Okay, so we were discussing optomechanics and after the introduction I just want to
focus first on the classical dynamics of these systems.
So that's the usual procedure.
If there is a meaningful classical limit, first discuss the classical equations of motion
and try to discuss the quantum vision.
So I want to start by writing down the classical equations of motion.
We wrote down a part of the quantum mechanical Hamiltonian, but we can really easily write
down the classical equations of motion including all the damping parts, for example, including
the fact that photons decay and that the mechanical oscillations decay.
So, the classical limit simply means for me that we replace the operator x by a classical
amplitude alpha, which is the variable x.
It's more difficult for the light field, but not really that difficult anyway if you know
about coherent states.
So in coherent states, which are the most classical states of the harmonic oscillator,
you would replace the operator a by a complex amplitude alpha that you can identify, say,
with the complex amplitude of the electric field inside the optical mode.
So the equations we are going to write down will be equations in x and the light field
and amplitude alpha.
We start with the mechanics because that is simple enough.
First I write down the equation of motion of a simple thermodynamic oscillator and then
I add to that the radiation pressure force.
So the left hand side describes the free damped harmonic oscillator and then we have the radiation
pressure force and we already discussed that in the quantum limit that was given by the
energy of one photon divided by the length of the cavity times the number of photons.
Now if you are in a highly excited state with a large complex amplitude alpha, then you
can replace a dagger a simply by alpha squared.
So this is the mechanics.
Now for the light mode, let's first try to write down the part that does not depend on
dissipation.
And that is something which we know in principle because we know, for example, what is the
equation of motion for the operator a and that directly translates into the equation
of motion for the complex amplitude alpha of a coherent state.
So that would simply tell you that alpha rotates at a frequency which would be the optical
frequency.
So what is the optical frequency?
Well, in our case it would be the bare optical frequency times this extra factor that takes
into account that we coupled to the mechanics.
So that would incorporate the fact that the light field oscillates at this frequency and
the frequency can change in response to this placement.
Now we have to add two terms and that is taking into account that photons decay and that there
is a laser driving the whole thing.
Now it's not so difficult to write down phenomenologically at least even without derivation a term that
would introduce some damping.
So then you would write alpha dot equals some decay rate times alpha.
So now we already defined a decay rate that was kappa.
Kappa was the decay rate for photons to leak out of the cavity so it would be the decay
rate for the intensity.
Kappa would be the rate at which the intensity alpha squared would decay if you have irradiated
the cavity and then you switch off the light field and then you look at the decay.
So if alpha squared goes like e to the minus kappa t then alpha should go like e to the
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01:08:24 Min
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2010-07-02
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2011-04-11 13:53:28
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Foundations of Quantum Mechanics:
Lecture 20
20.6.2013
(continued) Nelsons Stochastic Quantization (deriving the Schrödinger equation from a condition on a drift-diffusion process, nonlocality)
3.5 Optomechanical equations of motion (classical limit). 3.6 Linearized dynamics. Effective optomechanical damping rate and effective light-induced frequency shift (optical spring effect).