accélération d’atomes ultra-froids : vers une mesure …€¦ · accélération d’atomes...
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Accélération d’atomes ultra-froids :vers une mesure de h/M et de α
Laboratoire Kastler Brossel, Paris (ENS, CNRS, UPMC)
BNM - Institut National de Métrologie, Paris (CNAM)
P. Cladé, R. Battesti, S. Guellati, C. Schwob,B. Grémaud, F. Nez, L. Julien, F. Biraben
Determination of the fine structure constant
Rydberg constant(7 × 10-12)
(2 × 10-10)
atomic massproton mass
(4.6 × 10-10)
proton masselectron mass
h/MA α
Ae
p
p
A
Mh
mm
mM
cR
×××= ∞22α22
21 αcmchR e=∞
Hydrogen atom
• measurement of h/MA at 6 × 10-8
determination of α at 3 × 10-8
• total dispersion of α measurements: 2.4 ×10-7
(CODATA 1998)
Measurements of αCodata98
quantum Hall effectCodata02
muonium
h / M(neutron)h / M(Cs)
QED
h / M
Solid-statephysics
g – 2 of the electron
α-1
2e/h RK=h/e2=µ0c/2α
s.h.f
ae = f (α/π)
Mv=h/λatomic interferometry
10-7
Γ’ (lo)p,h-90
137,035 990 137,036 000 137,036 010
The principle of the experiment :measurement of the atomic recoil
velocity
a
b
ωħk MA MA vrecoil
AMkh
=recoilv 16v87 −⋅≈ smmRbrecoil
measurement of vrecoil and k ⇒ h/MA
Raman transitions (1) : velocity selection
MA
•coherent momentum transfert
k1 k2
v
e
ω1ω2
ab
δ
∆
r
( )21v kkM A −=∆ h
( ) ( )A
ab Mkkkkr 2
v22
212121
rr
hrrr −
−−⋅−−−= ωωωδπ
( )rab kkkkr vv2 and 0 2121 ++≈−⇒−≈== ωωωδ
•control of δr control of v•two hyperfine levels involved velocity selection and measurement
Raman transitions (2) : acceleration of atoms
p
E=p /2M2
2hk 4hk 6hk
ω 1 ω 2
δ’=2kvδ’=6kvδ’=10kvr
r
r
ω , k11 ω , k22
ω1 ω2
a
∆
MA
e
1)(2N2kvδ r −=′
bδ’
Acceleration ⇔ Bloch oscillations
87Rb
δR
D2780 nm
5S1/2
5P3/2
F=2F=1
∆Temporal sequence
initial velocitydistribution
subrecoilvelocity
class selection
coherentacceleration
measurementof the final
velocitydistribution
F=2
F=1
F=2→F=1 F=1→F=2
MOT andoptical molasses
«Raman» «Bloch» «Raman»
detectiontime of flight
t
blow away beam
12 ννν −=sel fixed '12 ννν −=meas tuned
Horizontal acceleration of atoms (1)
221 2).(221
cMhN
MkkkN
A
RB
ABlochmeassel
ννπ
νν =−=−hrrr
RamanBloch g
r
For , atoms miss the detection area.4≥N
MA
Problem !
Detection chamber Probe
Horizontal acceleration of atoms (2)
F=2→F=1 F=1→F=2
MOT andoptical
molasses
«Bloch»initial acceleration
«Raman»
«Bloch»acceleration
«Raman»
detectiontime of fight
t
gr
BlochRaman MA
Detection chamber Probe
Experimental curves (50 oscillations)to reduce systematic errors alternate and symmetric accelerations
in horizontal opposite directions
δ0= + (1 506 799,5 ± 3,1) Hz
νmeas – νsel (MHz)1.506 1.507
δ0= - (1 506 531,2 ± 3,1) Hz
-1.507 -1.506νmeas – νsel (MHz)
deduced recoil : 15 066, 690 (23) Hz
«+100 vr» «-100 vr»
uncertainty: 6105,1 −×
~ 1 kHz
Horizontal geometry : results
137,035930 137,035970 137,036010
QuantumHall effect
Muoniumge-2
h/mnh/MCs
h/MRb
α−1
CODATA 02
Γ’ (lo)p,h-90
h/MRb relative uncertainty : 4.2 × 10-7
Gap between our valueand the expected one : 6.1 × 10-7
χ2 = 99 for 43 measurements.
η (per Bloch oscillation) = 99.5%
R.Battesti et al, Phys. Rev. Lett. 92, 253001 (2004)
Vertical configurations (1)
Vertical acceleration with Bloch oscillations
Bloch Raman
MAgr
chNgtMM AAν2v ×−=∆
( )ν2
v cN
gtMh
A
∆−=
differential measurement («up» and «down» accelerations)independent of g
Vertical configurations (2)
Vertical beams so that the force due to the Raman transitions exactly compensates gravity
Bloch Raman
MAgr
atoms submitted to a verticalstanding wave
E
p
ν ν
-ħk + ħk
In the standing wave, theatom oscillates at the sameplace with the frequency:
kgM A
Bh2
=ν
Present work: vertical geometry
N/(N+N)
212
vertical acceleration of the atoms
• 80 recoil transfers
• careful investigations of experimental limiting factorsand systematic effects
observation of Bloch oscillations in the vertical standing wave
Experimental curves in vertical geometry
0
0,05
0,1
0,15
0,2
0,25
0,3
0,35
0,4
0,45
0,5
-2110500 -2110000 -2109500 -2109000 -2108500 -2108000
δ0= - (2 109 260,6 ± 1,7) Hz
center of the curve: 1,7 Hz 9000vr in 10 minutes80 oscillations
( )Hzmeassel νν −
~ 1 kHz
Inverting the sens of photons: a way to reduce systematic effects
6102 −×(h/M)relative
e
ν1ν2
ab
with ∆(x,t) a systematic effect (light shift, quadratic Zeeman effect (mF=0)..)
( ) [ ])),((2vmeas12 txkk HFS ∆+−=⋅− νδπ
( ) [ ])),((2v'meas21 txkk HFS ∆+−′=⋅− νδπ
( )txh
EEHFS
ab ,∆+=− ν
Raman «plus»
MA
ν 1 , k 1
ν2 , k2
v
ν 1 , k 1
Raman «minus»
MA
ν2 , k2
'v
( )δδπ−′=
k2vmeas independent of ∆(x,t)
kkk =≈ 21
Zeeman effect
-B0 -B0B0
-B0
B0
6102 −×(h/M
)
ħk2 ħk1
ba
MAħk2 ħk1
v
MA ħk2ħk1
v
∆Zee=K(2)B2 ; K(2) ~ 514 Hz/G2
6102 −×
500mG
(h/M
)
∆Zee(zselec)-∆Zee(zmes)~ B0 ∇B ∆z
Applied magnetic field(quantification axis) Residual gradiant
(50mG/cm)
Vertical motion(~1cm)
Zeevδ ∆=⋅rrr
)k-k( 12
Zeevδ ∆=⋅rrr
)k-k( 21
∆HFS+∆Zee
B0
ProspectsFuture : new cell + slow atoms source● better vacuum● better efficiency to load the MOT● magnetic shielding
µ-metal boxes
2D MOT
3D MOT +molasses
Uncertainties (1)
Lasers wavelenghtsuncertainty of 10 MHz on the Raman and Bloch laser frequencies
5.2 × 10-8
Angle between the different laser beamsestimation based on the fiber diameter (5 µm) and the focal lenghts (40 mm) → 63 µrd 2 × 10-9
RCWave fronts curvature
radius of curvature RC > 20 m
vertical motion in 20 ms ∼ 2 mm → θ ∼ 10-4 rd 5 × 10-9
Uncertainties (2) 5P3/2
F=2
∆
F=1
ω1ω2
ωHFSdifferential effect (I1=I2 and π pulse):
8 × 10-6τ ∼ 1.6 ms ∆ ∼ 340 GHz → 26 Hz
differential effect between the measurements +/- 50 oscillations 8 × 10-8
Light shifts
( ) ⎟⎟⎠
⎞⎜⎜⎝
⎛+∆
+∆
Γ==
HFSs
III
Fωπ
δ 212
8211
( ) ( )∆
−==−= HFSFF ωτ
δδ 212(N=50)
Magnetic fields fluctuations
transition between mF = 0 sub-levelsmagnetic field of 150 mG → 9,6 HzFluctuations [(Bsel − Bmes)+50 − (Bsel − Bmes) − 50] ∼ 1mG → 0,13 Hz
4 × 10-8
Comparison with S. Chu’s experiment
F=2
F=1
π
π
F=2
OBOB
Rubidium
π/2π
π
π/2
F=4
F=3Césium
vertical geometry
atomic interferometry : fringes width of 8 Hz (500 Hz in ourexperiment)
transfert by resonant adiabatic passages betweenthe F=3 and F=4 levels: efficiency 94% (99,5 % in our experiment)
interferometry: sensitivity to gradients (magnetic fields, intensity…)Bloch oscillation in the gravity field: sensitivity to gravity fluctuations