Step 1: The kinetic energy gained by the body when it is accelerated through a potential difference \( V \) is given by: \[ K.E = \frac{1}{2} m v^2 = qV \]
where:
- \( m = 5 \, {g} = 5 \times 10^{-3} \, {kg} \),
- \( v = 10 \, {m/s} \),
- \( q = 5 \, \mu C = 5 \times 10^{-6} \, {C} \).
Step 2: The equation becomes: \[ \frac{1}{2} \times 5 \times 10^{-3} \times (10)^2 = 5 \times 10^{-6} \times V \] \[ \Rightarrow 0.25 = 5 \times 10^{-6} \times V \]
Step 3: Solving for \( V \): \[ V = \frac{0.25}{5 \times 10^{-6}} = 50 \, {kV} \]
Thus, the required potential difference is 50 kV.
Kepler's second law (law of areas) of planetary motion leads to law of conservation of
In the travelling plane wave equation given by \( y = A \sin \omega \left( \frac{x}{v} - t \right) \), where \( \omega \) is the angular velocity and \( v \) is the linear velocity.
The dimension of \( \omega t \) is:
Kepler's second law (law of areas) of planetary motion leads to law of conservation of