Concept:
In ray optics, Newton's formula relates the object distance, image distance, and focal length of a spherical mirror when the distances are measured from the principal focus instead of the pole. This often provides a faster way to solve mirror problems.
Step 1: Defining the coordinates from the pole.
Let the distances measured from the pole of the concave mirror be:
• Object distance, \(u = -(f + x)\)
• Image distance, \(v = -(f + y)\)
• Focal length, \(= -f\)
Step 2: Applying the spherical mirror formula.
The standard mirror formula is:
\[
\frac{1}{v} + \frac{1}{u} = \frac{1}{f}
\]
Step 3: Substituting values and simplifying.
Substituting the values from
Step 1:
\[
\frac{1}{-(f+y)} + \frac{1}{-(f+x)} = \frac{1}{-f}
\]
Multiplying the entire equation by \(-1\):
\[
\frac{1}{f+y} + \frac{1}{f+x} = \frac{1}{f}
\]
Taking the LCM on the left side:
\[
\frac{(f+x) + (f+y)}{(f+x)(f+y)} = \frac{1}{f}
\]
\[
\frac{2f + x + y}{(f+x)(f+y)} = \frac{1}{f}
\]
Cross-multiplying:
\[
f(2f + x + y) = (f+x)(f+y)
\]
\[
2f^2 + fx + fy = f^2 + fy + fx + xy
\]
Canceling common terms (\(fx\) and \(fy\)) and subtracting \(f^2\):
\[
2f^2 - f^2 = xy
\]
\[
f^2 = xy
\]
Step 4: Selecting the correct option.
From the calculation above, we get:
\[
\boxed{xy = f^2}
\]
Therefore, the correct option is:
\[
\boxed{\text{Option (B)}}
\]