wofsy said:
perhaps you could elaborate a little more. I am still confused. I guess Feynman is just saying the KE is negative for pedagogical reasons though usually when he does something like that he has a disclaimer in the footnotes.
I still come down to his original argument which is 1) the bound electron in the hydrogen molecule has negative energy. 2) In regions of space where the electrostatic potential is low it is essentially a free particle. 3) from this it follows that p^2/2m is negative and p is imaginary ( de Broglie relations for a free particle). 4) the reason the electron can be found in these regions is because the quantum mechanical amplitude for the electron to flip from one proton to the other is non-zero.
1.) Right but that's total energy PE+KE and both classically and quantum mechanically that's no problem PE+KE< 0 <---> bound particle. (remember PE < 0)
2.) "Essentially" being the loaded word. Classically and quantum mechanically that's fine provided the KE is still less than the PE in magnitude. Be careful here to distinguish the cases of
I. > An excited but still bound particle far from the potential center (positive KE slightly less than PE in magnitude so TE < 0 but very close to 0 and momentum real.)
vs
II. >the nearly zero component of a ground-state (or nearly so) particle far from the center.
It is the first case applies both classically and quantum mechanically. No negative KE here.
I think it is in this case where in QM we may compare the bound particle's wave-function locally with that of a plane-wave. But remember the plane-wave solution is assuming the potential has been removed.
It is no different in essence than comparing the classical bound particle at a point in its orbit to the classical particle which is not bound (given you remove the potential) having the same momentum and moving in a straight line (tangent to the first's orbit at this point).
In the second case one is trying to make sense of observing a particle at a given position which has a kinetic energy less in magnitude than the potential energy at that position. This may be puzzling at first but you must remember that the act of measurement which gives this probability meaning will necessarily perturb both the potential and the total energy. In the specific case of say a ground state H atom the act of measuring position doesn't commute with the projection onto the s-orbital. Thus the fact that the electron is in the s-orbital is invalidated once the measurement of position is made (said measurement being what defines this probability far from the center.)
3.) Not necessarily as I've qualified 1.) and 2.)
4.) That "flipping" is a at worst a tunneling event, you never observe the particle where you would define its KE < 0. Only near one of the two protons where its KE > 0. So the issue becomes what do you mean by KE of the particle in a quantum setting between acts of measurement.
Also again you are deriving KE = TE-PE and assuming TE remains unchange and PE remains defined by the potential in the absence of external influences. When discussing the probability of measuring the position you are invalidating the "no external influences" assumption so it is not proper to hold TE constant while talking about the probability of measuring the particle at a given position.
Say you try to measure the position of the electron by focusing a pulse light at a region and seeing if the electron scatters light from a point in that region. (i.e. you try to "photograph" the electron.) Then the light being an electromagnetic wave will alter the electromagnetic potential and the scattering event will alter the total energy of the electron.
Now if you want to use negative KE and imaginary PE as a mathematical tool, fine. But you can't measure a particle with these properties and so shouldn't give them meaning in a physical context.
One example is where you resolve a physical particle's wave-function into components which do not all represent physical particles but rather differences in wave-functions of physical particles. This is sometimes necessary and we get "ghosts" or "virtual particles".
But this is no different in essence than say in a classical setting resolving a relativistic time-like particle motion (as seen by some observer) into a non-physical instantaneous spatial jump x\to x+\Delta x and a stationary physical wait t\to t+\Delta t. These are but components of the physical displacement vector (x,t)\to(x,t)+(\Delta x,\Delta t).
We can write
(x+\Delta x,t + \Delta t) = (x,t) + (\Delta x,0) + (0,\Delta t)
but we don't take the (\Delta x, 0) seriously as a physical motion. Its meaning is at best as the difference in two physical motions: (\Delta x,\Delta t)-(0,\Delta t).
So too we may sometimes write \psi = \psi_1 + \psi_2 where say \psi_1 by itself doesn't represent a physical mode.
Finally if you are trying to find say an imaginary eigen-value to the momentum operator you are choosing a representation where the momentum operator is no longer Hermitian and it becomes problematic to give it meaning as an observable. The eigen-function may be useful mathematically but saying it corresponds to a particle with imaginary momentum is stepping outside the domain of momentum as a physical observable.