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A portion of lecture notes from a university-level physics course on quantum optics. The lecture, titled 'quantum field theory', discusses the application of quantum theory to the behavior of light and photons. The professor outlines the intuition behind treating the electromagnetic field as a quantum field, the problem of handling an infinite number of photons, and the solution through mode expansion. The lecture also covers the concept of quantum states of light, including coherent and fock states, and the phenomenon of entangled field modes.
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Phys 531 Lecture 27 1 December 2005
Last time, discussed photon optics
Light energy comes in units of ℏω particles called photons observable with good detector
One consequence: light is intrinsically noisy
Today: introduce proper quantum theory Quantum field theory of light
Note, this work recognized with 2005 Nobel prize 1
Outline:
Do need some QM for this Material won’t be on final
Warning: derivations today not rigorous, some definitions simplified Consult Scully and Zubairy for real deal
Next time: review... bring questions!
Want proper quantum theory for photon
From last time, expect E(r) ∼ wave function ψ(r)
Since:
3
Intuition is right, but one problem
Number of photons is indefinite: photons easy to create and destroy
“Normal” QM assumes fixed N N = number of particles
Problem not just that N is unknown:
Can have quantum system in superposition
|ψ〉 =
( |atom + photon〉 + |excited atom〉
)
Photon in superposition of existing or not!
Could measure this state with polarizer along x
Imagine sending repeated pulses: each pulse in state Ψ
Each time get either 100% or 0% transmission unpredictable per pulse
Works even if EX and EY are classical states with many photons Simple version of Schrodinger’s cat
Could also have superpositions of beam position, frequency, etc.
7
Still have problem that E = E(r)
How to handle Ψ[E(r))]?
Solve by decomposing field into modes Usually, mode = plane wave
Easier to work inside a box, volume V
Then only discrete values of k allowed Get sums instead of integrals
Main advantage: makes normalization easier
Can write any E(r, t) as
E(r, t) =
∑ k
Akei(k·r−ωkt)
so state of field uniquely specified by {Ak}’s
Each mode k = independent degree of freedom Do QM on each independently
Treat each Ak as independent quantum variable Now a simple variable like X for a particle
9
But still one issue: Ak is complex
Really
E(r, t) =
∑ k
Re [Ak] cos (k · r − ωkt)
− Im[Ak] sin (k · r − ωkt)
Real and imaginary part of Ak both needed really two quantum variables per mode
Define
qk =
√ 0 V 2 ℏωk
Re Ak pk =
√ 0 V 2 ℏωk
ImAk
Two main results:
(1) Energy eigenstates are En = ℏω(n + 12 ) for integer n
⇒ photons!
(2) q and p don’t commute: [q, p] =
i 2 for our scale factors
Then can’t know q and p simultaneously:
∆q∆p ≥ 1 4 13
What do q and p correspond to physically?
Have A ∝ q + ip = amplitude of mode
Field ∝ q cos(k · r − ωt) − p sin(k · r − ωt)
So q is amplitude of wave ∼ cos() p is amplitude of wave ∼ sin()
Call components “quadratures” of wave
Of course, arbitrary which is which usually imagine a “reference oscillator” ∼ cos Define modes relative to it
Since ∆q∆p ≥ 1 /4, amplitudes can’t have definite values
Draw picture: Say 〈q〉 large, 〈p〉 = 0 and ∆q ∆p
E
t Amplitude of wave is uncertain
15
Or, if 〈q〉 large but ∆q ∆p:
E
t
Amplitude well-defined, but phase uncertain
Question: What if 〈p〉 and ∆q were large, and 〈q〉 and ∆p were small? Would the phase or amplitude be more certain?
What is uncertainty in N?
Have N ' q^2 + p^2
So ∆N '
( ∂N ∂q
) 2 ∆q^2 +
( ∂N ∂p
) 2 ∆p^2
1 / 2
[ (2q)^2 ∆q^2 + (2p)^2 ∆p^2
] 1 / 2
( q^2 + p^2
) 1 / 2
since ∆q = ∆p = 1/ 2
Same quantum noise from last time!
19
If ∆q 6 = ∆p, called “squeezed state” Generally don’t have ∆N = N 1 /^2
Useful for precision interferometry:
Generate squeezed states in nonlinear crystals Rather difficult to achieve
Local expert: Olivier Pfister
Can have coherent state with α = 0
Then 〈N 〉 = 0: no photons present Called vacuum state
Electric field also zero on average But still have fluctuations ∆q = ∆p = 1/2:
E
t
Fluctuations called vacuum noise Help explain spontaneous emission 21
Another possible state: Fock state
Has definite energy (N + 1/2)ℏω → mode contains N photons
Both ∆q and ∆p large, = (^12)
E
t
Note vacuum state is also a Fock state
Most common nonclassical source: “Parametric down conversion”
Use special crystal with nonlinear interactions
Can “split” one photon into two: ω 0 → ω 1 + ω 2 with ω 0 = ω 1 + ω 2 (conserve energy) k 0 = k 1 + k 2 (conserve momentum) k 1
k 2
k 0
25
Input pulse (ω 0 ) in coherent state
Produces output pulse of form
Ψout =
∑ n
cnΨn(k 1 )Ψn(k 2 )
where Ψn(k) is Fock state for mode k
Typically operate with c 0 ≈ 1, c 1 small, higher c’s negligible
Then usually get nothing, but sometimes get pair of single photons
Polarization depends on crystal setup
possible to produce state √^1 2
One way:
k 1 k 0
k 2
Crystals thin, can’t tell where photons emitted
27
Then say modes are entangled quantum states not separable
Gives interesting effects:
Before measurement, total field state is
√^1 2
(aX 1 Y 2 X 3 + aY 1 X 2 X 3 + bX 1 Y 2 X 3 + bY 1 X 2 Y 3 )
Rewrite by adding and subtracting many terms:
1 23 /^2
( aY 1 X 2 X 3 + aY 1 Y 2 Y 3 + bX 1 X 2 X 3 + bX 1 Y 2 Y 3 +aY 1 X 2 X 3 − aY 1 Y 2 Y 3 − bX 1 X 2 X 3 + bX 1 Y 2 Y 3
+aX 1 X 2 Y 3 + aX 1 Y 2 X 3 + bX 1 X 2 Y 3 + bY 1 Y 2 X 3
−aX 1 X 2 Y 3 + aX 1 Y 2 X 3 + bX 1 X 2 Y 3 − bY 1 Y 2 X 3
)
31
This factors into
1 23 /^2
[ (aY 1 + bX 1 )(X 2 X 3 + Y 2 Y 3 ) +(aY 1 − bX 1 )(X 2 X 3 − Y 2 Y 3 )
+(aX 1 + bY 1 )(X 2 Y 3 + Y 2 X 3 )
−(aX 1 − bY 1 )(X 2 Y 3 − Y 2 X 3 )
]
or 1 2
[ (aY 1 + bX 1 )ΨA + (aY 1 − bX 1 )ΨB
]
When Bob makes measurement, wavefunction collapses
Then Alice’s photon in state related to Υ
Bob knows result of his measurement
Calls Alice on phone and tells her how to change her state to Υ (easy using λ/2 and λ/4 plates)
Now Alice has state Υ indistinguishable from original photon 3 33
If we could do this with 10^23 atoms instead of one photon, could teleport a mouse
Teleportation theory: C. H. Bennett et al. Phys. Rev. Lett. 70 1895 (1993)
Some experiments: D. Bouwmeester et al. Nature 390 575 (1997) T. C. Zhang et al. Phys. Rev. A 67 033802 (2003) M. D. Barrett et al. Nature 429 737 (2004)