Towards ultracold RbSr ground-state moleculesstrontiumbec.com › StrontiumLab › RbSr ›...
Transcript of Towards ultracold RbSr ground-state moleculesstrontiumbec.com › StrontiumLab › RbSr ›...
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Florian SchreckUniversity of Amsterdam
Towards ultracoldRbSr ground-state molecules
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Many-body systems
www.thepistrophy.com
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Quantum many-body physics
Strong quantum correlations render description difficult.Especially difficult:
Fermionic systems
?Frustrated systems Dynamics
𝑡𝑡
𝑂𝑂
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Quantum simulation (and beyond)
Control everything
…
potential interactions internal state
difficult to studyquantum system
well-controlledultracold systemsimplified model
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Alkaline-earth(-like) elementsYb, Sr, Ca
New ultracold systems
Magnetic atoms Cr, Dy, Er
Ground-state moleculesclosed-shell: KRb, NaK, RbCs,...
open-shell: RbYb, RbSr, YbCs
Rydberg atoms
More interesting interactions
Benefits
• long-range • anisotropic
More internal structure
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Molecules
Richer structure than atomsrotational and vibrational states
Dipole-dipole interactions due to electric dipole moment
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Example: quantum magnetismMagnetism requires spin dependent interactions.
Provided by super-exchange in ultracold ground-state atoms
𝑡𝑡𝑈𝑈
𝑡𝑡
spin dependent interaction
Requires extremely low motional temperature
In dipolar molecules simply provided by spin-state dependent dipole interaction
Requires only low spin temperature
Theory:Micheli et al., nature physics 2, 341 (2006)Gorshkov et al., PR A, 84, 033619 (2011)
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Examples: dipolar gases in 2D
Interlayer Cooper pairing
G. Pupillo et al., PRL 104, 223002 (2010)
Monte-Carlo density distributions in dependence of interaction strength
Bosonic molecules Fermionic molecules
ReviewsM. A. Baranov, M. Dalmonte, G. Pupillo, and P. Zoller, Chem. Rev. 112, 5012 (2012)
M. L. Wall, K. R. A. Hazzard, and A. M. Rey, arXiv:1406.4758
Pikovski, A. et al., PRL 105, 215302 (2010)
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Two paths to ultracold molecules
Atoms Molecules
hot
cold
cool
associate
cool
associate
Path 1
Path 2
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Status
• KRb 0.5 Debye dipole moment Science 322, 231 (2008) Ye, Jin group• Cs2 0 Debye Faraday Disc., 284 (2009) Nägerl group• RbCs 1.2 Debye PRL 113, 205301 (2014) Ferlaino, Grimm, Nägerl gr.• NaK 2.7 Debye PRL 114, 205302 (2015) Zwierlein group
Observation of dipolar spin-exchange interactions with lattice-confined polar moleculesNature, 501, 521 (2013)
Many-body dynamics of dipolar molecules in an optical latticePRL 113, 195302 (2014)
Four systems, all based on alkali atoms:
Ye, Jin group
Challenge
Cooling to quantum degeneracy
First experiments studying magnetism:
Other alkali-alkali molecule experiments being set up by many groups.
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Evaporative cooling
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KRb + KRb K2 + Rb2 + energy
Challenge for evaporative cooling
Chemistry
© m
astil
oade
d.co
m
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Counter measures
© m
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oade
d.co
m
Repulsive molecules in 1D lattice
might allow evaporative cooling to quantum gas
e.g. RbCs, NaK,…
Non-reactive species
Dangerous „sticky collisions“ ?Bohn group, PR A 87, 012709 (2013)
Repulsive van der Waals interactions
Gorshkov et al. PRL 101, 073201 (2008)
Bohn group, PR A 73, 022707 (2006)
Zoller group, PRL 98, 060404 (2007)
Bohn group, PR A 81, 060701(R) (2010)
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RbSr ground-state molecules
unpaired electron
alkali + alkali atom
Our goal
Our group RbSrGörlitz group RbYbGupta, Takahashi groups LiYbCornish group CsYb
So faralkali + alkaline earth atom
only paired electrons
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Repulsive van der Waals interactionsinstantaneous dipole – induced dipole interaction
Can be repulsive in excited state:
evaporative cooling of OH at mK temperatures, Ye group, Nature 492, 396 (2012)
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E
383 G
N=0
N=1
magnetic field
E = 150 V/cm
RbSr energy, neglecting hyperfine structure
repulsive vdW interaction!
Repulsive van der Waals interactions
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0
1
2
3
4
5
6
7
8
9
10
600 800 1000 1200 1400 1600 1800 2000
Ener
gy (µ
K)
preliminary result by John Bohn, JILA, neglecting hyperfine interaction
E = 150 V/cm B = 383 G
RbSr interaction potential
r (Bohr radii)
expectedtemperatureof molecular gas
Evaporative cooling possible?
Repulsive van der Waals interactions
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Experimental realizationRb-Sr mixtures87Rb
N = 1.3 x 105
84Sr
N = 2.3 x 105
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Molecule association
Standard technique
magneto association Sr is non-magnetic magneto association not trivial
Alternative technique
STIRAP association let‘s demonstrate it by creating Sr2
Hutson group, PRL 105, 153201 (2010)
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SchemeBEC
Mott insulator
ramp on optical lattice
associate molecules
BEC
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Molecule association by STIRAP
1S0 + 1S0
1S0 + 3P1
external trap(lattice well)
|e>
Ω1Ω2
|m>
|a>
Γ
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Molecule association by STIRAP
1S0 + 1S0
1S0 + 3P1
external trap(lattice well)
|e>
Ω2
|m>
|a>
Γ
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Molecule association by STIRAP
1S0 + 1S0
1S0 + 3P1
external trap(lattice well)
|e>
Ω1
|m>
|a>
Γ
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Molecule association by STIRAP
1S0 + 1S0
1S0 + 3P1
external trap(lattice well)
|e>
Ω1Ω2
|m>
|a>
|Ψ> = Ω1|m> + Ω2|a>
Γ
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0 20 40 60 80 1000,0
0,5
1,0
L2 L1
Inte
nsity
Time (µs)
Molecule association by STIRAP
1S0 + 1S0
1S0 + 3P1
external trap(lattice well)
|e>
Ω1Ω2
|m>
|a>
Γ
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STIRAP transition
singlet states triplet states
461 nm30 MHz
689 nm7.4 kHz
1S0
1P1
3PJ
698 nmmHz
210671 nm
mHz
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STIRAP transition
singlet states triplet states
689 nm7.4 kHz
1S0
1P1
3PJ210
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L1L2
Result
See also 88Sr2 work by Tanya Zelevinsky, PRL 109, 115303 (2012).
30% conversion efficiency
60µs lifetime
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L1L2
Result
See also 88Sr2 work by Tanya Zelevinsky, PRL 109, 115303 (2012).
30% conversion efficiency
60µs lifetime
What are the limitations?
Can we improve performance?
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Short lifetime of molecules
532 nm (Verdi) used in Innsbruck
1064 nm
A. Stein et al., Eur. Phys. J. D 64, 227 (2011)
Sr2 molecular potentials
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Lifetime in 1064nm lattice
110(25) s lifetime
STIRAP efficiency: 55%
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Lightshift on binding energy
1S0 + 1S0
1S0 + 3P1
|e>
L1
|m>
|a>
228 MHz
compensation beam
75 MHz
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Compensating binding energy shift
1S0 + 1S0
1S0 + 3P1
|e>
L1
|m>
|a>
228 MHz
compensation beam
75 MHz
compensation beam intensity / L1 intensity (%)
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STIRAP with compensation
~50% single pass efficiency
80% single pass efficiency
Inte
nsity
(abr
)
L2 L1 C
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STIRAP with compensation
80% single pass STIRAP efficiency
efficiency increase bycompensation beam
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Why initially lower efficiency?
~50% single pass efficiency
80% single pass efficiency
Inte
nsity
(abr
)
L1 L2 C
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STIRAP parameter dependenceatom number after STIRAP round-trip
|e>
|m>|a>
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What limits STIRAP efficiency?
2) dark state lifetime of 3.5 ms
1) off-resonant scattering of photons on atomic line
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Next goal
RbSr molecules
Sr2 molecules
84Sr87Rb
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Rb-Sr mixture87Rb
N = 1.3 x 105
84Sr
N = 2.3 x 105
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RbSr molecular potentialsZuchowski et al., PR A 90, 012507 (2014)
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RbSr molecular potentialsZuchowski et al., PR A 90, 012507 (2014)
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Photoassociation spectroscopy
88Sr-87Rb 84Sr-87Rb
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Photoassociation spectroscopy
88Sr-87Rb 84Sr-87Rb
ObservationRb hyperfine splitting decreases by3 MHz for 2GHz binding energy of F=2 state
Observations• Transition linewidth increases
from 20kHz to 400kHz withincreasing binding energy
• 84Sr87Rb Rabi frequencies ~10x lower than Sr2 or 88Sr87Rb Rabi frequencies at given intensity
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Molecular potential fit resultsTo fit data, ground-state molecular potential needs to be 10% lower than predicted.
Scattering lengths obtained from fit (preliminary)
84Sr 86Sr 87Sr 88Sr85Rb 300a0 90a0 50a0 -10a0
87Rb 90a0 -15a0 -400a0 275a0
Simplest mixtures to work with
84Sr-87Rb
87Sr-87Rb
Bose - Bose
Fermi - Bose
Sr intraspecies 122a0 800a0 96a0 -2a0
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1-color PA: thermal cloud vs. BEC
-20 -15 -10 -5 0 5 100
5
10
15
Rb a
tom
num
ber (
104 )
Detuning (MHz)
thermal clouds
BECs
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Spatial overlap
interspecies scattering length intraspecies scattering lengths87Rb - 84Sr: 90 a0
87Rb: 105 a0 , 84Sr: 124 a0
no phase separationexpected
Phase-separation if
<
;
position
dens
ityde
nsity
position
low interspeciesscattering length
large interspeciesscattering length
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Spatial overlapWe use 1064 nm dipole trap: 3x deeper for Rb than for Sr
• gravitational sagging• weaker trap for Sr
Vertical position (µm)
Den
sity
(101
4cm
-3)
87Rb
84Sr
Vertical position (µm)
Pote
ntia
l (µK
)
1064nm dipole trap
Rb trap
Sr trap
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Bi-chromatic dipole trapBalance trap by 532nm dipole trap(attractive for Sr, repulsive for Rb) 1064nm
dipole trap
532nmdipole trap
Vertical position (µm)
Den
sity
(101
4cm
-3)
87Rb
84Sr
Vertical position (µm)
Pote
ntia
l (µK
)
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-20 -15 -10 -5 0 5 100
5
10
15
Rb a
tom
num
ber (
104 )
Detuning (MHz)
PA with trap compensation
thermal clouds
BECs, different potentials
-20 -15 -10 -5 0 5 100
5
10
15
Rb a
tom
num
ber (
104 )
Detuning (MHz)
BECs, similar potentials
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87Rb-84Sr Mott insulator
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PA of double Mott insulator
20 000 siteswith atoms of each species
-4 -3 -2 -1 0 1 2 3 4 50
1
2
3
4
5
6
7
Rb a
tom
num
ber (
104 )
Detuning (MHz)
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STIRAP attempts with 87Rb-84Sr
Rb 2S1/2 + Sr 1S0
Rb 2S1/2 + Sr 3P1|e>
Ω1Ω2
|m>
Γ
|a>
All attempts failed because of weak free-bound transition
Why is this transition so weak?
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Free-bound transition strength
88Sr - 87Rb
84Sr - 87Rb 7x10-4
4x10-3
87Sr - 87Rb 3x10-2
174
273
115
Excited statebinding energy
(MHz)
Franck-Condonfactor
40 times higherRabi frequency!
Try with 87Sr - 87Rb !
Predictions from ab-initio model fitted to data
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2S1/2 + 1S0
2S1/2 + 3P1
Towards the RbSr ground state
few 100 MHz binding energy~50 a0 radius
30 THz binding energy9 a0 radius
~500 a0 radius
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Spectroscopy of "hot" RbSr
HeN
Rb pickup cellSr pickup cell
pulsedlaser
Pickup process
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Spectroscopy of "hot" RbSrJ. Chem. Phys.141(23):234309 (2014)
12000 12100 12200 12300 12400 12500
E [cm-1]
0
1
2
3absorption[arb. units] simulation
experiment
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Current projectsRbSr molecules
Perpetual atom laser
Li-Sr quantum gas microscope
K quantum gases
Veni & Vici
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The team
AlexBayerle(PhD)
FlorianSchreck
(PI)
Chun-ChiaChen(PhD)
AlessioCiamei(PhD)
ShayneBennetts
(PhD)
GeorgiosSiviloglou
(Marie Curiefellow)
OleksiyOnichshenko
(PhD)
NamrataDutta-Mazumdar
(master)
Funding
Veni & Vici
VincentBarbé(PhD)
SergeyPyatchenkov
(PhD)BenjaminPasquiou(Veni PI)
DenisKurlov(PhD)