Nature always finds the path with the least 'cost' — like water flowing along the shortest and easiest channel.
In practice: Allows building optimal trajectories for spacecraft and designing energy-efficient mechanisms.
Even in antiquity, Heron of Alexandria noticed that light reflects at equal angles, as if seeking the shortest path. In 1744, Pierre Louis Maupertuis formulated a general principle: nature always acts in the most economical way. Leonhard Euler and Joseph-Louis Lagrange developed the mathematics: for mechanical systems there is a Lagrange function L (difference between kinetic and potential energy), and its integral over time — the action S — must be minimal on the real trajectory. William Hamilton reformulated mechanics in terms of action, and Emmy Noether showed that from the invariance (unchangingness) of the action under transformations follow conservation laws — of energy, momentum, charge. Today, the principle of least action is the foundation of all theoretical physics.
How it works
This principle explains why a thrown ball flies in a parabola: the parabola is the trajectory with the least action. It works everywhere: from planetary motion to scattering of elementary particles.
💡 Using this principle, Maxwell's equations for electromagnetism and the Schrödinger equation in quantum mechanics are derived.
The principle of least action says: from all possible ways of moving from point A to point B, the system 'chooses' the one where a special quantity — the action (denoted S) — reaches a minimum value. Action is like a total 'cost' of the path: it is made up of the difference between kinetic energy of motion (energy of speed) and potential energy (energy of position) at each moment in time. Nature 'pays' this cost in the least possible way. The condition δS = 0 (read 'the variation of the action is zero') is a mathematical way to say that the trajectory is precisely that one, with extremal action.
How it works
This principle explains why a thrown ball flies in a parabola: the parabola is the trajectory with the least action. It works everywhere: from planetary motion to scattering of elementary particles.
💡 Richard Feynman built quantum mechanics by assuming that a particle 'tries' all trajectories, and the classical path with minimal action is only the most probable. He tested his method on problems from a school olympiad.
The principle of least action (or principle of stationary action) asserts that the dynamics of a physical system is completely determined by the requirement of extremality of the action functional S = ∫ L dt, where L is the Lagrangian of the system. The variational condition δS = 0 yields the Euler-Lagrange equations. In classical mechanics L = T - V, in field theory — the Lagrangian density. Historically, the principle goes back to Maupertuis, Euler and Lagrange; Hamilton showed equivalence to the formulation through Hamiltonian equations. Noether (1918) linked symmetries of the action with conserved quantities. The principle extends to quantum mechanics through Feynman path integrals, where contributions of trajectories with non-extremal action are suppressed by interference.
Discovery
Ancient mechanics (Heron) used the idea of the shortest path for light. Pierre Louis Maupertuis in 1744 proposed the teleological 'law of economy'. Leonhard Euler reformulated it for mechanics, and Joseph-Louis Lagrange (1788) created analytical mechanics on the basis of variational calculus. William Rowan Hamilton (1834–35) introduced the concept of action as a fundamental notion. Emmy Noether in 1918 established the connection between symmetries of the action and conservation laws. Henri Poincaré developed the theory of variational principles in celestial mechanics and relativity theory.
How it works
The principle applies to any systems with finite or infinite number of degrees of freedom provided that the equations of motion can be derived from a variational principle. Limitations: dissipative systems (with friction) may not be variational without introducing additional variables. In quantum mechanics, the principle of least action is a limiting case ℏ → 0, but quantum corrections are described by a sum over all trajectories. Modern theories, including string theory, rely on the Lagrangian form.
Caveats
Is the principle violated for systems with irreversibility and dissipation without generalized Lagrangians?; Is the principle fundamental or an emergent property of quantum probabilities?; How to formulate action in quantum gravity theories without background spacetime?
S = \int_{t_1}^{t_2} L(q, \dot{q}, t) \, dt
S — action (functional on trajectories), L — Lagrangian (function of coordinates q, velocities \dot{q} and time t, usually the difference between kinetic and potential energy), t_1, t_2 — initial and final moments of time.
\delta S = 0
δ — variation, δS = 0 means that the action takes an extreme (usually minimum) value on the true trajectory.
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