloud of an electron
Figure 15: Probability cloud of an electron around the nucleus.
Essential Questions
How are the Pauli exclusion principle, the aufbau principle, and Hund's rule used to write electron configurations using orbital diagrams and electron configuration notation?
Aufbau principle
Electrons fill orbitals starting with the lowest energy levels.
Pauli exclusion principle
Each orbital can hold a maximum of two electrons with opposite spins.
Hund's rule
In degenerate orbitals (same energy level), one electron is added to each orbital before pairing begins.
Valence electrons
Electrons in the outermost energy level of an atom, responsible for chemical properties.
Electron-dot structures
A shorthand representation of valence electrons as dots around an element's symbol.
Electron configuration
Arrangement of electrons in an atom.
Aufbau Diagram
Shows the relative energy levels of orbitals.
Ground-State Electron Configuration
The most stable arrangement of electrons, where the atom is in its lowest energy state.
Energy Levels and Sublevels
Orbitals fill in order of increasing energy.
Electron Configuration Notation
Format: Principal energy level (e.g., 1, 2, 3...), Sublevel (s, p, d, f), Number of electrons in that sublevel.
Silicon
Orbital Diagram: in 1s, 2s, 2p; Electron Configuration: .
Fluorine
Orbital Diagram: .; Electron Configuration: .
Exceptions to the Aufbau Principle
Chromium: (half-filled d-orbital stability); Copper: (fully filled d-orbital stability).
Example of Valence Electrons
Sulfur () has 6 valence electrons.
Example of Electron-Dot Structure
Oxygen () is represented with its symbol surrounded by dots representing valence electrons.
Rules for Writing Electron Configurations
Start with the lowest energy orbital; Apply the Pauli exclusion principle and Hund's rule to fill orbitals.
Features of the Aufbau Principle
Electrons occupy the lowest-energy orbitals first; Orbitals within the same sublevel are degenerate; Overlap between levels occurs.
Example of Aufbau Principle
Hydrogen (), Lithium ().
Example of Pauli Exclusion Principle
Helium ().
Example of Hund's Rule
Nitrogen (): orbitals are singly occupied before electrons pair.
Summary of Key Points
Electron configurations explain the arrangement of electrons in orbitals; Valence electrons determine chemical properties; Electron-dot structures visually depict valence electrons.