Understanding optics and concepts like paraxial magnification and Snell's Law can be challenging, but with some practice and knowledge of the basic principles, you will be able to solve problems like this one.
To start, let's break down the problem into smaller parts. First, we need to understand what is meant by "paraxial domain." In optics, the paraxial domain refers to a small angle approximation, where the angles involved are small enough that we can use the tangent of the angle instead of the angle itself.
Next, we need to understand what is meant by "magnification produced by a single spherical interface between two continuous media." This refers to the change in size of an object when it passes through a curved surface, such as a lens. In this case, we are looking at a single spherical lens that separates two continuous media, with different refractive indices (n1 and n2).
The formula given, Mt=-n1s1/n2s0, represents the paraxial magnification produced by this spherical interface. The letters "s1" and "s0" represent the distances of the object and image from the lens, respectively. The negative sign indicates that the image is inverted compared to the object.
To solve this problem, we will use the small-angle approximation for Snell's Law, which states that sin θ ≈ θ for small angles. This allows us to use the tangent of the angles instead of the angles themselves.
Now, let's look at the problem step by step. We need to show that Mt=-n1s1/n2s0. We know that Mt represents the magnification, so let's start by finding the expression for it.
To do this, we can use the basic formula for magnification, which is given by M = -s'/s, where s' is the distance of the image from the lens and s is the distance of the object from the lens. Since we are dealing with a spherical interface, we can use the radius of curvature of the lens (R) to express s' and s.
s' = R - s0 and s = R - s1
Substituting these values into the magnification formula, we get:
Mt = -(R-s0)/(R-s1)
Next, we need to use Snell's Law to express the distances s0 and s1 in terms of the refractive indices (n1 and n2)
