Tunable Molecular Many-Body Physics and the Hyperfine Molecular Hubbard Hamiltonian
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Transcript of Tunable Molecular Many-Body Physics and the Hyperfine Molecular Hubbard Hamiltonian
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Tunable Molecular Many-Body Physics and the Hyperfine Molecular
Hubbard Hamiltonian
Michael L. Wall
Department of Physics
Colorado School of Mines
in collaboration with
Lincoln D. Carr
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Motivation: Ultracold atoms in optical lattices
Extremely tunable interactionsOver 8 orders of magnitude!
Repulsive or attractive
PRL 102 090402
Trapping in optical potentialOptical potential couples to
dynamical polarizability of object
Simple 2-state picture: AC Stark effect
Potential proportional to intensity
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The Bose-Hubbard Model
• Excellent approximation for deep lattices!• Accounts for SF-MI transition• Simplest nontrivial bosonic lattice model
Field operator
Hopping
Interaction
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Diatomic Molecules
3 energy scalesElectronic potential
Vibrational excitations
Rotational excitations
Rough scaling based on powers of m_e/M_N
At ultracold temps neglect all except for rotational terms
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Focus on Heteronuclear Alkali Dimers
No spin or orbital angular momentum:
Rotational energy scale determined by B~GHz
Heteronuclear->permanent dipole moment d~1D
Dynamical polarizability is anisotropic
K
Rb
QuickTime™ and a decompressor
are needed to see this picture.
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Experimental setup
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Internal structure
Rotational Hamiltonian
Integer Angular momenta
Linear level spacing
Spherical Symmetry
Hyperfine HamiltonianLots of terms, most small
Nuclear Quadrupole dominates
Nuclear QuadrupoleDiagonal in F=N+I
Mixing of rotational/nuclear spin states
Parameters taken from DFT/experiment
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External FieldsStark effect
Breaks rotational symmetry
Couples N->N+1
Dipole moments induced along field direction
1D~0.5 GHz/(kV/cm)
Zeeman effect
Rotational coupling-small
Nuclear spin coupling-large
New handle on system
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Dipolar control
Separation of dipolar and hyperfine degrees of freedom Selection rule for nuclear spin projection along E-field
Dipole strongly couples to E field, insensitive to B field
Reverse for Nuclear spin-rotate using B field
Dipole character “smeared” across many states
E B
E
B
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What does the dipole get us?
Resonant dipole-dipole interaction
Anisotropic and long range
Dominates rethermalization via inelastic collisions
Ultracold chemistry->bad news for us!
Stabilize using DC field and reduced geometry
Coupling to AC microwave fields
Dynamics!
Easy access to internal states
PRA 76 043604 (2007)
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Optical lattice effects
Dynamical polarizability is anisotropicReducible rank-2 tensor
Write in terms of irreducible rank-0 and rank-2 components
Tunneling depends on rotational modeDifferent “effective mass”
Put this all together…
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The Hyperfine Molecular Hubbard Hamiltonian
Energy offsets from single particle spectra
Tunneling dependent on rotational mode
Nearest neighbor Dipole-Dipole interactions
Transitions between states from AC driving
Wall and Carr PRA 82 013611 (2010)
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Applications 1: Internal state dependence
No AC field->Extended Bose-Hubbard model
Studies of quantum phase equilibria
Dynamics of interactions between phases
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Applications 2: Quantum dephasing
Exponential envelope on Rabi oscillationsPurely many-body in nature
Emergent timescale
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Applications 3: Tunable complexity
Many interacting degrees of freedomCan dynamically alter the number and timescale
Interplay of spatial and internal dof->Emergence
“Quantum complexity simulator”
Quantitative discussion in the works
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Conclusions/Further research
• Cold atoms are great “quantum simulators”• Molecules have interesting new structure that
can be controlled• Emergent behavior, complexity simulator• Future work will quantify complexity, study
different molecular species, include loss terms related to chemistry, study dissipative quantum phase transitions, etc.
• Wall and Carr PRA 82 013611 (2010)
• Wall and Carr NJP 11 055027 (2009)
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Stark Spectra
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Experimental Progress
Molecules at edge of quantum degeneracy87Rb-40K, JILA
Absolute ground state
STIRAP procedure
Hyperfine state is important!A single hyperfine state is populated
Can be chosen via experimental cleverness
http://physics.aps.org/viewpoint-for/10.1103/PhysRevLett.101.133005
http://jila.colorado.edu/yelabs/research/cold.html
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How do we simulate such a Hamiltonian?
We want to solve the Schroedinger eqn.
Question: How big is Hilbert space?Answer 1: Big
Exponential scaling->exact diagonalization difficult
Answer 2: Too big
Finite range Hamiltonians can’t move states “very far”
All eigenstates of such Hamiltonians live on a tiny submanifold of full Hilbert space
In 1D, restate as: critical entanglement bounded by
Perform variational optimization in class of states with restricted entanglement->”Entanglement compression”
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Time-Evolving Block Decimation
Variational method in the class of Matrix Product States
Polynomial scalingFind ground states of nearest-neighbor Hamiltonians
Simulate time evolution (still difficult)
Google “Open source tebd”
Original paper G. Vidal PRL 91 147902 (2003)
What does it say about HMHH?
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Hubbard ParametersChoose appropriate Wannier basis, compute overlaps
Hopping
Internal energy
Transitions
Interaction
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Route I: Single and many molecule physics decoupled
DC Ground state structure DC+AC Ground
state structure
Dynamics
E BNs = 2
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Decoupled: Entanglement and structure factors
E BNs = 2
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Now couple single to many molecule physics
E BNs = 2
DC Ground state structure DC+AC Ground
state structure
Dynamics
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Coupled: Entanglement and Structure Factors
E BNs = 2
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Route II: Turning on Internal State Structure
Ns = 4E B
DC Ground state structure DC+AC Ground
state structure
Dynamics
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Entanglement and Structure Factor
E BNs = 4
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Route II.3 E
BNs = 4
DC Ground state structure DC+AC Ground
state structure
Dynamics
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Route II.4Ns = 4
E
B
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Physical Scales for this Problem