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Fermi Gases in Slowly Rotating Traps: Superfluid vs Collisional Hydrodynamics. Marco Cozzini and Sandro Stringari Università di Trento and BEC-INFM.
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Fermi Gases in Slowly Rotating Traps:Superfluid vs Collisional Hydrodynamics Marco Cozzini and Sandro Stringari Università di Trento and BEC-INFM
RECENT EXPERIMENTS WITH FERMI GASES NEAR A FESHBACH RESONANCE HAVE REVEALED STRONG INTERACTION EFFECTS:HYDRODYNAMIC EXPANSION(DUKE, JILA, ENS)FORMATION OF MOLECULES (a>0)(JILA, ENS)both effects are compatible with superfluidity but do not test it
Hydrodynamics predicts anisotropic expansion in Fermi superfluids(Menotti et al, PRL 89, 250402(2002))
Anisotropic expansion in Fermi gases:- test of hydrodynamic forces- test of superfluidityonly if normal gas is collisionless and expands ballistically (true at low T far from Feshbach resonance)
PLAUSIBLE SCENARIO:Near a Feshbach resonance a Fermi gas exhibits universal hydrodynamic behaviour • Below Tc hydrodynamics is due to superfluidity • Above Tc hydrodynamics is due to collisions
Can we distinguish between superfluid and collisional hydrodynamics? • NO if we consider irrotational flow (for example: expansion) • YES if we look for vorticity effects
POSSIBLE TEST OF SUPERFLUIDITY IN TRAPPED FERMI GASES: ROTATIONAL PROPERTIES(PROBE TRANSVERSE RESPONSE) • QUANTIZED VORTICES (cannot be described by hydrodynamics) • MOMENT OF INERTIA (described by hydrodynamics)
Outline • Superfluid (irrotational) and Collisional (rotational) Hydrodynamics • Collective Oscillations without rotation • Collective oscillations with rotating trap: test of superfluidity
Recent applications of rotational hydrodynamics to Bose-Einstein condensed gases containing many vortical lines (diffused vorticity): M. Cozzini and S. Stringari, Phys. Rev.A 67, 041602 (2003) F. Chevy and S. Stringari, Kelvin modes, in preparation
Collisional (rotational) hydrodynamics zero-order approximation of Boltzmann equation (no viscosity) Superfluid (irrotational) hydrodynamics
Expansion of non rotating gas - Collective oscillations built on top of non rotating gasSAME BEHAVIOUR IN SUPERFLUID AND COLLISIONAL HYDRODYNAMICS(including scissors oscillation !!)
Collective Oscillations (static trap) Axisymmetric case Quadrupole oscillations
RotatingHarmonic Potential Stationary solutions in rotating frame Rotational hydrodynamics Time needed to spin up a normal gas by rotating the trap: Small static anisotropy unimportant in hydrodynamic regime Irrotational hydrodynamics
TIME NEEDED TO SPIN UP A NORMAL GAS IN HYDRODYNAMIC REGIME(Guery-Odelin, 2000) Small static anisotropy unimportant in hydrodynamic regime
SPLITTING of m= 2 and -2 QUADRUPOLE FREQUENCIES (rotational hydrodynamics):twice the angular velocity of the fluid consistent with
Rotationaltest of Superfluidity(1) • Initial condition: deformed trap rotating at small angular velocity • Switch off trap deformation: excitation of m=+2 and m=-2 quadrupole modes
Superfluid HD • (b) collisional HD
Rotationaltest of Superfluidity(2) • Initial condition: deformed trap rotating at small angular velocity • Stop the rotation of the trap: excitation of the scissors mode
Collisional HD: beating of m=+2 and m=-2 modes Superfluid HD: oscillation with scissors frequency
Superfluid HD; • Collisional HD
Conclusion • Rotation of trapped Fermi gas at small angular velocity: natural tool to test superfluidity