A Hamiltonian system is a dynamical system governed by Hamilton's equations. In physics, this dynamical system describes the evolution of a physical system such as a planetary system or an electron in an electromagnetic field. These systems can be studied in both Hamiltonian mechanics and dynamical systems theory.
Informally, a Hamiltonian system is a mathematical formalism developed by Hamilton to describe the evolution equations of a physical system. The advantage of this description is that it gives important insight about the dynamics, even if the initial value problem cannot be solved analytically. One example is the planetary movement of three bodies: even if there is no simple solution to the general problem, Poincaré showed for the first time that it exhibits deterministic chaos.
Formally, a Hamiltonian system is a dynamical system completely described by the scalar function , the Hamiltonian. The state of the system, , is described by the generalized coordinates 'momentum' and 'position' where both and are vectors with the same dimension N. So, the system is completely described by the 2N dimensional vector
and the evolution equation is given by the Hamilton's equations:
The trajectory is the solution of the initial value problem defined by the Hamilton's equations and the initial condition .
Time independent Hamiltonian system
If the Hamiltonian is not explicitly time dependent, i.e. if , then the Hamiltonian does not vary with time at all:
One example of time independent Hamiltonian system is the harmonic oscillator. Consider the system defined by the coordinates and whose Hamiltonian is given by
The Hamiltonian of this system does not depend on time and thus the energy of the system is conserved.
the evolution equation of the dynamical system can be written as
and IN the N×N identity matrix.
One important consequence of this property is that an infinitesimal phase-space volume is preserved. A corollary of this is Liouville's theorem, which states that on a Hamiltonian system, the phase-space volume of a closed surface is preserved under time evolution.
where the third equality comes from the divergence theorem.
- Dynamical billiards
- Planetary systems, more specifically, the n-body problem.
- Canonical general relativity
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- Treschev, D., & Zubelevich, O. (2010). Introduction to the perturbation theory of Hamiltonian systems. Heidelberg: Springer
- Zaslavsky, G. M. (2007). The physics of chaos in Hamiltonian systems. London: Imperial College Press.