BackAtomic Structure, Electromagnetic Radiation, and the Bohr Model: Study Notes
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Wave Properties of Electromagnetic Radiation
Electromagnetic Radiation as "Radiant Energy" (Light)
Electromagnetic radiation consists of oscillating electric and magnetic fields that propagate through space as waves. Light is a form of electromagnetic radiation and can be described by its wave properties.
Wavelength (λ): The distance between two consecutive peaks (or troughs) of a wave. Measured in meters (m), nanometers (nm), or angstroms (Å).
Frequency (ν): The number of wave cycles that pass a given point per second. Measured in hertz (Hz), where 1 Hz = 1 s-1.
Speed (c): The speed of light in a vacuum is a constant, m/s.
Relationship between speed, wavelength, and frequency:
Where is the speed of light, is the wavelength, and is the frequency.
Property | Definition | Symbol | Common Unit |
|---|---|---|---|
Wavelength | Peak-to-peak distance | m, nm, Å | |
Frequency | Number of cycles per second | Hz (s-1) | |
Speed | Velocity of light | m/s |
Different wavelengths correspond to different colors of visible light.
Longer wavelength = lower frequency
Shorter wavelength = higher frequency
Example: If three waves (A, B, C) are shown, the one with the longest wavelength has the lowest frequency.
Practice: Frequency-Wavelength Calculations
To find the wavelength of red light emitted by a barcode scanner at a frequency s-1:
Substitute values:
Result: m (or 649 nm)
The Photoelectric Effect
What Happens When Light Shines on Metals?
The photoelectric effect describes the emission of electrons from a metal surface when light of sufficient frequency shines on it. This phenomenon provided evidence for the particle nature of light.
If the frequency of light () is below a threshold value (), no electrons are emitted, regardless of intensity.
If , electrons are emitted. Increasing intensity increases the number of electrons emitted, but not their energy.
If , electrons are emitted with kinetic energy ().
Kinetic energy of emitted electrons:
Where is Planck's constant ( J·s), is the frequency of incident light, and is the work function (minimum energy required to remove an electron from the metal).
Energy Quantization and Photons
Energy is absorbed or emitted in discrete packets called quanta. A photon is a quantum of electromagnetic radiation.
Energy of a photon:
Where is Planck's constant and is the frequency.
Energy is quantized: only certain energy values are allowed.
Electromagnetic radiation exhibits both wave and particle properties (wave-particle duality).
Practice: Energy-Frequency-Wavelength Calculations
Example: UV radiation can break chemical bonds. To find the longest wavelength of light that can break a C–C bond (energy required: 348 kJ/mol):
Convert energy per mole to energy per photon:
Use to solve for .
Result: m (or 579 nm)
The Electromagnetic Spectrum
Overview and Classification
The electromagnetic spectrum encompasses all types of electromagnetic radiation, classified by wavelength and frequency.
Type | Wavelength Range | Frequency Range | Energy |
|---|---|---|---|
Radio | 103–10-1 m | 104–108 Hz | Lowest |
Microwave | 10-1–10-3 m | 108–1011 Hz | |
Infrared | 10-3–10-6 m | 1011–1014 Hz | |
Visible | 700–400 nm | 4.3 × 1014–7.5 × 1014 Hz | |
Ultraviolet | 10-7–10-8 m | 1015–1016 Hz | |
X-ray | 10-8–10-11 m | 1016–1019 Hz | |
Gamma ray | 10-11–10-14 m | 1019–1022 Hz | Highest |
Visible light is only a small portion of the spectrum, ranging from about 400 nm (violet) to 700 nm (red).
Absorption and Emission Spectra
Discrete Spectral Lines and Element Identification
When a hydrogen lamp emits light, it produces discrete wavelengths (lines), not a continuous spectrum. These lines are unique to each element and are used for identification.
Balmer and Rydberg developed equations to predict the wavelengths of hydrogen's spectral lines.
Absorption/emission spectra are unique to each element and are used in flame tests and instrumental analysis.
Element | Flame Test Color |
|---|---|
K (Potassium) | Violet |
Li (Lithium) | Red |
The Bohr Model of the Atom
Quantized Energy Levels in Hydrogen
The Bohr model proposes that electrons in a hydrogen atom move in certain allowed circular orbits around the nucleus, each with a specific energy. Energy levels are quantized, and electrons can only occupy these discrete levels.
Energy of an electron in the nth energy level:
J
Energy change for a transition between levels:
J
Ground state: Lowest energy level ()
Excited state: Any energy level higher than ground state ()
Energy is absorbed when an electron moves from lower to higher energy level.
Energy is emitted when an electron moves from higher to lower energy level.
Example: An electron transition from to emits energy as a photon.
Practice: Identifying Energy Level Transitions
Which energy level transitions result in absorption or emission of a photon?
Absorption: Electron moves to a higher energy level (e.g., to )
Emission: Electron moves to a lower energy level (e.g., to )
Shortest wavelength (highest energy) photon: Largest energy difference between levels.
Summary Table: Key Equations
Equation | Description |
|---|---|
Speed of light, wavelength, and frequency relationship | |
Energy of a photon | |
Kinetic energy of photoelectrons | |
Energy change for electron transitions in hydrogen |
Additional info: These notes cover foundational concepts in atomic structure, electromagnetic radiation, and quantum theory, which are essential for understanding chemical bonding and periodic properties in General Chemistry.