Transcript Document

Experiments with Trapped
Potassium Atoms
Robert Brecha
University of Dayton
Outline
Basics of cooling and trapping atoms
Fermionic and bosonic atoms - why
do we use potassium?
Parametric excitation and cooling
Sympathetic cooling and BEC
Co-workers and Affiliations
Giovanni Modugno – LENS
Gabriele Ferrari – LENS
Giacomo Roati – Università di Trento
Nicola Poli – Università di Firenze
Massimo Inguscio – LENS and Università
di Firenze
In the Lab at LENS
Motivations for Trapping Atoms
Fundamental atomic physics measurements
Condensed matter physics with controllable
interactions (“soft” condensed matter)
Tabletop astrophysics – collapsing stars,
black holes, white dwarfs
Quantum computing
Atomic Cooling
Laser photons
Physics2000 Demo
Cooling Force
Random emission directions
 momentum kicks
 retarding force
Force = (momentum change per absorbed photon)
 (scattering rate of photons)
(Depends on intensity, detuning, relative speed)
Force is not position-dependent  no permanent
trapping
Laser Cooling and Trapping
Magnetic Field
Coils
(anti-Helmholtz)
Circularly
polarized
laser beams
Far Off-Resonance Trap (FORT)
One disadvantage of MOT – presence of magnetic
fields; only certain internal states trappable
Solution – Use all-optical method
Laser electric field induces an atomic dipole
  E
Interaction potential of dipole and field:
U dipole
1
1
   E  
Re   I
2
2 0c
FORT Trapping Potential
Standing-wave in z-direction, Gaussian radially
U  r , z   U 0 cos 2 kz exp  2r 2 / w2 
Oscillation frequencies:
A  2 2U 0 / M t2
R  4U 0 / Mw02
1

2 2
U

m

x 

2


450 mK
Fermions
vs.
Bosons
Spin-1/2
Integer spin
State-occupation limited
Gregarious
f 
1
e
   m 
1
Do not collide*
f 
1
e
   m 
Collide
1
Fermions vs. Bosons
Ensher, et al., PRL 77, 4984 (1996)
Fermionic occupation
probabilities
Bosonic ground-state
occupation fraction
Potassium
Three isotopes:
39K (93.26%)  boson
40K (0.01%)  fermion
41K (6.73%)  boson
Potassium Energy Levels
FORT Experimental Schematic
Absorption beam
MOT: 5 × 107 atoms
T ~ 60mK
FORT: 5 × 105 atoms
T = 80 mK
Absorption Image from FORT
N = 5 × 105 atoms
n = 5 × 1011 cm-3
T = 50 – 80 mK
dT/dt = 40 mK/s
r = 2 × 1 kHz
a = 2 × 600 kHz
U0 = 300 - 600 mK
450 mK
Elastic Collisions
t = 10(3) ms
s = p/2tnu
 41011cm2
at = 169(9)a0
Inelastic Collisions
Frequency Measurements
“Parametric Excitation”
Driving an oscillator by modulating the
spring constant leads to resonances for
frequencies 20/n.

0
Here we modulate
the dipole-trap
laser by a few
percent
Parametric Resonances
1.8a
2
a
Parametric Heating ...
and Cooling
2
Tex = 10 ms
 = 12 %
a
1.8a
Tex = 2 ms
 = 12 %
Trap Anharmonicity
Cooling by Parametric Excitation
Selective excitation of high-lying levels
 forced evaporation
Occurs on a fast time-scale
Independent of internal atomic structure
 works on external degrees of freedom
Somewhat limited in effectiveness
The New Experiment
Transfer Tube - MOT1 to MOT2
Sympathetic Cooling
Use “bath” of Rb to cool a sample of K atoms
Goal 1 – Achieve Fermi degeneracy for
40K atoms
Goal 2 – (After #1 did not seem to work)
Achieve Bose-Einstein condensation
for 41K
Some Open Questions
Do K and Rb atoms collide? (What is the
elastic collisional cross-section?)
Do K and K atoms collide? Is the
scattering length positive (stable BEC)
or negative (unstable BEC at best)
Some Cold-Collision Physics
Scattered particle wavefunction is written as a sum
of “partial waves” with l quantum numbers.
For l > 0, there is repulsive barrier in the corresponding
potential that inhibits collisions at low temperatures.
For identical particles, fermions have only l-odd
partial waves, bosons have only l-even waves.
 Identical fermions do not collide at low temperatures.
Rubidium Energy Levels
87Rb
F´= 3
267 MHz
F´= 2
F´= 1
F´= 0
157 MHz
72 MHz
F=2
6835 MHz
F=1
780 nm
(4×108 MHz)
Rubidium Ground-State
“Low-field-seeking states”
Apply a B-field:
mF = 2
F=2
6835 MHz
mF = -1
F=1
BEC Procedure
Trap 87Rb, then 41K in MOT1
Transfer first Rb, then K into MOT2
Now have 107 K atoms at 300mK and
5×108 Rb atoms at 100mK
Load these into the magnetic trap after preparing in
doubly-polarized spin state |F=2,mF=2>
Selective evaporative cooling with microwave knife
Check temperature (density) at various stages (a
destructive process)
QUIC Trap
Figure by Tilman Esslinger, ETH Zurich
QUIC Trap Transfer
Quadrupole
field
Magnetic trap
field
Figure by Tilman Esslinger, ETH Zurich
Microwave “Knife”
(Link to JILA group Rb BEC)
Temperature (mK)
Temperature and Number of Atoms
100
10
1
Rb
4
Atom Number (10 )
10000
1000
100
K
10
1
0.1
1
10
Microwave Treshold (MHz)
Potassium BEC Transition
A
B
C
(Link to JILA group Rb BEC)
Optical Density Cross-section
Condensate
Mixed
Thermal
Absorption Images
87 Rb
41 K
40mK
1mK
2mK
0mK
Rb density remains K density increases
constant
100x
Elastic Collisional Measurements
Return to parametric heating (of Rb) and
watch the subsequent temperature increase
of K.
tequil   3n v s 
1
Determined from absorption images
Elastic Collisional Measurements
Potassium temperature
after parametrically
heating rubidium
Temperature dependence of
elastic collision rate (Is a >0
or is a < 0?)
Ferrari, et al., submitted to PRL
Double Bose Condensate
Future Directions