Resource Lesson
Speed of Light in Transparent Media
Printer Friendly Version
When radiation enters most transparent media, the ultraviolet photons and infrared photons are absorbed while the frequencies of visible light are transmitted. As the photons, the quanta of electromagnetic waves, move through the media, the electrons in the medium begin to move [vibrate] in response to the electruc field of the traveling radiation as it passes and exerts electric forces on the charged particles. The electrons, in turn, now start producing their own electric waves which superposition with both those of other electrons as well as with the original electromagnetic wave of the traveling photon. Since the waves produced by the vibrating electrons are moving much slower that that of the photon, the net result is a final wave moving through the medium at a speed slower than
c
.
In the following video Fermilab's Dr. Don Lincoln of
FermiLAB
explains this "slowing down of light" as it moves through a transparaent medium. He also explains why the "scattering" and "absorption" explanations for this phenomena are incorrect along with why light "apparently" speeds up when it exits the medium.
As Allen Everhear
stated
in an online forum: "The constant
c
is the speed of light in vacuum, far away from strong gravitation. In a transparent media the oscillating electromagnetic fields of light wiggle the electrons of the media. Wiggling electrons produces a light wave slightly out of phase with the incident wave. The combined incident and induced waves move through the medium slower than light in vacuum."
This question of why light slows while traveling through a medium is extremely complicated and still remains a subject of debate among physicists. Quantum mechanical events are prevasive in the more detailed arguments. Let this page and its links spark your curiosity and stimluate your further study.
Related Documents
Lab:
Labs -
A Photoelectric Effect Analogy
Labs -
Basic Particles
Labs -
Experimental Radius
Labs -
Hydrogen Spectrum
Labs -
Hydrogen Spectrum
Labs -
Mass of an Electron
Labs -
Mass of the Top Quark
Labs -
Mirror Symmetry
Labs -
Quantized Mass
Labs -
Radiation of a Metal Cylinder
Labs -
Using Young's Equation - Wavelength of a Helium-Neon Laser
Resource Lesson:
RL -
An Outline: Dual Nature of Light and Matter
RL -
Atomic Models and Spectra
RL -
Derivation of Bohr's Model for the Hydrogen Spectrum
RL -
Dr. Brian Cox Videos (In Search of Giants)
RL -
Energy-Level Diagrams
RL -
Famous Discoveries and Experiments
RL -
Famous Discoveries: Bohr Model
RL -
Famous Discoveries: de Broglie Matter Waves
RL -
Famous Discoveries: The Franck-Hertz Experiment
RL -
Famous Discoveries: The Photoelectric Effect
RL -
Famous Experiments: Davisson-Germer
RL -
Famous Experiments: Michelson-Morley
RL -
Famous Experiments: Millikan's Oil Drop
RL -
Famous Experiments: The Compton Effect
RL -
Famous Experiments: The Discovery of the Neutron
RL -
Fundamental Forces
RL -
Nuclear Reaction
RL -
Radioactive Halflife
RL -
What is Mass?
WS -
Parallel Reading - In Search of Giants
REV -
Orbitals
Worksheet:
APP -
Eternally Bohring
APP -
Nuclear Flu
APP -
The Science Fair
APP -
What's My Line
CP -
Atomic Nature of Matter
CP -
Atomic Nucleus and Radioactivity
CP -
Balancing Nuclear Equations
CP -
Natural Transmutations
CP -
Nuclear Fission and Fusion
CP -
Radioactive Half Life
CP -
The Atom and the Quantum
NT -
Atomic Number
NT -
Beta Decay
NT -
Binding Energy
NT -
Black Holes
NT -
Electrostatic Attraction
NT -
General Relativity
NT -
Helium Balloons
NT -
Hot Springs
NT -
Hydrogen Atom
NT -
Hydrogen Fusion
NT -
Nuclear Equations
NT -
Photoelectric Effect
NT -
Radiant Energy
NT -
Radioactive Cookies
NT -
The Ax Handle
NT -
Uranium Decay
NT -
Uranium Fission
RL -
Chapter 3: Electrons
WS -
Atomic Models and Spectra
WS -
Energy Level Diagrams
WS -
Parallel Reading - In Search of Giants
WS -
Particle Interactions and Feynman Diagrams
WS -
Rotational and Reflection Symmetries
WS -
Standard Model: Particles and Forces
WS -
Test Scenario: History of Matter
TB -
38A: Atomic Physics
TB -
Half-Life Properties
PhysicsLAB
Copyright © 1997-2026
Catharine H. Colwell
All rights reserved.
Application Programmer
Mark Acton