Download presentation
Presentation is loading. Please wait.
Published byAbner Johns Modified over 5 years ago
1
Dynamics of spinor condensates: dipolar interactions and more
Eugene Demler Harvard University Collaborators: Ehud Altman, Robert Cherng, Vladimir Gritsev, Mikhail Lukin, Anatoli Polkovnikov, Ana Maria Rey Experimental collaborators: Immanuel Bloch’s group and Dan Stamper-Kurn’s group Funded by NSF, DARPA, MURI, AFOSR, Harvard-MIT CUA
2
Outline Dipolar interactions in spinor condensates
Larmor precession and dipolar interactions. Roton instabilities. Following experiments of D. Stamper-Kurn Superexchange interaction in double well systems Towards quantum magnetism of ultracold atoms. Collaboration with I. Bloch’s group. Many-body decoherence and Ramsey interferometry Luttinger liquids and non-equilibrium dynamics.
3
Dipolar interactions in spinor condensates.
Introduction
7
Possible supersolid phase in 4He
Phase diagram of 4He A.F. Andreev and I.M. Lifshits (1969): Melting of vacancies in a crystal due to strong quantum fluctuations. Also G. Chester (1970); A.J. Leggett (1970) T. Schneider and C.P. Enz (1971). Formation of the supersolid phase due to softening of roton excitations
8
Resonant period as a function of T
9
Interlayer coherence in bilayer quantum Hall systems at n=1
Hartree-Fock predicts roton softening and transition into a state with both interlayer coherence and stripe order. Transport experiments suggest first order transition into a compressible state. Eisenstein, Boebinger et al. (1994) L. Brey and H. Fertig (2000)
10
Roton spectrum in pancake polar condensates
Santos, Shlyapnikov, Lewenstein (2000) Fischer (2006) Origin of roton softening Repulsion at long distances Attraction at short distances Stability of the supersolid phase is a subject of debate
11
Magnetic dipolar interactions in spinor condensates
q Comparison of contact and dipolar interactions. Typical value a=100aB For 87Rb m=mB and e= For 52Cr m=6mB and e=0.16 Bose condensation of 52Cr. T. Pfau et al. (2005) Review: Menotti et al., arXiv take a=100a_0
12
Magnetic dipolar interactions in spinor condensates
Interaction of F=1 atoms Ferromagnetic Interactions for 87Rb A. Widera, I. Bloch et al., New J. Phys. 8:152 (2006) a2-a0= aB Spin-depenent part of the interaction is small. Dipolar interaction may be important (D. Stamper-Kurn)
13
Spontaneously modulated textures in spinor condensates
Vengalattore et al. PRL (2008) Fourier spectrum of the fragmented condensate
14
This talk: Instabilities of F=1 spinor condensates due to dipolar interactions. New phenomena due to averaging over Larmor precession Theory: unstable modes in the regime corresponding to Berkeley experiments Results of Berkeley experiments Wide range of instabilities tuned by quadratic Zeeman, AC Stark shift, initial spiral spin winding
15
Instabilities of F=1 spinor condensates due to
dipolar interactions and roton softening Earlier theoretical work on dipolar interactions in spinor condensates: Meystre et al. (2002), Ueda et. al. (2006), Lamacraft (2007). New phenomena: interplay of finite transverse size and dipolar interaction in the presence of fast Larmor precession
16
Dipolar interactions after averaging over Larmor precession
17
Energy scales Magnetic Field B F S-wave Scattering Dipolar Interaction
Larmor Precession (100 kHz) Quadratic Zeeman (0-20 Hz) B F S-wave Scattering Spin independent (g0n = kHz) Spin dependent (gsn = 10 Hz) Dipolar Interaction Anisotropic (gdn=10 Hz) Long-ranged Reduced Dimensionality Quasi-2D geometry
18
Dipolar interactions Static interaction
parallel to is preferred “Head to tail” component dominates z Averaging over Larmor precession perpendicular to is preferred. “Head to tail” component is averaged with the “side by side”
19
Instabilities: qualitative picture
20
Stability of systems with static dipolar interactions
Ferromagnetic configuration is robust against small perturbations. Any rotation of the spins conflicts with the “head to tail” arrangement Large fluctuation required to reach a lower energy configuration
21
Dipolar interaction averaged after precession
“Head to tail” order of the transverse spin components is violated by precession. Only need to check whether spins are parallel XY components of the spins can lower the energy using modulation along z. X X Z components of the spins can lower the energy using modulation along x Strong instabilities of systems with dipolar interactions after averaging over precession
22
Instabilities: technical details
23
From Spinless to Spinor Condensates
Charge mode: n is density and h is the overall phase I would like to begin this talk by discussing what distinguishes a spinor condensate from a spinless one. Spinless particles have a rather simple structure characterized by two conjugate variables: phase and particle number. The hallmark of Bose-Einstein condensation is development of coherence in the phase variable. In turn, the experimental signature of this condensate is the macroscopic occupation of the ground state. What makes spinor condensates more interesting is that they have a richer and more complex internal structure. In addition to developing phase coherence, spinor condensates still have additional degrees of freedom describing the orientation of magnetization for example. Experimentally, this means that this rather featureless condensate peak describing spinless condensates can develop complex patterns and structure in spinor condensates. However understanding and manipulating this complex internal structure poses a number of difficult challenges for experiment (which have been the focus of the Stamper-Kurn group at Berkeley) and theory (some aspects of which I will be discussing today). Spin mode: f determines spin orientation in the XY plane c determines longitudinal magnetization (Z-component)
24
Hamiltonian Magnetic Field Quasi-2D Dipolar Interaction
S-wave Scattering The geometry I want to consider is the following: n is the normal to the 2D plane of the condensate and B points along the magnetic field at an angle alpha wrt n. k is the momentum vector in the plane and kappa is the wavevector for the spiral which are at angles theta and beta wrt to e1, which is the projection of the magnetic field vector in the plane. The thickness of the plane is dn. In order to study these competing effects, we consider the following Hamiltonian. Here psi is the spin 1 field describing the condensate and there is the usual kinetic energy and chemical potential terms. Harmonic confinement along n gives rise to the 2D geometry. The magnetic field enters through the linear and quadratic Zeeman terms. There are also interaction terms coupling the total density and spin densities with strength guv. S-wave scattering terms are contact interactions while the dipolar interaction is long ranged.
25
Precessional and Quasi-2D Averaging
Rotating Frame Gaussian Profile It turns out the bare 3D dipolar interaction is strongly modified due to the precessional dynamics of the spins and the quasi-2D nature of the system. To take into account the precessional dynamics, we use the fact that the time scale for precession 115 Hz is much faster than the time scale for dipolar interactions 10 Hz. By transforming to a rotating frame comoving with the spins, we can then obtain the effective dipolar interaction by time averaging. To take into account the reduced dimensionality, we assume the spins are frozen along the n direction and take a gaussian trial wavefunction along this direction. The final, quasi-2d time averaged dipolar interaction relevant for the spin dynamics is heavily modified by these two effects. Quasi-2D Time Averaged Dipolar Interaction
26
Quasi-2D Time Averaged Dipolar Interaction
27
Collective Modes Equations of Motion δφ δfB δη δn Ψ0 Spin Mode
Mean Field Equations of Motion Collective Fluctuations (Spin, Charge) δφ δfB δη δn Ψ0 Spin Mode δfB – longitudinal magnetization δφ – transverse orientation Charge Mode δn – 2D density δη – global phase
28
Instabilities of collective modes
Q measures the strength of quadratic Zeeman effect
29
Instabilities of collective modes
30
Berkeley Experiments: checkerboard phase
To original goal of this talk was to try to explain some of the observations of the Berkeley group on spinor condensates. The left hand side shows the measured modulated spin texture in real space and momentum space with dipolar interactions at full strength and strength reduced by sequences of random pi/2 pulses. In real space there is a distinct checkerboard pattern with a roughly length scale of 10 microns in either direction. In momentum space, the spin texture has a distinctive shape with two lobes connected to the origin and two lobes disconnected from the origin. The right hand side shows the magnitude of the imaginary part of the excitation energies in momentum space. There are two lobes connected to the origin along the direction perpendicular to the axis of the field while the two lobes along the field are disconnected from the origin. In addition the two lobes are of roughly equal magnitude and are peaked near a length scale of 10 microns. M. Vengalattore, et. al, arXiv:
31
Dipolar interaction averaged after precession
XY components of the spins can lower the energy using modulation along z. X X Z components of the spins can lower the energy using modulation along x
32
Instabilities of collective modes
33
Instabilities of collective modes. Spiral configurations
Spiral wavelength Spiral spin winding introduces a separate branch of unstable modes
34
Superexchange interaction in experiments with double wells
Refs: Theory: A.M. Rey et al., Phys. Rev. Lett. 99: (2007) Experiment: S. Trotzky et al., Science 319:295 (2008)
35
Two component Bose mixture in optical lattice
Example: Mandel et al., Nature 425:937 (2003) t t Two component Bose Hubbard model
36
Quantum magnetism of bosons in optical lattices
Duan, Demler, Lukin, PRL 91:94514 (2003) Altman et al., NJP 5:113 (2003) Ferromagnetic Antiferromagnetic
37
Observation of superexchange in a double well potential
Theory: A.M. Rey et al., PRL (2007) J J Use magnetic field gradient to prepare a state Observe oscillations between and states Experiment: Trotzky et al., Science (2008)
38
Preparation and detection of Mott states
of atoms in a double well potential
39
Comparison to the Hubbard model
Experiments: I. Bloch et al.
40
Beyond the basic Hubbard model
Basic Hubbard model includes only local interaction Extended Hubbard model takes into account non-local interaction
41
Beyond the basic Hubbard model
42
Observation of superexchange in a double well potential.
Reversing the sign of exchange interactions
43
Many-body decoherence and Ramsey interferometry
Collaboration with A. Widera, S. Trotzky, P. Cheinet, S. Fölling, F. Gerbier, I. Bloch, V. Gritsev, M. Lukin Phys. Rev. Lett. (2008)
44
Ramsey interference Working with N atoms improves the precision by .
1 Working with N atoms improves the precision by Need spin squeezed states to improve frequency spectroscopy
45
Squeezed spin states for spectroscopy
Motivation: improved spectroscopy, e.g. Wineland et. al. PRA 50:67 (1994) Generation of spin squeezing using interactions. Two component BEC. Single mode approximation Kitagawa, Ueda, PRA 47:5138 (1993) In the single mode approximation we can neglect kinetic energy terms
46
Interaction induced collapse of Ramsey fringes
Ramsey fringe visibility - volume of the system time Experiments in 1d tubes: A. Widera, I. Bloch et al.
47
Spin echo. Time reversal experiments
Single mode approximation The Hamiltonian can be reversed by changing a12 Predicts perfect spin echo
48
Spin echo. Time reversal experiments
Expts: A. Widera, I. Bloch et al. Experiments done in array of tubes. Strong fluctuations in 1d systems. Single mode approximation does not apply. Need to analyze the full model No revival?
49
Interaction induced collapse of Ramsey fringes. Multimode analysis
Low energy effective theory: Luttinger liquid approach Luttinger model Changing the sign of the interaction reverses the interaction part of the Hamiltonian but not the kinetic energy Time dependent harmonic oscillators can be analyzed exactly
50
Time-dependent harmonic oscillator
See e.g. Lewis, Riesengeld (1969) Malkin, Man’ko (1970) Explicit quantum mechanical wavefunction can be found From the solution of classical problem We solve this problem for each momentum component
51
Fundamental limit on Ramsey interferometry
Interaction induced collapse of Ramsey fringes in one dimensional systems Only q=0 mode shows complete spin echo Finite q modes continue decay The net visibility is a result of competition between q=0 and other modes Conceptually similar to experiments with dynamics of split condensates. T. Schumm’s talk Fundamental limit on Ramsey interferometry
52
Summary Dipolar interactions in spinor condensates
Larmor precession and dipolar interactions. Roton instabilities. Following experiments of D. Stamper-Kurn Superexchange interaction in double well systems Towards quantum magnetism of ultracold atoms. Collaboration with I. Bloch’s group. Many-body decoherence and Ramsey interferometry Luttinger liquids and non-equilibrium dynamics.
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.