meopemuk
- 1,768
- 69
Arnold,
before doing any specific exercises I would like to understand the logic of what's going on.
It seems that we both agree that we are doing quantum mechanics in a certain Hilbert space (Fock space or non-Fock space, whatever). One of quantum postulates is that the time evolution is described by the Hamiltonian H as
|\psi(t) \rangle = \exp(iHt) |\psi(0) \rangle......(1)
If I understand correctly, the axiomatic Wightman approach does not use this formula and even refuses to provide an explicit form of the Hamiltonian H. Instead, it is suggested to use a set of Wightman functions in order to do the time evolution. I can believe that such Wightman functions can be calculated (perturbatively or non-perturbatively, exactly or approximately, it doesn't matter now). I can even believe that using these Wightman functions one can reproduce the same time evolution as given by equation (1).
If this is so, then given the full set of Wightman functions one should be able to recreate the Hamiltonian H. Presumably, this Hamiltonian should be formulated in terms of observables of physical (rather than bare) particles. I would like to know whether such a Hamiltonian has been constructed in simple QFT models? I haven't seen explicit formulas in the references that you've provided earlier. Is it because
(a) the Hamiltonian formulation is theoretically unacceptable for some reason?
(b) this is difficult to do, but people are working on it?
(c) I've just missed this piece of information?
(d) people working on these models dislike Hamiltonians for some reason, or just don't care to derive them?
(e) other?
Thanks.
Eugene.
before doing any specific exercises I would like to understand the logic of what's going on.
It seems that we both agree that we are doing quantum mechanics in a certain Hilbert space (Fock space or non-Fock space, whatever). One of quantum postulates is that the time evolution is described by the Hamiltonian H as
|\psi(t) \rangle = \exp(iHt) |\psi(0) \rangle......(1)
If I understand correctly, the axiomatic Wightman approach does not use this formula and even refuses to provide an explicit form of the Hamiltonian H. Instead, it is suggested to use a set of Wightman functions in order to do the time evolution. I can believe that such Wightman functions can be calculated (perturbatively or non-perturbatively, exactly or approximately, it doesn't matter now). I can even believe that using these Wightman functions one can reproduce the same time evolution as given by equation (1).
If this is so, then given the full set of Wightman functions one should be able to recreate the Hamiltonian H. Presumably, this Hamiltonian should be formulated in terms of observables of physical (rather than bare) particles. I would like to know whether such a Hamiltonian has been constructed in simple QFT models? I haven't seen explicit formulas in the references that you've provided earlier. Is it because
(a) the Hamiltonian formulation is theoretically unacceptable for some reason?
(b) this is difficult to do, but people are working on it?
(c) I've just missed this piece of information?
(d) people working on these models dislike Hamiltonians for some reason, or just don't care to derive them?
(e) other?
Thanks.
Eugene.