Step 1: Write equations for the two SHMs
Let the amplitude of each SHM be \(A\) and angular frequency be \(\omega\).
Let the phase difference between them be \(\phi\).
$$ y_1 = A \sin(\omega t) $$ $$ y_2 = A \sin(\omega t + \phi) $$
Step 2: Find resultant amplitude formula
When two SHMs of same frequency and same direction superpose, the resultant amplitude \(R\) is given by:
$$ R = \sqrt{A_1^2 + A_2^2 + 2A_1A_2\cos\phi} $$
Here \(A_1 = A_2 = A\), so:
$$ R = \sqrt{A^2 + A^2 + 2A \cdot A \cos\phi} = \sqrt{2A^2 + 2A^2\cos\phi} $$ $$ R = A\sqrt{2(1 + \cos\phi)} $$
Step 3: Use given condition
Given that resultant amplitude equals individual amplitude:
$$ R = A $$ $$ A = A\sqrt{2(1 + \cos\phi)} $$
Divide both sides by \(A\):
$$ 1 = \sqrt{2(1 + \cos\phi)} $$
Squaring both sides:
$$ 1 = 2(1 + \cos\phi) $$ $$ \frac{1}{2} = 1 + \cos\phi $$ $$ \cos\phi = \frac{1}{2} - 1 = -\frac{1}{2} $$
Step 4: Find phase difference
$$ \phi = \cos^{-1}\left(-\frac{1}{2}\right) $$
We know \(\cos\frac{2\pi}{3} = -\frac{1}{2}\)
$$ \phi = \frac{2\pi}{3} $$
Physical Interpretation: For the resultant to have the same amplitude as each component, the two vectors must be at \(120^\circ\) to each other. This forms an equilateral triangle with the two individual amplitudes and the resultant.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
Kepler's second law (law of areas) of planetary motion leads to law of conservation of