SUMMARY
The electric potential energy \( U \) of a uniformly charged hollow sphere and a point charge is defined as \( U = k \frac{q_1 q_2}{r} \) at the surface of the hollow sphere, where \( q_1 \) and \( q_2 \) are the charges of the sphere and the point charge, respectively, and \( r \) is the radius of the sphere. This relationship holds true under the assumption that the hollow sphere behaves like a point charge due to its spherical symmetry, as established by Newton's Shell Theorem. For distances greater than the radius of the sphere (\( R > r \)), the potential energy is given by \( U(R) = k \frac{q_1 q_2}{R} \), while for distances less than the radius (\( R < r \)), it remains \( U(R) = k \frac{q_1 q_2}{r} \).
PREREQUISITES
- Understanding of electric potential energy and Coulomb's law
- Familiarity with Newton's Shell Theorem
- Knowledge of spherical charge distributions
- Basic concepts of point charges in electrostatics
NEXT STEPS
- Study the implications of the Shell Theorem on non-spherical charge distributions
- Explore the derivation of electric potential energy formulas for various charge configurations
- Investigate the behavior of electric fields in relation to different geometrical shapes
- Learn about the applications of electric potential energy in real-world electrostatic systems
USEFUL FOR
Students of physics, electrical engineers, and anyone interested in electrostatics and the behavior of charged objects in various configurations.