JustinLevy said:
In the Fock basis, there would be a function of N positions for the N particle basis, right? And then there'd be a sum over all N.
Could someone please show the steps connecting the state in the "field eigenbasis" to the state in the "Fock basis" a bit more explicitly? Not just the math of "here is an equation", but the procedure ... ie. how we derive the connection between the two.
Can someone show what the "wavefunctional" equation would be for QED? I still don't understand how you are deriving these things since there are fields in the Lagrangian, but no wavefunctional.
First consider the single-particle case, i.e., ordinary quantum mechanics.
Working in the position representation just means working with the wave function whose values are the coefficients in the eigenbasis |x> of the commuting position operators x_1, x_2, x_3, short x:
|\psi> = \int dx \psi(x) |x>, where \psi(x)=<x|psi>
Working in the momentum representation just means working with the wave function whose values are the coefficients in the eigenbasis |p> of the commuting momentum operators p_1, p_2, p_3, short p:
|\psi> = \int dp \psi(p) |p>, where \psi(p)=<p|psi>
To translate between the two, one needs to know how to find the eigenstates
of p in the x-representation, and the eigenstates of x in the p-representation.
This is given by the Fourier transform.
Now consider a field theory. To get a representation one needs to pick a maximal commuting family of operators and their eigenstates. Depending on the choice, one gets different but isomorphic representations. By diagonalizing momenta, one gets
the traditional Fock representation in terms of eigenstates |p_1,...,p_N>, where N=0,1,2,... and each p_k is in R^3, and the wave functions are the coefficients \psi_N(p_1,...,p_N) in
|\psi> = \sum_N \int dp^N \psi_N(p_1,...,p_N) |p_1,...,p_N>,
Note that any 1-particle operator A lifts to the resulting Fock space by means of
\hat A = \int dp a^*(p) A a(p) with the corresponding c/a operators,
giving in particular for the total momentum
\hat p |p_1,...,p_N>=(p_1+...+p_N) |p_1,...,p_N>,
showing that we have indeed eigenstates. This is the appropriate representation for
scattering experiments, where the input configurations are prepared in momentum eigenstates.
By diagonalizing instead Hermitian field operators at time t=0 (which commute because of the canonical commutation relations), one gets the functional Schroedinger representation in terms of eigenstates |\phi> (one state for each possible classical field configuration \phi at time t=0), and the wave functions \psi(\phi) are coefficients in a corresponding functional integral over all fields \phi.
(To get references, go to scholar.google.com and enter the key words functional schroedinger.) This is the appropriate representation when the field was prepared at time t=0.
Again conversion from one to the other representation requires the solution of the corresponding eigenproblems, but I haven't seen anyone do this explicitly.