- 0. Functions7h 52m
- Introduction to Functions16m
- Piecewise Functions10m
- Properties of Functions9m
- Common Functions1h 8m
- Transformations5m
- Combining Functions27m
- Exponent rules32m
- Exponential Functions28m
- Logarithmic Functions24m
- Properties of Logarithms34m
- Exponential & Logarithmic Equations35m
- Introduction to Trigonometric Functions38m
- Graphs of Trigonometric Functions44m
- Trigonometric Identities47m
- Inverse Trigonometric Functions48m
- 1. Limits and Continuity2h 2m
- 2. Intro to Derivatives1h 33m
- 3. Techniques of Differentiation3h 18m
- 4. Applications of Derivatives2h 38m
- 5. Graphical Applications of Derivatives6h 2m
- 6. Derivatives of Inverse, Exponential, & Logarithmic Functions2h 37m
- 7. Antiderivatives & Indefinite Integrals1h 26m
- 8. Definite Integrals3h 25m
5. Graphical Applications of Derivatives
Applied Optimization
Problem 4.5.56
Textbook Question
Snell’s Law Suppose a light source at A is in a medium in which light travels at a speed v₁ and that point B is in a medium in which light travels at a speed v₂ (see figure). Using Fermat’s Principle, which states that light travels along the path that requires the minimum travel time (Exercise 55), show that the path taken between points A and B satisfies (sinΘ₁/v₁ = (sin Θ₂) /v₂ . <IMAGE>

1
Start by understanding Fermat's Principle, which states that light travels between two points along the path that requires the least time. This principle will guide us in deriving Snell's Law.
Consider the path of light traveling from point A in medium 1 to point B in medium 2. The light will refract at the boundary between the two media. Let the angle of incidence be \( \theta_1 \) and the angle of refraction be \( \theta_2 \).
The time taken for light to travel from A to B can be expressed as the sum of the time taken in each medium. If \( d_1 \) is the distance traveled in medium 1 and \( d_2 \) is the distance in medium 2, then the total time \( T \) is given by \( T = \frac{d_1}{v_1} + \frac{d_2}{v_2} \).
Using trigonometry, express \( d_1 \) and \( d_2 \) in terms of the angles \( \theta_1 \) and \( \theta_2 \), and the horizontal distance \( x \) from the point of incidence to the point directly below A. This gives \( d_1 = x \tan \theta_1 \) and \( d_2 = (D-x) \tan \theta_2 \), where \( D \) is the total horizontal distance between A and B.
To find the path that minimizes the travel time, take the derivative of \( T \) with respect to \( x \) and set it to zero. This will lead to the condition \( \frac{\sin \theta_1}{v_1} = \frac{\sin \theta_2}{v_2} \), which is Snell's Law.
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