ana maria rey - solvay institutes...band (or mott) insulator clock but….. •for many-body physics...
TRANSCRIPT
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Solvay Workshop on quantum simulation with cold matter
and phonons, February 8-11, 2016
Ana Maria Rey
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The JILA Sr team:Theory:
Jun Ye
V. Gurarie, R. Kaiser, S. F. Yelin, M. D. Lukin
J. Schachenmayer M. Wall
B. Zhu
S. Syzranov
X. Zhang
S. Bromley
M. Bishof
T. Nicholson
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A TALE OF TWIN ELECTRONS
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Many-body
Physics
Optical AEA
Clock
1S0 (g)
3P0 (e)Dn0~ mHz
n0=5x1014 Hz
87Sr lifetime ~ 102 sec
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10-17
10-16
10-15
10-14
10-13
10-12
10-11
10-10
Fra
ctio
na
l F
req
ue
ncy U
nce
rta
inty
201020001990198019701960
Year
Cs Beam / Cs Fountain Ion Clock Sr Optical Lattice Clock Yb Optical Lattice Clock
Achieving this
100x faster
than other clocks
Sr: lowest
uncertainty in atomic
clocks:
6.4 x 10-18
Bloom et al., Nature 506, 71 (2014).
Now:
2.1 x10-18
Nicholson et al, Nat. Com., 6, 6896( 2015)
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Band (or Mott) Insulator clock
But…..
• For many-body physics
– Single-site control & manipulation
– SU(N) two orbital magnetism
• For metrology• High accuracy at highest density
• All degrees of freedom at quantum level
• No contact interaction for shifts
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𝑒𝑖𝑘𝑟
𝑘𝑟Optical dipole moment
~ 10-4 – 10-5 Debye
Sr clock: the next systematic uncertainty – collective dipolar couplings
We need to understand long-range dipolar coupling !
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Communication channel dipolar interactions: exchange of virtual
photons.Instantaneous: r « l elastic
3
2
12
||
)cos31(
rV
dd
=
12
21 dddd VddH =
r 0.5 mm l~10 cm
Nature 501, 521 (2013).
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Retardation effects need to be consider when: ζab = k0 rab ~1
a
b
0
0
g:elasticf: Inelastic
superradiance
ζab =0.1, 0.5 1
k0: photon wave-vector
d: dipole momentNatural linewidth Γ0 =𝑘03𝑑2
3𝜋ℏ𝜖0
H 𝒓𝑎𝑏 = 𝑔 𝒓𝑎𝑏 + i 𝑓 𝒓𝑎𝑏
ζab =0.1, 0.5 1
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--Include both elastic and dissipative interactions
far-field physics A(r),B(r)→→𝑒𝑖𝑘0𝑟
𝑘0𝑟Optical transitions
near-field physics A(r),B(r)→1
𝑘03𝑟3
Microwave transitions
--Include near-field and far-field interactions:
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G𝐢𝐣±𝟐 ∝ e∓2φijdi
±dj±
G𝐢𝐣±𝟏 ∝ e∓φijdi
±djz
Project መ𝐝 in J=0,J=1 manifolds
Gij0 ∝ di
−dj+, di
+dj−, di
zdjz
𝐝 𝒊± = ∓
𝐝 𝒊𝐱 ±𝐢𝐝 𝒊
𝐲
√𝟐
𝜑𝑖𝑗
𝜃𝑖𝑗
10 -1
J=0
1 0 -1
J=0
J=1J=1
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𝐻𝒅𝒅±𝟐 ∝ 𝐬𝐢𝐧𝟐𝜽𝒆∓𝒊𝟐𝝋(𝒅𝒊
±𝒅𝒋±)
Conservation of total angular momentum: Coupling spin and motional degrees of freedom
Einstein De-Hass effect
Various proposals to see the effect in bosonic magnetic atoms.• Vortex formation: Santos, Ueda
Not seen yet.• Demagnetization: Laburte-Tolra, Pfau
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𝑯𝒆𝒇 =
𝑖𝑗𝜎�
𝐺𝑖𝑗𝝈𝝈 𝑏𝑖,𝜎
† 𝑏𝑗𝜎
Dilute: most particles in Ji=0: vacuum
An excitation
Excitation can propagate even for pinned
particles in a lattice while flipping their spin
Jj
J
𝑏𝑖,𝝈†
=| Ji=1, 𝜎 = ±1,0 |Ji=0,0ۦ
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𝒌𝟎𝒂 ≪ 𝟏
ℎ 𝒑 ~ 𝜉 𝒑 𝐼 + 𝑣⊥(𝐾𝑅)( ො𝜎𝑥𝑝𝑥 ො𝜎𝑦𝑝𝑦) 𝑣∥(𝐾𝑅) ො𝜎𝑧𝑝𝑧
𝒒 = 𝒑 + 𝑲𝑅
𝑎𝑞𝑥
𝑎𝑞𝑧
𝑎𝑞𝑦
𝜋−𝜋
−𝜋
𝜋
−𝜋
𝜋
B
pz=0px=0
q
q 𝑎𝑞𝑦
𝑎𝑞𝑥
𝑎𝑞𝑧
𝑎𝑞𝑦
Po
pu
lation
s=
1
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Weyl fermions are fundamental massless particles with a definite handedness that were first predicted by Hermann Weyl back in 1929, but they have never been observed in high-energy experiments.
Recently found in solid materials (TaAs --Princeton & Beijing--, Photonic crystals –MIT--)
Naturally appear in excitations of dipolar systems
Possible issues:
Disorder: perfect system requires
unit filling
Dissipative process from dipolar
interactions: radiative dipoles
Indication that Weyl points survive
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• Mott Insulator of Sr atoms
• Trapped in a magic wave lattice
B. Olmos, et al PRL. 110, 143602 (2013)
• G0=2.9 x105 s 1
• a/l=0.1
• Dipole moment d=4.03 D
Jj
J
Near field physics
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Spontaneous decay suppressed at Weyl points:
“subradiance”
Decay orders of magnitude smaller than elastic part
00
0
q
q
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Use momentum resolves Ramsey spectroscopy
2p/DEps
Contrast:
~sin2(
Phase: dispersion
time
p
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• Ideal: a/l«1, n=1 • a/l~0.1 n=1
• a/l«1, n=0.99 • a/l«1, n=0.93
G G
GG
pz
py
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1S0
1P1
3P2
1
0
Sr level structure: weak and strong interactions
698 nm G0/2p = 1 mHzClock transition
Two simple transitions providing
strong and weak dipole interactions ∝ Γ0Γ0blue
Γ0red ~1000
Temperature ~ 1mK , Doppler broadening ~ 50 kHz
Negligible for the blue transition, but important for the red transition
461 nmG0/2p = 32 MHz
689 nmG0/2p = 7.5 kHz
Figure 1: (a) The experimental scheme and concept. We weakly excite the strontium atoms with a
linearly polarized probe beam and measure the fluorescence with two detectors, one in the forward
direction, x , and the other almost in the perpendicular direction, z. We probe two different J = 0
to J’ = 1 transi tions. The first transition is a 1S0−1P1 blue transition with a natural l inewidth of
Γ = 32 M Hz and the second is a 1S0−3P1 red transition with Γ = 7.5 kHz. (b) In the coherent
dipole model photons are shared between atoms. When the Doppler broadened linewidth becomes
comparable to the natural l inewidth, dephasing must be considered. A t our ⇠ 1µK temperatures the
Doppler broadening is ⇡ 40 kHz meaning motional effects are important only for the red transition.
(c) The 3D intensity distribution predicted for a blue probe beam. The coupled-dipole model
predicts a strong 103 enhancement of the forward intensity compared to other directions and a finite
fluorescence along a direction parallel to the incident polarization. The speckled pattern is due to
randomly positioned atoms and can be removed by averaging over multiple atom configurations.
22
Figure 1: (a) The experimental scheme and concept. We weakly excite the strontium atoms with a
linearly polarized probe beam and measure the fluorescence with two detectors, one in the forward
direction, x , and the other almost in the perpendicular direction, z. We probe two different J = 0
to J’ = 1 transi tions. The first transition is a 1S0−1P1 blue transition with a natural l inewidth of
Γ = 32 M Hz and the second is a 1S0−3P1 red transition with Γ = 7.5 kHz. (b) In the coherent
dipole model photons are shared between atoms. When the Doppler broadened linewidth becomes
comparable to the natural l inewidth, dephasing must be considered. A t our ⇠ 1µK temperatures the
Doppler broadening is ⇡ 40 kHz meaning motional effects are important only for the red transition.
(c) The 3D intensity distribution predicted for a blue probe beam. The coupled-dipole model
predicts a strong 103 enhancement of the forward intensity compared to other directions and a finite
fluorescence along a direction parallel to the incident polarization. The speckled pattern is due to
randomly positioned atoms and can be removed by averaging over multiple atom configurations.
22
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Coherent dipole coupling: Probe model
Motional effects: Frozen particles (blue)
No lattice: Random position, far field
Dipolar effects: Intensity, line broadening and line center shift
First test bed experiments at JILA
TOF Peak density (cm-3) ODav ka
1ms 1.5x1012 21 11
25ms 1.5x1011 4.3 25
Measure: forward and transverse fluorescence
Vary probe laser polarization
Tune density and optical depth by time
of flight
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Coherent dipole model
Steady-state
𝑯𝒆𝒇 =
𝑗𝜎
(Ω𝑗𝜎𝑏𝑗,𝜎
† + ℎ. 𝑐 ) +
𝑗𝜎
Δ𝝈𝑏𝑗,𝜎† 𝑏𝑗𝜎 +
𝑗𝑛𝜎�
𝐺𝑗𝑛𝝈𝝈𝑏𝑗,𝜎
† 𝑏𝑛𝜎 Weak driving field
Ω ≪ Γ0
Driving Laser Detuning Dipole Coupling
forward
fluorescence:
Coherent emission
Fluorescence at far-field
𝑏𝑗𝜎 =Ω𝜎𝑒𝑖𝑘0𝑥𝑗
2(Δ𝜎 + 𝑖Γ0/2)+
𝑛≠𝑗�
𝐺𝑗𝑛𝜎𝜎 𝑏𝑛𝜎
𝑖(Δ𝜎 + 𝑖Γ0/2)
𝑏𝑖,𝝈†
=| Ji=1, 𝜎 = ±1,0 |Ji=0,0ۦ
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Forward fluorescence intensity
Narrow interference cone shows phase
coherence, wavelength dependentFigure 2: Forward Scatter ing. (a) Comparison of forward scattering intensity versus angle using
a red and blue probe beam. We use the setup shown in the inset to block the probe beam. After
interacting with the atoms the probe beam is focused using a lens, which also collimates the flu-
orescence from the atoms. We block the probe beam using a beam stopper, which we translate
perpendicular to the probe beam to change the angular range of fluorescence collected by the de-
tector, characterized by the angle (✓) between x and the edge of the beam stopper (see Methods).
The measured intensity, I x,0 (✓), for each probe beam is normalized to the intensity at ✓max = 7.5
mRad. The dephasing caused by motion reduces the forward intensity peak for the red transition.
(b) Comparison of intensity in the forward direction, I x , versus intensity in the transverse direc-
tion, I z. Both arevaried by changing N . All measurements aremadeat ✓= 2 mRad (arrow in (a))
and normalized to the intensity, I x,0, for the atom number used in (a). (c) Linewidth broadening in
the forward direction measured by scanning the blue probe beam frequency across resonance. Ex-
ample lineshapes for different optical depths are shown in the inset. Two different atom numbers
areused, N = 1.7(2) ⇥107 (blue squares) and N/ 4 (cyan triangles). The dashed line representsΓ
for reference. All solid curves are based on the full theory of coupled dipoles and the band in (c)
is for a± 20% atom number uncertainty. All errorbars are for statistical uncertainties.
23
θmax=7.5 mRad
Δ𝜃~1/𝑘0𝑅⊥
𝑅⊥: cloud size perpendicular to k0
I~|Ω𝜎|𝟐
|Δ|2+(Γ0/2)2 (𝑁 + 𝑁2 𝑒−|𝒌𝑠−𝒌0|
2𝑅⊥2)
Collective enhancement of forward
fluorescence
Coherent dipole modelExperiment
Well captured by coherent dipole model
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Figure 2: Forward Scatter ing. (a) Comparison of forward scattering intensity versus angle using
a red and blue probe beam. We use the setup shown in the inset to block the probe beam. After
interacting with the atoms the probe beam is focused using a lens, which also collimates the flu-
orescence from the atoms. We block the probe beam using a beam stopper, which we translate
perpendicular to the probe beam to change the angular range of fluorescence collected by the de-
tector, characterized by the angle (✓) between x and the edge of the beam stopper (see Methods).
The measured intensity, I x,0 (✓), for each probe beam is normalized to the intensity at ✓max = 7.5
mRad. The dephasing caused by motion reduces the forward intensity peak for the red transition.
(b) Comparison of intensity in the forward direction, I x , versus intensity in the transverse direc-
tion, I z. Both arevaried by changing N . All measurements aremadeat ✓= 2 mRad (arrow in (a))
and normalized to the intensity, I x,0, for theatom number used in (a). (c) Linewidth broadening in
the forward direction measured by scanning the blue probe beam frequency across resonance. Ex-
ample lineshapes for different optical depths are shown in the inset. Two different atom numbers
areused, N = 1.7(2) ⇥107 (blue squares) and N/ 4 (cyan triangles). Thedashed line representsΓ
for reference. All solid curves are based on the full theory of coupled dipoles and the band in (c)
is for a± 20% atom number uncertainty. All errorbars are for statistical uncertainties.
23
Forward Direction
: cloud size perpendicular to k0
Atom#
N ~1.7×107
¼ atom number
Significant linewidth with increasing OD
Coherent dipole modelExperiment
Collapse as a function of OD
Shadow: 20% atom number uncertainty
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Coherent dipole model
Weak driving field
Ω ≪ Γ0For one dipole emission
parallel to polarization is
forbidden
But is allowed for many-dipoles:
𝑏𝑗𝜎 =Ω𝑗𝜎
2(Δ𝜎 + 𝑖Γ0/2)+
𝑛≠𝑗�
𝐺𝑗𝑛𝜎𝜎 𝑏𝑛𝜎
𝑖(Δ𝜎 + 𝑖Γ0/2)
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Transverse fluorescence Experiment agree well with “spin-orbit” coherent dipole model
Anisotropy of dipole-dipole interactions: polarization and geometry
dependent linewidth and intensity
Fluorescence intensity and linewidth are collective enhanced for the forbidden
polarization
Linewidthy:Allowedz: Forbidden
Intensity Ratio
Coherent dipole modelExperiment
y:Allowed
z: Forbidden
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Transverse fluorescence
Coherent dipole model prediction:
frequency shift on the order of
Γ0𝑛𝑘0−3
Frequency shift agrees with theory
What about the red transition? Motion effects not negligible
Doppler broadening ~ 50 kHz Γ0~ 7.5 kHz
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𝑏𝑗𝜎 =Ω𝑗𝜎
2(Δ𝜎 + 𝛿𝑗 + 𝑖Γ0/2)+
𝑛≠𝑗�
𝐺𝑗𝑛𝜎𝜎 𝑏𝑛𝜎
𝑖(Δ𝜎 + 𝛿𝑗 + 𝑖Γ0/2)
Coherent dipole model
Lowest order correction from motion:
atomic motion accounted by as random
detunings
Void-profile line shape: Convolution Gaussian and Lorentzian
: Doppler width
: detuning of probe laser
: dipole-dipole interaction
random detuning for each atom
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Forward fluorescence intensity
Δ𝜃~1/(𝑘0𝑅⊥)
Coherent dipole modelExperiment
Interference cone: k0 dependence
Motion decreases phase
coherence
Well captured by coherent dipole
model
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Transverse fluorescence intensity
Ω/Γ0~0.3 − 0.6Coherent dipole model+ random detunning
Experiment: T. Ido, et al PRL 94, 153001(2005).
Weak transition: Large frequency shift exceeding theory prediction
Other effects caused by motion (such as recoil, momentum diffusion), nonlinearity,
short-range physics? Red transition: Complex regime
Single photon recoil energy ~ linewidth~ Rabi frequency
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Progress towards quantum degeneracy
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Progress quantum degeneracy: 87Sr lab @JILA
5 x 105 atoms at 1.5 mK(crossed dipole trap) ~ 104 atoms, T< 80 nK, T/TF ~ 0.3
for each nuclear spin component(after evaporation in dimple)
Preliminary, January 2016
Then loaded in a lattice
TOF
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Alkaline earth atoms: A great vista ahead !
Super-exchange
Spin-orbital coupling
Retarded dipolar interactions P-wave
magnetism
Complexity
Temperature SU(N)Mott-insulator
Su(N)Heisenberg:Chiral spin liquid?
Su(N)Lattice Kondo
Su(N)Dynamical gauge fields
SU(N) orbitalmagnetism
P-wave su(N)magnetism
Weyl quasiparticles
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