Processing math: 100%

Classical phase density

Set

context M,H … classical Hamiltonian system
definiendum ˆρit
postulate M,H … Hamiltonian system
range ΓMM×TM
postulate ˆρ:ΓM×RR+
range ˆρ::ˆρ(q,p,t)
postulate tˆρ=(ˆρXH)
todo: Total derivative for the 'Continuity equation' (last postulate)
todo: Hamiltonian vector field

Discussion

For all initial values π(0)ΓM, the solutions of the Hamiltonian equations of motion follow the Hamiltonian flow XH. Because phase trajectories can't intersect (the Hamiltonian equations are first order in time), a given sub volume Σ of ΓM flows along XH with only smooth distortion of its boundary Σ. Morally, the phase density counts the number of system points in any given subset of the phase volume: If we specify such a volume Σt0ΓM where the index denotes some point in time, then Σt0ˆρ(q,p,t0)=Σt1ˆρ(q,p,t1). The phase density doesn't literally count ensemble points, as there are be infinitely many. So ˆρ is assigned any initial value ˆρ(q,p,0) which is soon factored out in a normalization, see Classical probability density function.

We denote the measure in ΓM simply by dΓ.

Using the Hamiltonian equations, we can pull out XH and get the Liouville equations:

Theorems

Liouville equation

(t+XH)ˆρ=0

which can also be written as

ddtˆρ(π(t),t)=0

where π is the solution of the Hamiltonian equations.

Reference

Wikipedia: Continuity equation, Liouville equations, Cluster expansion


Refinement of

ODE system

Context

Classical Hamiltonian system

Hamiltonian equations