Flashcards for topic Speed of Light
What is the condition for no net angular dispersion when combining two thin prisms (crown and flint glass)?
For no net angular dispersion, the ratio of refracting angles (A'/A) must equal:
Where:
This ensures that the dispersive effects of both prisms exactly cancel each other out while still allowing for net deviation.
Derive the fundamental equation used in Foucault's method for determining the speed of light.
In Foucault's method:
The speed of light equation is derived by:
Where R is mirror radius, ω is angular speed, a is the distance from lens to source, b is distance from mirror to lens, and s is the measured displacement.
What fundamental principle about the speed of light led to the special theory of relativity, and how does this affect how we define length today?
Fundamental principle: The speed of light in vacuum is invariant - it has the same value in all inertial reference frames regardless of the observer's motion.
This led to Einstein's special theory of relativity and a complete revision of our concepts of space and time.
Modern impact on length definition:
This invariance of light speed represents one of the most profound shifts in our understanding of physics.
Derive the formula for angular dispersion produced when two thin prisms with refracting angles A₁ and A₂ are combined with similar orientations.
For thin prisms with similar orientation:
Angular dispersion for a single prism: ω = A(μᵥ - μᵣ) Where (μᵥ - μᵣ) is the difference in refractive indices for violet and red light
For two prisms with similar orientation, dispersions add: ω = A₁Δμ₁ + A₂Δμ₂ Where Δμ = (μᵥ - μᵣ) for each material
Example calculation (from problem 11b): For prisms with A₁ = 5.3°, Δμ₁ = 0.014, A₂ = 3.7°, Δμ₂ = 0.024: ω = 5.3° × 0.014 + 3.7° × 0.024 ω = 0.0742 + 0.0888 ω = 0.163°
This is much larger than when the prisms are oppositely directed (0.0146°), demonstrating how similar orientation increases dispersion.
For a combination of two prisms, what is the condition for no net deviation in the yellow ray while still allowing for dispersion?
For no net deviation in the yellow ray (while still allowing dispersion):
Where:
This creates a system where:
This principle is used in direct-vision spectroscopes to produce a spectrum along the original light direction.
Why did Galileo's proposed method for measuring light speed fail, and what was the first successful approach to measuring it?
Galileo's method failed because:
First successful measurements:
Roemer's astronomical approach demonstrated that light had a finite speed, contradicting the prevailing belief that light propagation was instantaneous.
How does the current definition of the meter impact modern light speed measurements?
Current impact of meter definition on light speed measurements:
Key implications:
This represents a fundamental shift from pre-1983 when length was defined independently (prototype meter bar) and light speed was measured experimentally.
Derive the formula for calculating the speed of light using Foucault's rotating mirror method, starting from the relationship between mirror rotation angle and light travel time.
Derivation of Foucault's formula for speed of light:
Define key variables:
Core relationships:
Apply magnification principle:
Substitute θ = ω(2R/c):
Solve for c:
This formula allows calculation of light speed by measuring all quantities on the right side.
How does Fizeau's toothed wheel experiment measure the speed of light, and what are the physical principles and significance of this method?
The speed of light can be determined using: Where:
The experiment's elegance lies in converting the time domain (light's travel time) into the spatial domain (angular rotation of a physical object), making an extremely fast phenomenon measurable with 19th century technology.
Explain Foucault's method for measuring the speed of light, including its key innovations, advantages over Fizeau's method, and its historical significance in resolving the wave-particle debate.
Laboratory Implementation:
Measurement Capabilities:
This method transformed our understanding of light's properties and established measurement techniques that influenced future optical experiments.
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