2014
DOI: 10.1126/science.1244059
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Giant Spin Oscillations in an Ultracold Fermi Sea

Abstract: Collective behavior in many-body systems is the origin of many fascinating phenomena in nature, ranging from the formation of clouds to magnetic properties of solids. We report on the observation of collective spin dynamics in an ultracold Fermi sea with large spin. As a key result, we observed long-lived and large-amplitude coherent spin oscillations driven by local spin interactions. At ultralow temperatures, Pauli blocking stabilizes the collective behavior, and the Fermi sea behaves as a single entity in s… Show more

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Cited by 57 publications
(87 citation statements)
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References 37 publications
(35 reference statements)
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“…Additionally, at very low temperatures, Pauli blocking can partially prevent mode changing collisions for a spinpolarized sample, as recently observed in Ref. [66]. However, even in a spin-polarized gas, spin-and mode-changing processes may occur, resulting in a doubly occupied mode.…”
Section: The Generalized Spin Model Approximation: Validity and Discusupporting
confidence: 55%
“…Additionally, at very low temperatures, Pauli blocking can partially prevent mode changing collisions for a spinpolarized sample, as recently observed in Ref. [66]. However, even in a spin-polarized gas, spin-and mode-changing processes may occur, resulting in a doubly occupied mode.…”
Section: The Generalized Spin Model Approximation: Validity and Discusupporting
confidence: 55%
“…Actually, the experimental setup for spin dynamics in LSFG33343536 can be shared to examine the results in this work. The system can be initially prepared with a balanced spin mixture with , which is confined in a harmonic trap, and evaporated to a temperature .…”
Section: Resultsmentioning
confidence: 99%
“…Recently, considerable effort has been devoted to the spin dynamics33343536 and Mott-insulator transformation3738 in the LSFG. To our best knowledge, however, the study related to FM transition in LSFG is rare.…”
mentioning
confidence: 99%
“…The direct observation of several periods of these oscillations has allowed us to demonstrate the coherence of the process and to measure the exchange interaction strength in an accurate, model-independent way. We note that, if compared with the spin dynamics observed in other atomic systems, arising from either small differences in the scattering lengths [23][24][25] or from second-order tunneling between adjacent sites of an optical lattice [26], the oscillation that we have measured is significantly fast. In particular, the exchange energy V ex , on the order of ∼h × 10 kHz, is much larger than either the Fermi (k B T F ) or the thermal (k B T) energy, which makes 173 Yb remarkably interesting for the observation of quantum magnetism in a two-orbital system with SUðNÞ interaction symmetry [4].…”
Section: -3mentioning
confidence: 90%