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PHY 411 / 412 / 436
QUANTUM OPTICS
Prof. Mark Fox
A sub-module of the
ASPECTS OF MODERN PHYSICS module
Spring Semester
10 lectures
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Module Synopsis
Course text:Fox, M.
Quantum Optics, an IntroductionOxford University Press, 2006
I. Laser Cooling & Bose-Einstein Condensation(Lectures 1-5)
II. Photon statistics (Lectures 6-9)
III. Quantum Information Processing
(Cryptography) (Lecture 10)
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Part I: Laser cooling & BEC
Reading: Fox, Quantum Optics, Chapter 11
Other useful books
Foot, Atomic Physics, Oxford, 2005, Chapters 9-10Demtrder, Atoms, Molecules and Photons, 12.1Haken & Wolf, Physics of Atoms & Quanta, 22.6, 23.11
Topics to be covered Techniques for laser cooling of atoms
Theoretical limits on the temperature Bose-Einstein Condensation of atoms
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Useful resources
Web resources for laser cooling & BEC:
http://nobelprize.org/nobel_prizes/physics/laureates/1997/
http://nobelprize.org/nobel_prizes/physics/laureates/2001/
http://www.lkb.ens.fr/recherche/atfroids/tutorial/index2.htm *http://www.colorado.edu/physics/2000/bec/
http://bec01.phy.georgiasouthern.edu/bec.html/
* in French !
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Atomic temperatures
oven, temp T
2
B
2
B
1 33 D
2 2
1 1
1 D2 2x
mv k T
mv k T
=
=
Principle of equipartition of energy:kBTper degree of freedom
atomic beam
B3mp
k Tv
m=
vmp = most probable velocity
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Doppler cooling mechanism
0Lab
sorption
frequency
0
absorption
frequency
0a
bsorption
frequency
2
v
v
v
(a)
L
L
(b)
(c)
absorption only for case (b) laser must be tuned below
the transition frequency must be tuned as
atoms cool
velocity = vx
atom laser beam
L = 0 +
=0
xv
c
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Absorption-emission cycles
t= 0
t=
1. Laser photon impinges on atom
2. Atom promoted to excited stateat t = 0
3. Atom re-emits at mean time in a random direction
Average momentum kick of (h/) in time d
d
x x
x
p p hF
t
= =
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Limits on Doppler cooling
stop
min stop
2
min
B min
min
B
initial
per cycle /
22
~
2
x x
x
x
x
p muN
p h
mut Nh
m u
d h
k T h v
Tk
=
=
Number of absorption
- emission cycles tostop atom,time to do so, anddistance travelled
Doppler limit temperature
= 1 / 2 (natural linewidth) Factor of 2 from stimulated
emission
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Sisyphus Cooling
Sisyphus
Laser cooling experiments using counter-propagatingbeams worked better than expected !
Tfinal < TDoppler
Caused by the Sisyphus cooling effect
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Mechanism of Sisyphus cooling
Energy
MJ = 1/2
MJ = +1/2
abso
rptione
mission
x
excited state: J= 3/2
Position
ground state: J= 1/2
http://www.lkb.ens.fr/recherche/atfroids/tutorial/index2.htm
7. LE REFROIDISSEMENT DATOMES PAR LASER
counter-propagating
beams createinterference pattern Atomic levels shifted
by the AC-Starkeffect
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Recoil limit temperature
p= h/
2 2
B recoil 2
2
recoil 2
B
1 ( )
2 2 2
p hk T
m mh
Tmk
= =
=
Photon recoil ultimately
limits Twhile atom isundergoing absorption-emission cycles
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Magneto-optic traps
x
y
z
i
i
Magnetic quadrupole:
B (x2 + y2 4z2)1/2
Atomic energy shift:E= gJBBMJ
attractive for MJ
> 0
repulsive for MJ< 0
Optical Molasses6 counter propagating beams
+ magneto-optic trap
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Experimental cooling kit
sodium
oven
tapered solenoid
cooling beam
probe
pulse
molasses
regioncamera
escapin
gatoms
precooling region
Lasers tuned to sodium D2 line (3s2S1/2 3p 2P3/2, 589 nm)
Use tapered solenoid to tune atoms as they cool
Further details in Dr Phillips Nobel Prize lecture:
see http://www.physics.nist.gov/News/Nobel/1997nobel.html
600 C
~2.5 K 40 K
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Temperature achieved
0 10 20 30 400
200
400
600
Laser detuning (MHz)
Temperature
(K)
Doppler limit
Sodium D2 line at 589 nm: = 16 ns
Tmin (Doppler) = 240 K
Tmin (recoil) = 2.4 K
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Ion traps
Cooling
laser
magnetic field
+
+
+
+
trapped ions
Ions easily trapped byelectric & magnetic fields
Two common designs:Penning & Paul traps
Use laser to cool ions to
Doppler limit temperature
Can trap and control singleions: used for quantum
information processing
Penning trap: Bfield traps in (x,y)plane & Efield traps in zdirection
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Bose-Einstein Condensation
Main reference
Fox, Quantum Optics, Chapter 11
Other useful reading
Mandl, F., Statistical Physics, 2nd Edition,Wiley (1988), Section 11.6
Web resources:http://www.colorado.edu/physics/2000/bec/http://nobelprize.org/nobel_prizes/physics/laureates/2001/
http://ucan.physics.utoronto.ca/
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Basic concepts of BEC
1 10 100 1000 100000
1
2
3
4
Temperature (K)
CVpe
rmolecule/kB
3/2 kB
5/2 kB
7/2 kBvibrational
motion rotational
motion
translationalmotion
?
Classical result: CV = kB per degree of freedom
Classical motion freezes out when kBT Equant
Heat capacity
of gas ofdiatomicmolecules
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Quantization of translational motion
Third law of thermodynamics: CV 0 as T 0
Translational motion must eventually be quantized
at sufficiently low T
Most gases liquefy and solidify before quantumeffects observed for the translational motion.(Helium is the exception.) Atoms/molecules in liquidor solid phase are not non-interacting.
Need to get to very low temperatures but with non-interacting atoms/molecules. ie need to cool a gasto very low T without it liquefying.
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Bose-Einstein condensation
From a certain temperature on, the moleculescondense without attractive forces, that is, theyaccumulate at zero velocity. The theory is pretty, butis there some truth to it.A. Einstein, letter to P. Ehrenfest, 29 Nov, 1924
Examples
- superfluid liquid helium TC = 2.17 K- cold atom gas TC 10
6 K
- Cooper pairs in superconductors, neutron stars
- excitons
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Transition temperature
deB
22
BdeB
1/ 3
deBB
2 / 32
CB
1 3~
2 2 2
~ ~3
~3
p hk T
m m
h V
Nmk T
h NT
mk V
=
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Statistical mechanics of BEC
BEC = accumulation of particles in the ground state
Fermions (e.g. spin particles) subject to Pauli
exclusion principle. Can only put one particle in theground state.
Hence only bosons (i.e. integer spin particles) can
undergo BEC.
2 / 32
C B
3/ 2
C
0.0839
( ) 1
h NT
mk V
Tf T
T
=
=
Condensation
temperature
Fraction in
condensed phase
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Atoms: boson or fermion ?
Ions no good for BEC because they repel, sothat high densities are not possible. Hence need
to use neutral atoms.
Electrons, protons, and neutrons are spin fermions
Satom = Selectrons + Snucleus
Nelectron = Nproton in neutral atom.
Hence boson for Nneutron even.
Examples: 4He, 23Na, 87Rb
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Recipe for BEC
magnetic trap
potential
x
Use laser cooling to cool atoms to near Trecoil
Confine atom cloud by using a magneto-optic trap
Turn off laser and reduce potential of trap toinstigate evaporative cooling.
most energeticatoms escape and
temperature goes
down
reduce magnetic field
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Observation of BEC
atomic
gas
resonantlaserlight
t= 0
t= te
free
expansion
D ~ vte
Measure velocity distribution by time of flight
expansion and shadow image technique
shadow of atomic gason screen / camera
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Experimental Results
BEC first observed in 1995 for 87Rb and 23Na
Now observed in many other atomic gases7
Li,1
H,85
Rb,4
He,41
K,133
Cs,174
Yb,52
Cr, Details of experiments from
http://ucan.physics.utoronto.ca/
Significant differences between:
2 / 32
CB
3/ 2
C
0.0839
( ) 1
h NTmk V
T
f T T
=
=
1/ 3CB
3
C
0.94
( ) 1
T Nk
T
f T T
=
=
BEC in free space BEC in harmonic trap
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BEC experimental data
0.2
mm
87Rb
5S1/2 5P3/2
transition at780nm
Cooling with
laser diodes N/V~
2.51018 m-3
TC ~ 170 nK
See Anderson et al, Science269, 198 (1995)
http:/jilawww.colorado.edu/bec
400nK
200nK
50nK
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Atom lasers
1.8 mm
3.9mm
1 mm
Trap is attractive only for MJ= +1/2 states
Apply RF pulse to tip the spin: trap becomes
repulsive and ejects pulses of atoms Interference between two atom pulses provescoherence
See Ketterle, Rev. Mod. Phys. 74, 1131 (2002)
23Na 200 Hz rep rate
10
5
10
6
atoms / pulse
http://cua.mit.edu/ketterle_group/Projects_1997/atomlaser_97/atomlaser_comm.html
Durfee and Ketterle, Optics Express, 2, 299 (1998)