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In Problems 5 to 7, use Fermat's principle to find the path followed by a light ray if the index of refraction is proportional to the given function. $$ x^{-1 / 2} $$

Short Answer

Expert verified
The path is found by solving the differential equation from Fermat's principle, involving the given index of refraction.

Step by step solution

01

Understand Fermat's Principle

Fermat's principle states that the path taken by a light ray between two points is the path that can be traversed in the least time. This means that we need to find the path which minimizes the optical path length given by the integral \[ \text{Optical Path Length} = \int n(x) \, ds \] where \(n(x)\) is the index of refraction and \(ds\) is the infinitesimal arc length along the path of the light ray.
02

Define the Index of Refraction

Given that the index of refraction \(n\) is proportional to \(x^{-1/2}\), we can write: \[ n(x) = k \cdot x^{-1/2} \] where \(k\) is a constant of proportionality.
03

Set Up the Integral for the Optical Path Length

The optical path length is given by: \[ \text{Optical Path Length} = \int k \cdot x^{-1/2} \, ds \] We need to parameterize the path \(ds\) in terms of \(x\) or \(y\). For simplicity, assume the path is parameterized in terms of \(x\).
04

Parameterize the Path

Using the parameterization in terms of \(x\), we have \[ ds^2 = dx^2 + dy^2 \quad \text{so} \quad ds = \sqrt{dx^2 + dy^2} \] To make integration possible, it's easier to express \(ds\) via a single variable. For example, if we express in terms of \(x\): \[ ds = \sqrt{1 + \left( \frac{dy}{dx} \right)^2} \, dx \]
05

Set Up the Integral with Path Parameterization

Now substitute \(ds = \sqrt{1 + \left( \frac{dy}{dx} \right)^2} \, dx\) into the optical path length integral: \[ \text{Optical Path Length} = \int k \cdot x^{-1/2} \sqrt{1 + \left( \frac{dy}{dx} \right)^2} \, dx \]
06

Apply the Euler-Lagrange Equation

To minimize the integral, apply the Euler-Lagrange equation \[ \frac{d}{dx} \( \frac{\partial F}{\partial y_x} \) - \frac{\partial F}{\partial y} = 0 \] where \(F = k \cdot x^{-1/2} \sqrt{1 + \left( \frac{dy}{dx} \right)^2} \) and \(y_x = \frac{dy}{dx} \). Here, \(F\) does not explicitly depend on \(y\), so the equation reduces to \[ \frac{d}{dx} \( \frac{\partial F}{\partial y_x} \) = 0 \]
07

Simplify and Solve the Euler-Lagrange Equation

Compute \(\frac{\partial F}{\partial y_x}\) and solve for the Euler-Lagrange equation: \[ \frac{\partial F}{\partial y_x} = k x^{-1/2} \frac{y_x}{\sqrt{1 + y_x^2}} \rightarrow \frac{d}{dx} \( k x^{-1/2} \frac{y_x}{\sqrt{1 + y_x^2}} \) = 0 \] This equality implies that \[ k x^{-1/2} \frac{y_x}{\sqrt{1 + y_x^2}} = \text{constant} \]
08

Find the Path Equation

Isolate \(dy/dx\) and solve the resulting differential equation to find the expression for \(y(x)\). Since detailed integration may be complex, note that substitution or standard methods of solving differential equations should be used for the explicit form of the light path.

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

index of refraction
The index of refraction, often symbolized as 'n', is a measure of how much the speed of light is reduced inside a medium compared to its speed in a vacuum. Mathematically, it's expressed as:
\[ n = \frac{c}{v} \] where:
  • c is the speed of light in a vacuum, roughly 3 x 10^8 meters/second
  • v is the speed of light in the medium

In the given exercise, the index of refraction is described as proportional to the function \( x^{-1/2} \), meaning:
\[ n(x) = k \, x^{-1/2} \]
Here, 'k' is a constant of proportionality, essentially scaling how much the index changes with 'x'. Having the index of refraction in this form helps understand how light bends while traveling through mediums that change their refractive properties in space.
optical path length
The optical path length (OPL) is a concept that combines the physical distance a light ray travels with the medium's refractive index that the ray passes through. It’s defined by the integral:
\[ \text{Optical Path Length} = \int n(x) \, ds \]
Here, 'n(x)' is the index of refraction as a function of position 'x', and 'ds' is an infinitesimal element of the path length.
For a light ray traveling through a medium with a changing index of refraction, the OPL determines the 'effective' distance traveled by accounting for how much slower or faster light moves through different parts of the medium.
In our specific case, once parameterized, the OPL equation becomes:
\[ \text{Optical Path Length} = \int k \, x^{-1/2} \, \sqrt{ 1 + \left( \frac{dy}{dx} \right)^2 } \, dx \]
This integrates the refractive index contribution along the path length considering the geometry of the light ray’s path.
Euler-Lagrange equation
The Euler-Lagrange equation is a fundamental tool in calculus of variations, used to find the path that minimizes a given integral. In optics, it's used to find the path that minimizes the optical path length, in line with Fermat's principle. The general form of the Euler-Lagrange equation is:
\[ \frac{d}{dx} \left( \frac{\partial F}{\partial y_x} \right) - \frac{\partial F}{\partial y} = 0 \]
where \( F \) is the integrand of the functional to be minimized, and \( y_x = \frac{dy}{dx} \).
In the given problem, after defining the functional \( F \) based on the refractive index and path parameterization, we get:
\[ F = k \, x^{-1/2} \, \sqrt{ 1 + \left( y_x \right)^2 } \]
Given that \( F \) does not explicitly depend on 'y', the Euler-Lagrange equation simplifies to:
\[ \frac{d}{dx} \left( \frac{\partial F}{\partial y_x} \right) = 0 \]
This leads to the solution:
\[ k \, x^{-1/2} \, \frac{y_x}{\sqrt{1 + y_x^2}} = \text{constant} \]
Ultimately, solving this equation provides the path of the light ray that satisfies Fermat's principle, by minimizing the optical path length in the given refractive medium.

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Most popular questions from this chapter

Two particles each of mass \(m\) are connected by an (inextensible) string of length \(l\). One particle moves on a horizontal table (assume no friction). 'The string passes through a hole in the table and the particle at the lower end moves up and down along a vertical line. Find the Iagrange equations of motion of the particles. Hint: Let the coordinates of the particle on the table be \(r\) and \(\theta\), and let the coordinate of the other particle be \(z\). Eliminate one variable from \(L\) (using \(r+|z|=l)\) and write two Lagrange equations.

A particle moves on the surface of a sphere of radius \(a\) under the action of the earth's gravitational field. Find the \(\theta, \phi\) equations of motion. (Comment: This is called a spherical pendulum.)

Write and solve the Euler equations to make the following integrals stationary. \(\int_{x_{1}}^{x_{2}} e^{x} \sqrt{1+y^{\prime 2}} d x\)

Show that if \(F=F\left(x, y, z, y^{\prime}, z^{\prime}\right)\), and we want to find \(y(x)\) and \(z(x)\) to make \(I=\int_{x_{1}}^{x_{2}} F d x\) stationary, then \(y\) and \(z\) should each satisfy an Euler equation as in (5.1). Hint: Construct a formula for a varied path \(Y\) for \(y\) as in Section \(2[Y=y+\epsilon \eta(x)\) with \(\eta(x)\) arbitrary \(]\) and construct a similar formula for \(z\) [let \(Z=z+\epsilon \zeta(x)\), where \(\zeta(x)\) is another arbitrary function]. Carry through the details of differentiating with respect to \(\epsilon\), putting \(\epsilon=0\), and integrating by parts as in Section 2 ; then use the fact that both \(\eta(x)\) and \(\zeta(x)\) are arbitrary to get \((5.1)\)

Write and solve the Euler equations to make the following integrals stationary. Change the independent variable, if needed, to make the Euler equation simpler. \(\int_{0}^{\theta_{2}} \sqrt{r^{\prime 2}+r^{2}} d \theta, \quad r^{\prime}=d r / d \theta\)

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