1. November 12, 2009 | Christian Stahl | 1 Fermion-Fermion and Boson-Boson Interaction at low Temperatures Seminar “physics of relativistic heavy Ions” TU Darmstadt, WS 2009/10 BCS – state: Long range attractive interaction between fermions BEC: 87 Rb above, at and below T C W. Ketterle, M. W. Zwierlein in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006 Anderson et al., 1995, Science 269, 198

2. Outline November 12, 2009 | Christian Stahl | 2  Cold trapped Fermions and Bosons BEC and BCS – states  Tuning atomic interactions: Feshbach resonances Short review on scattering theory Resonance scattering Interaction potentials between (alkali) atoms  Gas instabilities close to Feshbach resonances Atom loss due to inelastic collisions

3. Cold trapped Bosons November 12, 2009 | Christian Stahl | 3 Assume N non-interacting bosonic atoms trapped in a harmonic potential Single Particle Energies are Particle number is given by Symmetry of the trap fixes the symmetry of the problem

4. November 12, 2009 | Christian Stahl | 4 In the thermodynamic limit N→∞ and taking out the lowest state N 0 assuming N 0 → 0 at the Transition Temperature for BEC yields This gives the fraction of the condensed atoms below T C Cold trapped Bosons where

5. November 12, 2009 | Christian Stahl | 5 Cold trapped Bosons Data: dilute 87 Rb gas, Ensher et al., 1996, Phys. Rev. Lett. 77, 4984 Deviations of the experimental results from the prediction are due to finite size (particle number ≈ 40k at T C ) First order correction: lower T C for small N

6. November 12, 2009 | Christian Stahl | 6 Cold trapped Bosons Below T C the ground state has a macroscopic occupation → Bose-Einstein-Condensation Shape of the cloud is Gaussian (spherical Trap) condensed atoms thermal cloud (non-condensed gas) 5000 non-interacting Bosons at T=0.9T C in the model discussed above and assuming classical Boltzman distribution in the thermal cloud Dalfovo et al., 1999, Rev. Mod. Phys 71, 463

7. November 12, 2009 | Christian Stahl | 7 Cold trapped Bosons Inclusion of Interactions  For cold and dilute gases the main interactions are low energy two-body collisions  Main contribution comes from s-Wave scattering → More in the next Chapter…  Interaction is characterized by the Scattering Length a (a>0 → repulsive Interaction, a<0 → attractive Interaction)  Interatomic Potential V(r’-r) can be described by the parameterization where

8. November 12, 2009 | Christian Stahl | 8 Cold trapped Bosons Number of particles in ground state is expressed as where is a field with the meaning of an order parameter (“condensate wave function”) is governed by the Gross-Pitaevskii-Equation which is valid for  scattering length a much smaller than average particle distance  N 0 >> 1  Zero Temperature (all particles in condensate state)

9. November 12, 2009 | Christian Stahl | 9 Cold trapped Bosons Solution depends on ratio of kinetic and interaction energy ( is the oscillator length of the confining potential) Attractive interaction Repulsive interaction Figures from Dalfovo et al., 1999, Rev. Mod. Phys. 71, 475

10. November 12, 2009 | Christian Stahl | 10 Cold trapped Fermions Onset of quantum degeneracy is the same for bosons and fermions But the consequence is different! Bosons → phase transition to BEC Fermions → Multiple occupation of a state is forbidden → ? Classical gas Ideal Fermi gas De Marco et al., 2001, Phys. Rev. Lett. 86, 5409

11. November 12, 2009 | Christian Stahl | 11 Cold trapped Fermions For Fermions, the Fermi distribution function has to be used (with local density approximation): Introduce the single particle energy and the single particle density of states for the harmonic oscillator Then, the Particle number for a given spin species fixes the chemical potential

12. November 12, 2009 | Christian Stahl | 12 Cold trapped Fermions Density and Momentum distributions are where and is defined via the Fermi Energy (= the chemical potential at T=0) Density distribution is similar to that of bosons (Radius changes with for Fermions and for Bosons) Reason: Bosons → repulsive Interactions, Fermions → quantum pressure Momentum distribution: Width increases with N for Fermions and is independent of N for non-interacting Bosons (T=0)

13. November 12, 2009 | Christian Stahl | 13 Cold trapped Fermions For Fermions: Occurrence of Superfluidity only due to Interactions Assume weak attractive Interaction (a<0): Formation of bound states with exponentially small pairing energy ~ Pairs are very large, much larger than the inter-particle distance (Cooper, 1956) Pairs show bosonic character Fermionic Superfluidity below Suppression-Factor can easily be about 100 Superfluidity of electron-gas → Superconductivity (Bardeen, Cooper, Shrieffer 1957) W. Ketterle, M. W. Zwierlein in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006

14. November 12, 2009 | Christian Stahl | 14 Feshbach Resonances Interactions in dilute gases at low temperatures Relevant length scales: - inter-atomic Potential R 0 - thermal wavelength - inverse Fermi wave vector k F -1 or average Particle Distance d for Bosons, respectively In cold dilute gases: Interactions take place in form of two-body collisions. The cross section is given by and the scattering amplitude f can be expanded on Legendre Polynomials („partial waves expansion“)

15. November 12, 2009 | Christian Stahl | 15 Feshbach Resonances Low energy regime, that is with the wave vector of the scattered wave Centrifugal Barrier strongly suppresses interaction for l≠0: → All partial waves with l≠0 are negligible! → S-Wave scattering S-Wave scattering amplitude is independent of the scattering angle (S-Wave is spherical) Going to zero momentum, we get the  a shows the kind and strength of the interaction of the scattering particles S-Wave scattering length a ( is the phase shift)

16. November 12, 2009 | Christian Stahl | 16 Feshbach Resonances Expanding the scattering amplitude in a yields with „effective Range“ of the potential → Description becomes independent of the potentials details Strength and kind of Interaction is expressed by the scattering length a: 0 R: Deep Attraction (no bound states) (bound states) Figures: J. J.Sakurai: Mordern Quantum Mechanics

17. November 12, 2009 | Christian Stahl | 17 Feshbach Resonances Assuming 3D square-well potential and (broad Resonance):  Two-body bound States exist when Potential Depth exceeds, (E R stems from the Energy Uncertainty of the Particle confined in Potential-Well of Size R)  Binding Energy is where V-V n is the Detuning  Occurrence of a new bound State → diverging a = Phase Shift is π/2 (Resonance) Is there a Way to control the Detuning → control the Scattering Length?

18. November 12, 2009 | Christian Stahl | 18 Feshbach Resonances Controling the detuning  Scattering of two atoms with spins s 1 and s 2  Relative Orientation of the spins is crucial for the interaction: Singlet state Triplet state If no coupling: Scattering in Triplet potential V T (r) But: Hyperfine interaction potential is not diagonal in S = s 1 + s 2 Antisymmetric, thus coupling singlet (antisymmetric) and triplet (symmetric) state

19. November 12, 2009 | Christian Stahl | 19 Feshbach Resonances Singlet state Triplet state Initial triplet configuration can be scattered into a singlet bound state, if incoming energy and bound state energy match Singlet and Triplet state have different magnetic moment moments → relative Energy can be tuned by magnetic Field Singlet bound state Triplet state Figures: W. Ketterle, M. W. Zwierlein in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006

20.  Coupling of unbound tripled state („open channel“) and bound singlet state („closed channel“)  Both modeled by spherical well potentials and assuming only one bound state |m>  Continuum of plane waves of relative momentum k in the open channel are denoted |k>  Without coupling |m> and |k> are eigenstates of the free Hamiltonian H 0  Coupled state is described by  Hamiltonian is given by H=H 0 +V, the only non-zero Matrix Elements of V are November 12, 2009 | Christian Stahl | 20 Feshbach Resonances Controllable detuning via B-Field Figures: W. Ketterle, M. W. Zwierlein in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006

21.  Bound state has a size R far smaller than deBroglie-Wavelength  For low-Energy scattering we can assume up to an cut-off (E R stems from the energy uncertainty of the particle confined in Potential-Well of size R) Effects of the coupling  Resonance Position is shifted by  Two-Particle-Energy of the bound state is shifted downwards far from Resonance with close to the Resonance  At the Feshbach-Resonance, a diverges as with November 12, 2009 | Christian Stahl | 21 Feshbach Resonances

22. November 12, 2009 | Christian Stahl | 22 Feshbach Resonances  By the application of an magnetic field, a can be tuned from positive to negative values  At the resonance, a is divergent (“unitarity regime”) → System is at the same time dilute in the sense that R<<d and strongly interacting in the sense that a>>d → Gas is expected to show universal behavior independent of the details of the inter-atomic potential, that is all length scales associated with it disappear. For Example, at unitarity with  Negative and small values of a correspond to a Fermi Gas → becomes strongly interacting for large a → higher T C  Positive values of a correspond to bound Dimers → Bose Gas Continuous connection between Fermi Superfluidity and Bose-Einstein-Condensation  Fig.: W. Ketterle, M. W. Zwierlein in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006

23. November 12, 2009 | Christian Stahl | 23 Feshbach Resonances Fraction of bound Dimers in the state (|m> is the bound state) molecule fraction α² condensate fraction (In the discussed approach of two coupled Square-Wells) Fig.: Numerical thermodynamic Calculations by Williams et al., 2004, New J. of Phys. 6, 123

24. November 12, 2009 | Christian Stahl | 24 Feshbach Resonances For Bosons the situation is similar, but in some ways more difficult:  Going from negative to positive a and vice versa, a real Phase transition occurs between a) a phase where only molecule BEC-states exists (far on the molecule side of the Feshbach Resonance) b) a phase where both molecule and atomic BEC-states exists Existence of the phase transition (in contrast to the smooth crossover in the Fermi case) is due to the breakdown of the normal-phase symmetries in the annihilation operators and that do not occur for Fermions.  For attractive Interaction (a<0) the BEC is not stable (collapse due to high density). Critical value k is function of with k=0,574 k=0.459±0.012 ±0.054 (theoretical by Dalfovo et al., 1996, Phys. Rev. A 53, 2477 and others) (exp., Roberts et al., 2001, Phys. Rev. Lett.86, 4211) fig.: Romans et al., 2004, Phys. Rev. Lett. 93, 020405

25. November 12, 2009 | Christian Stahl | 25 Gas instabilities Atom Loss due to inelastic Collisions Dimers of size ~a formed in a Feshbach Resonance are usually in a highly excited rotovibrational state. In collisions, they can fall into deeper bound states of size R 0 (=Interaction Range) releasing Energy in the order causing the colliding Atom/Dimer that gains this Energy to leave the trap a E<<V HO R0R0 Dimer releases Energy E > V HO Collisions can occur between Dimers and Dimers as well as Dimers and Atoms with the scattering lengths for Atom/Dimer collisions and for Dimer/Dimer collisions causing loss rates for Atoms and for Dimers Loss coefficients α XY depend on the collision partner (atom/dimer) and on symmetry (distinguishable / indistinguishable constituents)

26. November 12, 2009 | Christian Stahl | 26 Gas instabilities Loss Rates in Dependence of Scattering Length a close to Resonance (large a) Simplest case: Dimer consists of 2 Fermions differing only in their Hyperfine state Collission with a Fermion identical to one of the Dimer’s constituents α ad ~a -3.33 and α dd ~a -2.55 (Petrov et al., 2004, Phys. Rev. Lett. 93, 090404) → Fermi-Fermi-Molecules are stabilized close to a Feshbach Resonance Bosonic Case: System of a Dimer consisting of 2 Bosons and and a bare bosonic Atom, two of the particles are identical α ad ~a and α dd ~a s with s>0 (D’Incao et al., 2006, Phys. Rev. A 73, 030702, Giorgini et al., 2008, Rev. Mod. Phys 80, 1215) → Boson-Boson-Molecules are destabilized close to a Feshbach Resonance

27. November 12, 2009 | Christian Stahl | 27 Gas instabilities System of a fermionic Molecule (composite of a Boson and a Fermion) colliding with a) distinguishable (Fermions) b) Bosons c) indistinguishable Fermions For large a: Loss rate is enhanced as expected due to bosonic attraction. For a<1000a 0 : Loss rate rises, maybe due to the bound Boson being effectively distinguishable from the free one. Expected Scaling is a -1, measured exponent is -0.97±0.16 for large a. (Which was done with respect to the molecule size, see inset) Decay rate is further suppressed for indistinguishable Fermions. 1/e Lifetime in this case (Bosons are 87 Rb and Fermions 40 K) is around 100ms (see inlet) figures from Zirbel et al., 2008, Phys. Rev. Lett. 100, 143201

28. November 12, 2009 | Christian Stahl | 28 Gas instabilities System of a fermionic Molecule (composite of a Boson and a Fermion) colliding with a) distinguishable (Fermions) b) Bosons c) indistinguishable Fermions figures from Zirbel et al., 2008, Phys. Rev. Lett. 100, 143201 Bosonic gas is instable due to collisions close to Resonance Fermionic gas is stabilized close to Resonance

29. November 12, 2009 | Christian Stahl | 29 Gas instabilities Mass-dependence of loss rates Considering a system with 2 identical Bosons or 2 Identical Fermions plus one distinguishable Atom with different mass m X Excerpt form Table I in D’Incao et al., 2006, Phys. Rev. A 73, 030702, figure from the same paper

30. November 12, 2009 | Christian Stahl | 30 Gas instabilities Mass-dependence of Dimer loss rates due to Dimer-Dimer collisions in a Fermion system For the Dimer-Dimer-Relaxation, the mass ratio is crucial, too:  For m1/m2=M/m > 12.3, the exponent s in the power law changes sign → Stabilization of the Fermion-Fermion Dimers is lost  For M/m > 13.6 the universal description in terms of a is lost due to Dominance of short-Range Physics figure from Petrov et al., 2005, J. Phys. B 38, S645

31. November 12, 2009 | Christian Stahl | 31 Summary  Both Bosons and Fermions show quantum effects when cooled down below  Bosons macroscopically occupy the ground state → Bose-Einstein-Condensation  Fermions form Cooper-Pairs and exhibit superfluid behavior  Interactions at low energy are characterized by the scattering length a  Variation of a can be obtained by varying an external B-Field → Feshbach-Resonances  Feshbach-Resonances allow for a continuous transition between weakly and deeply bound states → Creation of Fermion-Fermion pairs with bosonic character → BEC  Bose-Einstein- and Fermi-Statistics cause stability of fermionic gases and instability of bosonic gases close to the resonance (diverging scattering length a)

32. November 12, 2009 | Christian Stahl | 32 References (excerpt) Sections I+II S. Giorgini et al., 2008, “Theory of ultrocold atomic Fermi gases”, Rev. mod. Phys. 80, 1215 W. Ketterle, M. W. Zwierlein, 2006: “Making, probing and understanding ultracold Fermi gases” in Ultracold Fermi Gases, Proceedings of the International School of Physics ”Enrico Fermi”, Course CLXIV, Varenna, 20 - 30 June 2006 F. Dalfovo et al., 1999: “Theory of Bose-Einstein condensation in trapped gases”, Rev. Mod. Phys. 71, 463 Section III A.Koetsier et al., 2009: “Strongly interacting Bose gas: Noziéres and Schmitt-Rink theory and beyond”, Phys. Rev. A 79, 063609 D. S. Petrov et al., 2005: Diatomic molecules in ultracold Fermi gases—novel composite bosons, J. Phys. B 38, S645 J. J. Zirbel et al., 2009: Collisional Stability of Fermionic Feshbach Molecules, Phys. Rev. Lett. 100, 143201 J. L. Roberts et al., 2001: Controlled Collapse of a Bose-Einstein Condensate, Phys. Rev. Lett. 86, 4211

33. November 12, 2009 | Christian Stahl | 33 Reserve Figures: Mayer-Kuckuck, Kernphysik critical temperature in a fermionic system fig. from S. Giorgini et al., 2008, Rev. mod. Phys. 80, 1215

34. November 12, 2009 | Christian Stahl | 34 Reserve Koetsier et al., 2009, Phys. Rev. A 79, 063609

35. November 12, 2009 | Christian Stahl | 35 Reserve Manybody-Hamiltonian for Bosons BEC small perturbation, replace by where and

36. November 12, 2009 | Christian Stahl | 36 Reserve Further Problems for Boson Gases  molecular BEC states on the molecule Side of a Feshbach resonance are not stable when approaching Resonance (Situation of decreasing binding energy) (Romans et al., 2004, Phys Rev. Lett. 93, 020405)  The resulting atom cloud is mechanically unstable up to high pressures >10 3 times higher than reached in experiments so far  A mechanically stable atomic BEC on the molecular side of the Feshbach resonance exists, but is at a saddle point of free energy having energies higher than that of the molecules → Recombination of molecules (Basu et al., Phys. Rev. A 78, 2008, 053603)

37. November 12, 2009 | Christian Stahl | 37 Reserve Spherical trap, using the ansatz ( dimensionless parameter to controll the width of the BEC)