Method of Generating Functions
Let X and Y be two smooth manifolds, and let M=T∗X,N=T∗Y with corresponding symplectic forms ωM and ωN.
Question: How can we produce symplectomorphisms ϕ:M→N?
The most important construction from classical mechanics is the method of generating functions. I will outline this method, shameless stolen from Ana Cannas da Silva's lecture notes.
Suppose we have a smooth function f∈C∞(X×Y). Then its graph Γ is a submanifold of M×N: Γ={(x,y,dfx,y)∈M×N}. Since M×N is a product, we have projections πM,πN, and this allows us to write the graph as
Γ={(x,y,dfx,dfy)}
Now there is a not-so-obvious trick: we consider the twisted graph Γσ given by
Γσ={(x,y,dfx,−dfy)}
Note the minus sign.
Proposition If Γσ is the graph of a diffeomorphism ϕ:M→N, then ϕ is a symplectomorphism.
Proof By construction, Γσ is a Lagrangian submanifold of M×N with respect to the twisted symplectic form π∗MωM−π∗NωN. It is a standard fact that a diffeomorphism is a symplectomorphism iff its graph is Lagrangian with respect to the twisted symplectic form, so we're done.
Now we have:
Modified question: Given f∈C∞(M×N), when is its graph the graph of a diffeomorphism ϕ:M→N?
Pick coordinates x on X and y on Y, with corresponding momenta ξ and η. Then if ϕ(x,ξ)=(y,η), we obtain
ξ=dxf, η=−dyf
Note the simlarity to Hamilton's equations. By the implicit function theorem, we can construct a (local) diffeomorphism ϕ as long as f is sufficiently non-degenerate.
Different Types of Generating Functions
We now concentrate on the special case of M=T∗R=R×R∗. Note that this is a cotangent bundle in two ways: T∗R≅T∗R∗. Hence we can construct local diffeomorphisms T∗R→T∗R in four ways, by taking functions of the forms
f(x1,x2), f(x1,p2), f(p1,x2), f(p1,p2)
Origins from the Action Principle, and Hamilton-Jacobi
Suppose that we have two actions
S1=∫p1˙q1−H1dt, S2=∫p2˙q2−H2dt
which give rise to the same dynamics. Then the Lagrangians must differ by a total derivative, i.e.
p1˙q1−H1=p2˙q2−H2+dfdt
Suppose that f=−q2p2+g(q1,p2,t). Then we have
p1˙q1−H1=−q2˙p2−H2+∂g∂t+∂g∂q1˙q1+∂g∂p2˙p2
Comparing coefficients, we find
p1=∂g∂q1, q2=∂g∂p2, H2=H1+∂g∂t
p1=∂g∂q1, q2=∂g∂p2, H2=H1+∂g∂t
Now suppose that the coordinates (q2,p2) are chosen so that Hamilton's equations become
˙q2=0, ˙p2=0
Then we must have H2=0, i.e.
H1+∂g∂t=0
Now we also have ∂H2/∂p2=0, so this tells us that g is independent of p2, i.e. g=g(q1,t). Since p1=∂g/∂q1, we obtain
∂g∂t+H1(q1,∂g∂q1)=0
This is the Hamilton-Jacobi equation, usually written as
∂S∂t+H(x,∂S∂x)=0
Note the similarity to the Schrodinger equation! In fact, one can derive the Hamilton-Jacobi equation from the Schrodinger equation by taking a wavefunction of the form
ψ(x,t)=A(x,t)exp(iℏS(x,t))
and expanding in powers of ℏ. This also helps to motivate the path integral formulation of quantum theory.
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