Recall when we briefly investigated quantum statistics (Nov. 20, 2014 post) we saw that bosons have integral spin values and so an orbital may be populated by any number of bosons so the Pauli Exclusion principle doesn’t apply. (The Pauli Exclusion Principle prohibits two particles having identical quantum numbers from occupying the same energy level in a multi-electron atom.)
To prepare their gas, the researchers used two stages of laser cooling down to 2 μK and then introduced a single dimple trap for the atoms to pool into. To finish the cooling process, they left the gas to evaporate for as short as 0.6 s, down from about 10 s for two-spin gases. The more fermions that are colliding in each energy level, the faster they cool.
The researchers prepared Sr (strontium) atoms with all 10 possible nuclear spin states—that is, 10 atoms per energy level—and 5 × 104 atoms per spin state by the end of evaporation. Although the fermion interactions are weak, they measurably change the system’s density fluctuations, compressibility, and time-of-flight dynamics, in agreement with theoretical models.
Incredibly, research into SU(N) Fermi gases started only in the past decade. Not too surprising given that previous studies were limited by fact the temperature regimes accessible for the gases were too low. Hence, the resulting interactions didn't significantly alter the system's thermodynamic behavior, i.e. compared to non-iteracting Fermi gases that lack SU(N) symmetric interactions.
Now that researchers have an efficient preparation method and a basic understanding of the properties of interacting Fermi gases, says Ye, the gases will be “premium fuel for a quantum simulator.” Different combinations of kinetic energy, interaction energy, and nuclear spins can be used to systematically explore the phase diagram of, for example, the Fermi–Hubbard model (see the article by Gabriel Kotliar and Dieter Vollhardt, Physics Today, March 2004,
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