Coulomb's law describes the electrostatic force between charged particles as inversely proportional to the square of their distance.Coulomb's law is a rule that explains with what force electric charges attract or repel. Imagine you have two magnets: if you bring them together with like poles, they repel, and with opposite poles, they attract. The same with charges: like (plus-plus or minus-minus) repel, unlike (plus-minus) attract. The force depends on the magnitude of the charges and the distance between them: the larger the charges and the closer they are, the stronger the interaction.
The law was formulated by Charles-Augustin de Coulomb in 1785 based on experiments with a torsion balance. Earlier, a similar dependence for magnetic interactions was suggested by John Robison and Henry Cavendish, but Coulomb was the first to publish results for electric charges. Later, the law was incorporated by James Clerk Maxwell into his system of equations, becoming part of classical electrodynamics. The experimental accuracy of the law has been confirmed to a high degree, and its form is analogous to Newton's law of gravitation.
Coulomb's law applies to point charges or spherically symmetric charge distributions in electrostatics. It allows calculation of electric fields and potentials, underlies capacitors, motion of charged particles in accelerators, and many other phenomena. In atomic physics, it describes the attractive force between the nucleus and electrons, although quantum mechanics is needed for an accurate description of atoms. Limits of applicability: the law is valid in inertial reference frames for stationary charges; when charges move, magnetic effects and retardation must be considered.
Coulomb's law is surprisingly similar to Newton's law of universal gravitation! In both cases, the force depends on distance in the same way: inversely proportional to the square of the distance. Only in gravity the force always attracts, while in electricity it can also repel.
| dσ/dE | variable | Differential cross section for breakup as a function of energy — differential cross section metre squared per joule |
| N_γ(E) | variable | Number of virtual photons per unit energy — virtual photon number per joule |
| dB(E1)/dE | variable | Differential E1 transition strength per unit energy — differential transition probability coulomb squared metre squared per joule |
| ∝ | operator | Indicates direct proportionality between quantities — proportionality |
| σ | variable | Cross section — cross section metre squared |
| E | variable | Energy of the incident particle — energy joule |
| α | variable | Power-law exponent — dimensionless exponent |
| ∝ | operator | Proportional to, up to a constant factor — proportionality |
| i | variable | inclination angle of the orbital plane — inclination angle radian |
| b | variable | minor axis of the projected orbit — minor axis metre |
| a | variable | major axis of the projected orbit — major axis metre |
| cos | operator | cosine function — cosine function |


















