THE VOCABULARY
Instruments, concepts, and phenomena — the shared vocabulary of the site.
inertia
The tendency of a body to resist changes in its motion; the first of Newton's three laws.
inertial frame
A reference frame in which Newton's laws hold in their simple form; one that is not itself accelerating.
Inertial navigation
Navigation by integrating a vehicle's own rotations and accelerations — no external reference needed.
invariance
The property of a physical quantity or law of remaining unchanged under a specified transformation.
Invariant interval
The Lorentz-scalar combination s² = c²Δt² − Δx² − Δy² − Δz² between any two events. Invariant under Lorentz boosts and rotations; the special-relativistic analogue of Euclidean distance; its sign distinguishes timelike (s² > 0), spacelike (s² < 0), and null (s² = 0) separations.
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.
Kolmogorov spectrum
E(k) ∝ ε^(2/3) k^(−5/3) — the universal inertial-range energy spectrum of fully developed turbulence.
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.
Length contraction of current
The relativistic effect that a current-carrying lattice, viewed in the rest frame of its drift electrons, has its inter-ion spacing contracted by the Lorentz factor γ. Produces the net + charge density that explains magnetic attraction as relativistic electrostatics.
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.
lever
A rigid bar pivoting about a fulcrum, trading applied force against distance to achieve mechanical advantage.
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.