Okay, hello. We're just discussing the properties of the electromagnetic vacuum and in particular
we had been discussing an attempt at a local hidden variable theory that obviously cannot
work but still provides some interesting physical insights and that is termed stochastic electrodynamics.
And the idea is very simple. I told you last time you just assume that in classical Maxwell
electrodynamics you don't need to start with initial conditions where the field is just
zero everywhere but you can start instead with some arbitrary fluctuating field. Then
you can ask which properties does this fluctuating field has to have in terms of its spectrum
in order to be Lorentz invariance so that it does not select the preferred frame of
reference and it turns out there's exactly one and only one energy density spectrum that
gives you Lorentz invariance which is if the energy density spectrum goes like omega to
the third power. And so since you know the density of states in 3D is omega squared that
means the energy per mode automatically goes linear in frequency just as it does in quantum
electrodynamics simply because h bar omega half is the ground state energy of each mode.
And so starting from this h bar would be a free parameter which you take from experiment
and then you ask how does this affect say the motion of charges and we calculated the
simplest case which is a charge that is harmonically bound and interacts with this fluctuating
noise field. If there were only the noise then of course the charge would heat up and
increase its energy beyond any bound but also there is damping necessarily because it's
coupled to this radiation field and this damping is known as radiation damping and it has this
funny third time derivative of the position. Okay so that's the model we discussed. So
this is the fluctuating field plus our charge and we solved an equation which is the Newton's
equation of motion but the force would be the restoring force plus this radiation damping
force which goes like the third time derivative and so for dimensional reasons it should be
something like have a pre-factor with something like mass times the time plus the noisy field
and this particular time can be expressed in terms of the charge and fundamental constants.
It would be Q squared over M divided by 6 pi x down 0 C to the third. Okay and so since
this is a linear problem you can easily solve it. You'll find the response of the stamped
oscillator and in doing so we introduced a certain approximation. We said oh instead
of writing the third time derivative I can write down the second time derivative and
solve to lowest order this equation by equating it to x itself. So we said that x third time
derivative is about minus omega squared x dot so that automatically makes things easier
to solve. It tells you that this is indeed a damping force and it avoids some other problems
as well. So what is the spectrum we found? Here I'm plotting the fluctuation spectrum
for my position as a function of frequency. Of course it's strongly peaked at the resonance
frequency. The peak is of width gamma where gamma would be omega squared tau and then
it has some tails for example here it grows like omega to the third, here it goes down
like one over omega and so the variance of the position fluctuations will be just the
area under this curve. And it turns out this is h bar over 2 omega if you choose h bar
as the one adjustable parameter that would come from experiment and characterizes your
zero point fluctuations. Plus there are corrections. They will depend on the cutoff frequency
because the one over omega integral doesn't converge but these are like the corrections
in quantum electrodynamics. Again then you would have to introduce some randomization
procedure and so on. But this is obviously the ground state width of your quantum harmonic
oscillator and we also discussed that since the fluctuations of the field are Gaussian,
the fluctuations of x are Gaussian as well so even the full probability density just
looks exactly like in the quantum case. And so at least for this linear system there is
a nice correspondence between what quantum mechanics predicts and what you get from purely
classical electrodynamics assuming that you have such a Lorentz invariant zero point spectrum.
Now that means we have a very nice picture and it's good to compare the thermodynamics.
So in classical thermodynamics or statistical physics we would have the picture that I have
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01:22:26 Min
Aufnahmedatum
2013-07-15
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2013-09-02 12:33:42
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Foundations of Quantum Mechanics:
Lecture 28
(continued) Stochastic Electrodynamics;
9.4 Vacuum in Quantum optics;
9.5 Wave function of a photon;
9.6 Interaction of radiation with an atom (Purcell effect, virtual photon cloud) (note: chapter numbering is shifted in lecture)