THE VOCABULARY
Instruments, concepts, and phenomena — the shared vocabulary of the site.
inverse-square law
Force or intensity that falls as 1/r² with distance; the form of Newton's gravity and Coulomb's law.
isochronism
Property of oscillating with a constant period regardless of amplitude; Galileo's 1583 discovery.
KAM theorem
Most invariant tori of a near-integrable Hamiltonian system survive small perturbations. Proves the solar system is mostly stable.
kinematic equations
The three algebraic relations that describe motion under constant acceleration: v = v₀ + at, x = x₀ + v₀t + ½at², and v² = v₀² + 2a(x − x₀).
kinetic energy
The energy of a body in motion, ½·m·v², measured in joules.
kinetic friction
The friction force acting on a body that is already sliding; has fixed magnitude μ_k · N, independent of speed.
Kirchhoff's current law (KCL)
The sum of currents flowing into any node in a circuit equals the sum of currents flowing out. Equivalently: charge conservation applied to circuit junctions, ∇·J = 0 in steady state.
Kirchhoff's voltage law (KVL)
The sum of voltage drops around any closed loop in a circuit equals zero. Equivalently: the electrostatic field is conservative, ∮E·dℓ = 0 in the quasi-static limit.
Kramers formula
Hendrik Kramers's 1923 classical thick-target bremsstrahlung spectrum, dN/dE ∝ (E_max − E)/E, giving the continuous-continuum shape of an X-ray tube running at accelerating voltage U with E_max = eU. Full treatment in a later branch.
Lagrange points
Five equilibrium positions in the restricted three-body problem where gravitational and centrifugal forces balance.
Lagrangian
The scalar function L = KE − PE whose time-integral (the action) is minimised along the true path of a physical system.
Laminar flow
Orderly flow in parallel layers, without mixing across them. Characteristic of low Reynolds number.
Larmor formula
The classical expression P = q²a²/(6πε₀c³) for the total electromagnetic power radiated by a non-relativistic point charge of acceleration a. Derived by Joseph Larmor in 1897; the foundational result of classical radiation theory.
Larmor power
The instantaneous total radiated power P = q²a²/(6πε₀c³) of an accelerating point charge, integrated over all solid angle. Synonym of the Larmor formula result; the quantity that appears as the rate of energy loss in radiation-reaction problems.
Length contraction
The relativistic effect that an object of proper length L₀ measured in its rest frame appears contracted to L = L₀/γ along the direction of motion when measured by an observer in any inertial frame moving relative to the object. Symmetric; not a material compression; perpendicular dimensions unchanged.
Lenz's law
The direction of an induced current is always such that its own magnetic field opposes the change in flux that caused the induction. Equivalently: the minus sign in Faraday's law is a consequence of energy conservation.
libration
Bounded oscillation within a potential well, as opposed to full rotation.
Light-cone
The locus of events null-separated from a chosen origin event in spacetime; geometrically a 4D double cone with apex at the origin. The boundary between causally accessible (timelike-interior) and causally inaccessible (spacelike-exterior) regions; the structure that encodes relativistic causality.
Line integral
The integral of a vector field along a curve, measuring the accumulated effect of the field's component tangent to the path.
Linear polarization
An EM wave in which E oscillates along a single fixed line perpendicular to k. Equivalent to a superposition of two circularly polarised waves of equal amplitude with opposite handedness.
Liouville's theorem
Under Hamiltonian flow, phase-space volume is exactly conserved. The foundation of classical statistical mechanics.
Lorentz force
The total electromagnetic force on a point charge: F = q(E + v×B). Bridges Maxwell's macroscopic fields to the motion of individual particles.
Lorentz invariants of the EM field
The two scalar quantities — E·B and |E|² − c²|B|² — that every observer agrees on, regardless of their motion. Constructed as tensor traces from F^{μν}; classify the field as 'electric-like', 'magnetic-like', or 'null'.
Lorentz transformation
The linear coordinate transformation between two inertial frames in special relativity. For a boost along +x at velocity v: t' = γ(t − vx/c²), x' = γ(x − vt), y' = y, z' = z. Replaces the Galilean transformation; reduces to it in the limit β → 0.
Lorentz transformation of fields
The closed-form rule by which the components of E and B transform under a Lorentz boost. Parallel components are unchanged; perpendicular components mix linearly with the perpendicular components of the OTHER field. Derived by Hendrik Lorentz in 1895.
Lorenz gauge
The gauge condition ∇·A + (1/c²)∂V/∂t = 0, which decouples Maxwell's equations for the scalar potential V and vector potential A into two separate wave equations with the same speed c. Named for Ludvig Lorenz (not Hendrik Lorentz).
Luminiferous aether
The hypothetical all-pervasive medium that nineteenth-century physics posited as the substrate in which light waves propagate. Searched for via interferometry from 1881 onward; never detected. Discarded by Einstein's 1905 special-relativity paper.
Lyapunov exponent
The exponential rate λ at which nearby trajectories of a dynamical system diverge. Positive λ means chaos.
Mach number
The ratio of a source's speed to the speed of sound in the surrounding medium.
Magnetic dipole
The smallest possible source of a magnetic field — a tiny current loop or a single particle's intrinsic spin. The magnetic equivalent of an electric dipole.