method

lagrangian

A Lagrangian is a mathematical function used to describe the dynamics of a system, often applied in optimization and motion analysis.
25 related articles · 3 formulas · 2 who worked here

Description

The Lagrangian is a function depending on the coordinates and velocities of all parts of a system. Instead of considering forces, as in Newtonian mechanics, one operates with energies: kinetic (energy of motion) and potential (energy of position). From the principle of least action it follows that the actual motion of a system occurs such that the total difference of these energies along the trajectory is minimal. This approach is particularly convenient for systems with constraints, e.g., a pendulum on an inextensible string, and allows one to derive the equations of motion (Euler-Lagrange equations).

History

First presented by Joseph-Louis Lagrange in 'Analytical Mechanics' (1788) with the goal of constructing mechanics without geometric constructions. In the 19th century, William Rowan Hamilton reformulated it into Hamiltonian formalism. Henri Poincaré developed the theory of dynamical systems. Emmy Noether in 1918 proved the theorem linking continuous symmetries of the Lagrangian to conserved quantities. In quantum field theory, the Lagrangian became the basis of the Standard Model.

How it works

For a system with generalized coordinates q_i, the Lagrangian is written as L(q, q̇, t) = T − V. The Euler-Lagrange equations are obtained by requiring the variation of the action to be zero. For example, for a particle in a potential field, L = ½ m ẋ² − V(x). Noether's theorem states: to each continuous symmetry of the Lagrangian there corresponds a conserved integral of motion (energy, momentum, etc.).

In practice

Used for calculating the orbits of planets, trajectories of rockets, optimizing mechanical devices, and in the foundations of quantum theory.

Fun fact

Lagrange's method made it possible to solve problems that were too complex for the direct application of Newton's laws, such as the motion of many-body systems with constraints.

Concept graph →

Formulas

$$\ddot{x} + \gamma \dot{x} + \omega^2 x = \eta(t)$$
Describes motion with damping, restoring force, and random driving.
What is in the formula
xvariablePosition of the particle — position metre
γvariableDamping coefficient — damping coefficient per second
ωvariableNatural angular frequency of the oscillator — angular frequency radian per second
η(t)variableRandom force (noise) as a function of time — random force newton per kilogram
d²/dt²operatorSecond derivative with respect to time — second time derivative
d/dtoperatorFirst derivative with respect to time — first time derivative
\ddot{h}+γ\dot{h}+ω^2h=\eta(t) · 2607.28209v1
$$k(r) = rac{\sigma^2 2^{1-\nu}}{\Gamma(\nu)} \left( \frac{\sqrt{2\nu} r}{l} \right)^\nu K_\nu \left( \frac{\sqrt{2\nu} r}{l} \right)$$
A covariance function for Gaussian processes with smoothness parameter ν.
What is in the formula
rvariabledistance between two points — distance metre
νvariablesmoothness parameter
lvariablelength scale parameter — length metre
σvariablevariance amplitude — variance square metre
ΓoperatorGamma function, generalizes factorial — gamma function
K_νoperatorModified Bessel function of the second kind of order ν — modified bessel function second kind
k_ν(r)=σ_f^2\frac{2^{1-ν}}{\gamma(ν)}(\frac{\sqrt{2ν}r}{l_f})^νk_ν(\frac{\sqrt{2ν}r}{l_f}) · 2601.06656
$$S_E = \int L_E d\tau$$
Action in Euclidean time for path integral weighting.
What is in the formula
S_EvariableEuclidean action — action joule second
L_EvariableEuclidean Lagrangian — lagrangian joule
τvariableEuclidean time — time second
∫operatorIntegration over Euclidean time — integral operator
dτoperatorInfinitesimal time element — differential element

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