Okay, hello everybody. Let's start our first lecture this year. And last time it
was a lecture about polarization in quantum optics and I didn't finish. So
today I will continue about polarization and hopefully tell you the next lecture
which is lecture number nine which is about nonlinear effects creating
non-classical light. So polarization. I finished by introducing a polarized
single photon which had in short notation it was written like alpha h
plus beta v and so h and v are just single photon states polarized
horizontally and vertically and there was normalization condition alpha square
plus beta squared is one and so the pair the cup the pair of numbers alpha and
beta they are complex numbers but they have this restriction and also they
have the feature that the total phase of this state doesn't matter and we can
attribute the phase just to beta not to alpha and it means that we basically
have two real numbers characterizing this polarization qubit. In fact it is a
polarization qubit as I think I mentioned at the very first lecture a
single polarized photon but before explaining how it can be treated on the
Poincare sphere and so on I want to consider once again the subject of
polarization measurement and this is the Stokes measurement because classical and
quantum descriptions of measurement differ a little bit and because we
introduced the Stokes operators let's consider measurement of the Stokes
observables corresponding to the Stokes operators. In quantum mechanics measuring
an observable corresponding operator means that we have to project the state
on eigenstates on the eigenstates of this operator and so we have to find the
eigenstates of the Stokes operator. How do we do it? We consider this class of
states single photon states and let's consider first S1 which I remind you is
a h dagger a h minus a v dagger a v you remember what a h and a v are
annihilation operators in the horizontal and vertical polarization modes and we
just have to solve the equation that S1 psi is some number S1 times psi and if
we substitute all this we obtain the equation a h dagger a h minus a v dagger a
v times alpha h plus beta v is equal to S1 alpha h plus beta v and of course we
have to first let's let's see what happens when we act by this operator on
this state and this is the photon number operator in mode h this is photon
number operator in mode v so when we act by this operator on this state h we just
get the eigen this is the eigenstate of this operator right so the eigenvalue is
one and if we act by this operator on this state the eigenvalue is zero
because in the horizontal mode here there is no photon there are zero
photons so I remind you that this state basically is alpha one photon in h mode
and zero photon in v mode and the other way around for the second state so the
result of acting by this operator on this state will be alpha h because here
the eigenvalue is one minus beta v because of this minus and this has to be
equal to S1 alpha h plus beta v and then we have to write equality separately
for this vector and for this vector because they are orthogonal so we have a
system of equations first equation alpha is alpha minus 1 minus s1 is 0 by by
just taking the part of this inequality relating to h and for the v part we get
the equality beta 1 plus s1 is 0 and this is a system of equations we see
that the first equation has two solutions so either s1 is 1 and then but
then from the second equation we get that beta has to be 0 beta is 0 and we
get the qubit from this we get the qubit well first eigen state of the first
Stokes operator with the eigenvalue 1 is just well we write this vector like this
1 1 0 because beta is 0 means that alpha is 1 so we get this state and the second
case we get from this equation that s1 can be minus 1 and then from this
Presenters
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Offener Zugang
Dauer
01:42:29 Min
Aufnahmedatum
2019-01-17
Hochgeladen am
2019-01-21 09:57:50
Sprache
en-US
1. Basic concepts of statistical optics
2. Spatial and temporal coherence. Coherent modes, photon number per mode
3. Intensity fluctuations and Hanbury Brown and Twiss experiment
4. Interaction between atom and light (semiclassical description)
5. Quantization of the electromagnetic field
6. Quantum operators and quantum states
7. Heisenberg and Schrödinger pictures
8. Polarization in quantum optics
9. Nonlinear optical effects for producing nonclassical light
10. Parametric down-conversion and four-wave mixing, biphotons, squeezed light
11. Single-photon states and single-photon emitters
12. Entanglement and Bell’s inequality violation