In recent years, low-temperature fermion gases have demonstrated some remarkable properties. For example, under certain circumstances a trapped sample can be magnetically tuned through a so-called Feshbach resonance (see Physics Today, August 2004, page 12). On one side of the resonance, the spin-up and spin-down fermions pair strongly into molecules and form a superfluid Bose–Einstein condensate (BEC); on the other side, they pair weakly into a superconducting-type superfluid. Two independent groups—one at Rice University, the other at MIT—have now explored what happens when the spin-up and spin-down populations of lithium-6 atoms are unequal. Both groups found signatures in which leftover fermions are expelled into a halo surrounding the superfluid core. The MIT group found that when the polarization exceeded a critical value, the superfluid state collapsed under the pressure of the unpaired fermions. The Rice group observed that the phase separation occurred only above a critical polarization; for the resonantly interacting gas at small polarization, they saw evidence that unpaired fermions can coexist with the superfluid. If confirmed, that coexistence would constitute a new form of fermionic superfluidity. The work may have relevance to magnetized superconductors or to quark matter at the cores of neutron stars. (G. B. Partridge et al., Science , in press; M. W. Zwierlein et al., Science , in press. Both articles were posted to Science Express on 22 December 2005.)
The finding that the Saturnian moon may host layers of icy slush instead of a global ocean could change how planetary scientists think about other icy moons as well.
Modeling the shapes of tree branches, neurons, and blood vessels is a thorny problem, but researchers have just discovered that much of the math has already been done.
January 29, 2026 12:52 PM
This Content Appeared In
Volume 59, Number 2
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