2008
DOI: 10.1007/s10909-008-9802-x
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Spin Dynamics of a Trapped Spin-1 Bose Gas above the Bose-Einstein Transition Temperature

Abstract: We study collective spin oscillations in a spin-1 Bose gas above the Bose-Einstein transition temperature. Starting from the Heisenberg equation of motion, we derive a kinetic equation describing the dynamics of a thermal gas with the spin-1 degree of freedom. Applying the moment method to the kinetic equation, we study spin-wave collective modes with dipole symmetry. The dipole modes in the spin-1 system are classified into the three types of modes. Frequencies and damping rates of the dipole modes are obtain… Show more

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Cited by 16 publications
(39 citation statements)
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References 38 publications
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“…To understand the observed spin dynamics quantitatively, we model the Na condensate with the timedependent Gross-Pitaevskii equation [20,36] and the thermal Rb cloud with the kinetic equation for the Wigner distribution function [39,40]. The dynamics of the two species are coupled through the interaction in Eq.…”
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confidence: 99%
“…To understand the observed spin dynamics quantitatively, we model the Na condensate with the timedependent Gross-Pitaevskii equation [20,36] and the thermal Rb cloud with the kinetic equation for the Wigner distribution function [39,40]. The dynamics of the two species are coupled through the interaction in Eq.…”
mentioning
confidence: 99%
“…Bosonic and fermionic alkali pseudo-spin-1/2 systems have also been studied [13][14][15], and spin domain formation has been observed in these systems [16][17][18]. Due to the spindependent interaction that is absent in the pseudo-spin-1/2 system, a spin-1 gas is predicted to have additional interesting coherent collisional (spinor) dynamics which give rise to spin waves or population oscillations [19,20].The dynamics of spinor BECs have been widely investigated in spin-1 Na and Rb gases, as reviewed in Refs. [21,22].…”
mentioning
confidence: 99%
“…This transport equation was obtained previously in [19,20] and details of its derivation can be found there. We do not include the collision integral, which has the role of describing damping.…”
mentioning
confidence: 99%
“…There are a number of literatures related to the early stage of spin evolution [16][17][18][19][20][21][22][23]. Starting from an initial state | 0 , the system will evolve as (t) = e −i(H +H B )ωt | 0 .…”
Section: Temperature-dependent Hyperfine Populations and Their Oscillmentioning
confidence: 99%