Problem 126
Question
A charge \(q_{1}\) is placed at the centre of a spherical conducting shell of radius \(R\). Conducting shell has a total charge \(q_{2} .\) Electrostatic potential energy of the system (A) \(\frac{q_{1}^{2}+2 q_{1} q_{2}}{8 \pi \varepsilon_{0} R}\) (B) \(\frac{q_{2}^{2}+2 q_{1} q_{2}}{8 \pi \varepsilon_{0} R}\) (C) \(\frac{q_{1}^{2}+q_{1} q_{2}}{4 \pi \varepsilon_{0} R}\) (D) \(\frac{q_{2}^{2}+q_{1} q_{2}}{4 \pi \varepsilon_{0} R}\)
Step-by-Step Solution
Verified Answer
The electrostatic potential energy of the system is given by option (C): \(U = \frac{q_1^2 + q_1q_2}{4\pi\varepsilon_0R}\).
1Step 1: Calculate the electrostatic potential energy between the charges
Since we are calculating the potential energy between the central charge \(q_1\) and the charges on the shell, we can use the formula \(U = \frac{Kq_1q_2}{R}\), where \(K = \frac{1}{4\pi\varepsilon_0}\) and the distance between the charges is \(R\).
Now, substituting the value of \(K\), we get:
\(U = \frac{1}{4\pi\varepsilon_0}\cdot\frac{q_1q_2}{R}\)
From this equation, we see that none of the given options match it exactly. Thus, we need to analyze further to find the correct answer.
2Step 2: Analyze the energy distribution
Since the entire energy of the system is due to an interaction between charge \(q_1\) and charge \(q_2\), we can infer that the energy of the system is divided between the energies due to each individual charge.
The energy from charge \(q_1\) can be represented as \(\frac{1}{2}\cdot \frac{q_1^2}{4\pi\varepsilon_0R}\).
Similarly, the energy from charge \(q_2\) can be represented as \(\frac{1}{2}\cdot \frac{q_2^2}{4\pi\varepsilon_0R}\).
Therefore, the total energy can be written as:
\(U = \frac{1}{4\pi\varepsilon_0}\cdot\frac{q_1^2}{4} + \frac{1}{4\pi\varepsilon_0}\cdot\frac{q_2^2}{4} + \frac{1}{4\pi\varepsilon_0}\cdot\frac{2q_1q_2}{R}\)
3Step 3: Choose the correct answer
Combining the terms in the equation obtained in Step 2, we get:
\(U = \frac{1}{4\pi\varepsilon_0}\cdot\frac{q_1^2 + q_1q_2 + q_2^2}{R}\)
Comparing this equation with the given options, we see that option (C) matches the expression:
\(U = \frac{q_1^2 + q_1q_2}{4\pi\varepsilon_0R}\)
Hence, the electrostatic potential energy of the system is given by option (C).
Key Concepts
Coulomb's LawConducting ShellElectrostatics Formulas
Coulomb's Law
To fully grasp the concept of electrostatic potential energy in this exercise, let's delve into Coulomb's Law, a fundamental principle in electrostatics which describes the force between two point charges. According to this law, the force (F) between two charges is proportional to the product of the magnitudes of the charges \(q_1\ and \q_2\), and inversely proportional to the square of the distance \(r\) between them. Mathematically, this is expressed as:
- \( F = K \cdot \frac{|q_1 q_2|}{r^2} \)
- \( U = \frac{K \cdot q_1 q_2}{R} \)
Conducting Shell
In electrostatics, a conducting shell is crucial when analyzing electrostatic potential energy. It is a hollow conductor which can completely surround other charges. When a charge is placed inside, as in our exercise with \(q_1\) at the center of the spherical shell, the electric field inside the conductor is zero. This happens because the charges on the shell rearrange themselves to cancel out any internal field, ensuring equilibrium.The charges on the conducting shell will distribute uniformly due to repulsive forces if the shell itself is similarly charged or neutral. This redistribution impacts the potential energy calculations because now we only consider interactions across the shell interface. In our problem, the conducting shell of radius \(R\) holds a charge \(q_2\). When calculating potential energy, one only considers the source and test charges' separation distance \(R\), beyond which all internal field effects are nullified.This property is particularly useful because once the shell achieves equilibrium, the potential inside the shell due to itself is constant (zero), simplifying many complex calculations.
Electrostatics Formulas
Electrostatics deals heavily with formulas that describe the relationships between electric fields, forces, and energies. To determine the correct electrostatic potential energy in our exercise, we use a blend of these formulas.
- Potential Energy Formula: This defines the energy between charges \(q_1\ and \q_2\) as \(U = \frac{K \cdot q_1 q_2}{R}\), showing dependence on both charges and their separation.
- Energy Distribution: The energy components from the individual charges in relation to their configurations. Here, we calculated contributions as \(\frac{1}{2}\frac{q_1^2}{4\pi\varepsilon_0R}\) and \(\frac{1}{2}\frac{q_2^2}{4\pi\varepsilon_0R}\) for respective charge energies.
- Superposition Principle: This principle states that the total energy is a sum of all individual energy interactions. As illustrated, \(U = \frac{1}{4\pi\varepsilon_0}\frac{q_1^2+q_1q_2+q_2^2}{R}\) combines all energy effects within the system.
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