Initially, sphere A has a charge \( Q_A \) corresponding to the potential \( V \), and shell B is uncharged. When the two conductors are connected by a wire, charges will flow between them until they reach the same potential, because a conducting wire ensures that the potential difference between them becomes zero.
The potential of a sphere due to its charge is given by the formula: \[ V = \frac{kQ}{r} \] where: - \( k \) is Coulomb's constant \( \left( k = \frac{1}{4 \pi \epsilon_0} \right) \), - \( Q \) is the charge on the sphere, - \( r \) is the radius of the sphere.
The initial charge on sphere A, when its potential is \( V \), is: \[ Q_A = \frac{V r}{k} \]
When spheres A and B are connected, charge will flow until both spheres are at the same potential. Let \( V_f \) represent the final common potential of both sphere A and shell B.
Since charge is conserved, the total charge on both sphere A and shell B must remain the same. The total charge initially on the system is just the charge on sphere A (since shell B starts uncharged): \[ Q_{\text{total}} = Q_A = \frac{V r}{k} \]
The potential of sphere A after charge redistribution is: \[ V_A = \frac{k Q_A}{r} \] And the potential of shell B after redistribution is: \[ V_B = \frac{k Q_B}{R} \] Since \( Q_A = Q_B \), we can say that the final potential \( V_f \) on both spheres is: \[ V_f = \frac{k Q_A}{R} \]
Using the fact that the total charge is conserved, and that the potential on both spheres is the same, we get the final potential: \[ V_f = \frac{k Q_A}{r + R} \]
The final potential on sphere A and shell B is \( V_f \), and it is the same for both: \[ V_f = \boxed{\frac{V r}{R}} \]