
Hamiltonian mechanics is a reformulation of classical mechanics that describes the evolution of a system using generalized coordinates and momenta.The protagonist of Hamiltonian mechanics is the Hamiltonian function, i.e., the total energy of the system expressed in terms of coordinates and momenta. Unlike the Newtonian approach, where force causes acceleration, here energy reigns. A pair of Hamilton's equations (the first linking velocity to momentum, the second linking change in momentum to force) turns mechanics into the geometry of phase space: each state is a point, and evolution is a line on the energy landscape. This perspective clarifies why energy, momentum, and other quantities are conserved.
The idea grew out of geometric optics. William Rowan Hamilton in 1833 applied the optical-mechanical analogy to rewrite Newton's laws in terms of energy. Later, Henri Poincaré used Hamiltonian methods to analyze the stability of the Solar System, laying the foundation for chaos theory. Emmy Noether proved that every continuous symmetry of a Hamiltonian system corresponds to a conserved quantity — a result that cemented the foundation of all modern physics.
The Hamiltonian function H generates a vector field in phase space. The integral curves of this field are the system's trajectories. If H does not depend explicitly on time, energy is conserved. In the quantum picture, the Hamiltonian becomes an operator that determines the evolution of the wave function via the Schrödinger equation. Canonical transformations here become unitary transformations, and Liouville's theorem becomes the unitarity of quantum evolution.
Calculating satellite orbits, modeling quantum computers, synthesizing new materials with desired properties.
The formalism turned out to be so elegant that it crossed over into quantum mechanics almost unchanged: the Hamiltonian operator became the main tool for describing particles and fields.
| H | variable | Hamiltonian (total energy operator) — hamiltonian joule |
| J_{ij} | variable | Exchange coupling constant between sites i and j — exchange coupling joule |
| \mathbf{S}_i | variable | Spin operator at site i — spin operator |
| \mathbf{S}_j | variable | Spin operator at site j — spin operator |
| \sum_{\langle i,j \r | operator | Summation over all pairs of adjacent lattice sites — sum over nearest neighbors |
| H_eff | variable | effective static Hamiltonian — hamiltonian joule |
| H_0 | variable | time-averaged Hamiltonian — hamiltonian joule |
| H_{-1} | variable | first negative Fourier component of the Hamiltonian — hamiltonian joule |
| H_{+1} | variable | first positive Fourier component of the Hamiltonian — hamiltonian joule |
| frequency | variable | driving frequency — angular frequency radian per second |
| [ , ] | operator | measures the non-commutativity of two operators — commutator |
| H | variable | Hamiltonian operator — hamiltonian joule |
| t | variable | hopping amplitude — energy joule |
| γ_{2j} | variable | Majorana operator at site 2j — majorana operator |
| γ_{2j+1} | variable | Majorana operator at site 2j+1 — majorana operator |
| ∑ | operator | sum over lattice sites j — summation |
| x | variable | Position of the particle — position metre |
| γ | variable | Damping coefficient — damping coefficient per second |
| ω | variable | Natural angular frequency of the oscillator — angular frequency radian per second |
| η(t) | variable | Random force (noise) as a function of time — random force newton per kilogram |
| d²/dt² | operator | Second derivative with respect to time — second time derivative |
| d/dt | operator | First derivative with respect to time — first time derivative |
| J | variable | exchange coupling constant — exchange coupling constant joule |
| σ₊ | variable | spin raising operator — spin raising operator |
| σ₋ | variable | spin lowering operator — spin lowering operator |














