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Section 1: Electrostatics
1: Coulomb's Law
Coulomb's Law is the fundamental principle governing the electrostatic force between two stationary point charges. Formulated by Charles-Augustin de Coulomb in 1785, it states: The magnitude of the electrostatic force (F) between two point charges (q1 and q2) is directly proportional to the product of their magnitudes and inversely proportional to the square of the distance (r) between them. The force acts along the line joining the charges.
Mathematical Formulation
The scalar form is: F=4πϵ01r2∣q1q2∣
where:
ϵ0 is the permittivity of free space (8.854×10−12C2N−1m−2),
r is the separation in meters (m),
q1 and q2 are the charges in coulombs (C).
The vector form is crucial for direction and superposition: F12=4πϵ01r2q1q2r^12
Here, F12 is the force on charge q1due toq2, and r^12 is the unit vector pointing fromq2toq1. The force is:
Repulsive for like charges (q1q2>0),
Attractive for unlike charges (q1q2<0).
The Superposition Principle
For a system of n point charges, the net force on any charge qi is the vector sum of forces exerted by all other charges: Fnet=∑j=i4πϵ01rij2qiqjr^ij
This principle allows calculation of forces in complex charge configurations.
Key Comparisons & Notes
Inverse-Square Dependence: Similar to Newton’s Law of Gravitation, but electrostatic force can be attractive or repulsive.
Strength: Electrostatic force is ∼1039 times stronger than gravity for protons.
Limitations: Applies strictly to point charges (size ≪r) and static charges (no motion).
Constant: The term 4πϵ01 (Coulomb's constant, k) equals 9×109N\cdotpm2C−2.
Understanding Coulomb’s Law is essential for analyzing electric fields, Gauss’s Law, and potential in subsequent sections.