mpv_plate said:
Thanks for this explanation. When the x operates on a state, the state (vector in a Hilbert space) becomes sort of multiplied by x. In the QFT, is a state (vector in a Fock space) also "multiplied" by the field operator?
I'm actually trying to understand what is mathematically changed in the field \Phi, to make it behave like an operator. Because multiplying a state by a field (function that assigns a number to each coordinate) does not seem to do the job of being an operator action.
Okay, here's what I hope is an enlightening discussion about the relationship between quantum field theory and quantum mechanics.
Suppose we have the following weird situation: You have a line of masses (labeled by consecutive integers) connected to each other by springs and also connected to a platform by springs. To simplify the motion (at the cost of a more complicated picture), I'm assuming that the masses are constrained to move vertically by rigid vertical rods running through them.
The energy associated with this system is given by:
E = \sum_n \lbrace \frac{m}{2} \dot{y_n}^2 + \frac{\lambda}{2} (y_n)^2 + \frac{\lambda}{2} (y_{n+1} - y_n)^2\rbrace
where y_n is the height of the n^{th} mass above its equilibrium height, \dot{y_n} is \dfrac{dy_n}{dt}, m is the mass of each of the masses, and \lambda is the spring constant.
Now, if we assume that the spring constant is large enough (a very stiff spring) that the masses don't move far from their equilibrium positions, then we can assume that y_n can be approximated by a continuous function \Phi(x) where x measures the horizontal location of the mass. If L is the distance between masses, then the horizontal location of n^{th} mass is nL. Then we can relate y_n to y_{n+1} by
y_{n+1} = \Phi((n+1)L) = \Phi(nL) + \dfrac{\partial \Phi}{\partial x} \delta x + \ldots = \Phi(nL) + \Phi' (nL) L + \ldots
where \Phi' = \dfrac{\partial \Phi}{\partial x}. In terms of \Phi, the energy can be written as
E = \sum_n \lbrace \frac{m}{2}\dot{\Phi}(nL)^2 + \frac{\lambda}{2} \Phi(nL)^2 + \frac{\lambda L^2}{2} \Phi'(nL)^2 \rbrace
This discrete sum can be approximated by an integral:
E = \dfrac{1}{L} \int \lbrace \frac{m}{2}\dot{\Phi}(x)^2 + \frac{\lambda}{2} \Phi(x)^2 + \frac{\lambda L^2}{2} \Phi'(x)^2 \rbrace dx
Now, the final bit of trickery is to define new constants:
\mu = \sqrt{\frac{\lambda}{m}}
c = \sqrt{\frac{\lambda}{m}} L
In terms of these constants, the energy for our system of oscillators looks like this:
E = \dfrac{m}{L} \int \lbrace \frac{1}{2}\dot{\Phi}(x)^2 + \frac{\mu^2}{2} \Phi(x)^2 + \frac{c^2}{2} \Phi'(x)^2 \rbrace dx
Mathematically, this is the relativistic hamiltonian for a free real scalar field in a spacetime with only one spatial dimension, although the constant c isn't actually the speed of light, but is the speed that vibrational waves travel through the system of harmonic oscillators.
Now, if you quantize the original system of harmonic oscillators, by replacing each of the masses by a quantum particle obeying Schrodinger's equation, that should be the same (given the approximations) as if you treated \Phi as a quantum field.