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Thursday, July 26, 2012

Generating Functions

Method of Generating Functions


Let X and Y be two smooth manifolds, and let M=TX,N=TY with corresponding symplectic forms ωM and ωN.

Question: How can we produce symplectomorphisms ϕ:MN?

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 fC(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:MN, then ϕ is a symplectomorphism.

Proof By construction, Γσ is a Lagrangian submanifold of M×N with respect to the twisted symplectic form πMωMπNωN. 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 fC(M×N), when is its graph the graph of a diffeomorphism ϕ:MN?

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=TR=R×R. Note that this is a cotangent bundle in two ways: TRTR. Hence we can construct local diffeomorphisms TRTR 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˙q1H1dt, S2=p2˙q2H2dt
which give rise to the same dynamics. Then the Lagrangians must differ by a total derivative, i.e.
p1˙q1H1=p2˙q2H2+dfdt
Suppose that f=q2p2+g(q1,p2,t). Then we have
p1˙q1H1=q2˙p2H2+gt+gq1˙q1+gp2˙p2
Comparing coefficients, we find
p1=gq1, q2=gp2, H2=H1+gt

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+gt=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
gt+H1(q1,gq1)=0
This is the Hamilton-Jacobi equation, usually written as
St+H(x,Sx)=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(iS(x,t))
and expanding in powers of . This also helps to motivate the path integral formulation of quantum theory.

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