2009
DOI: 10.1103/physreva.80.023602
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Excited spin states and phase separation in spinor Bose-Einstein condensates

Abstract: We analyze the structure of spin-1 Bose-Einstein condensates in the presence of a homogenous magnetic field. We classify the homogenous stationary states and study their existence, bifurcations, and energy spectra. We reveal that the phase separation can occur in the ground state of polar condensates, while the spin components of the ferromagnetic condensates are always miscible and no phase separation occurs. Our theoretical model, confirmed by numerical simulations, explains that this phenomenon takes place … Show more

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Cited by 41 publications
(94 citation statements)
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References 49 publications
(112 reference statements)
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“…Since the Hamiltonian is invariant with respect to such spin rotations, we consider only the effects of the quadratic Zeeman shift [17,18]. For sufficiently weak magnetic field we can approximate it by a positive energy shift of the m f = ±1 sublevels…”
Section: The Model and Its Phase Diagrammentioning
confidence: 99%
“…Since the Hamiltonian is invariant with respect to such spin rotations, we consider only the effects of the quadratic Zeeman shift [17,18]. For sufficiently weak magnetic field we can approximate it by a positive energy shift of the m f = ±1 sublevels…”
Section: The Model and Its Phase Diagrammentioning
confidence: 99%
“…In the case of a homogeneous system V (x) = 0, one has to take into account the possibility of phase separation which occurs due to the relation between the self-and cross-scattering terms in the Hamiltonian, as it has been observed experimentally [23]. [22]. Moreover, the antiferromagnetic 2C state remains dynamically stable, up to a critical field b c > b 1 [12].…”
Section: Antiferromagnetic Spinor Condensates In One Dimensionmentioning
confidence: 99%
“…Since the Hamiltonian is invariant with respect to such spin rotations, we consider only the effects of the quadratic Zeeman shift [21,22]. For a sufficiently weak magnetic field we can approximate it by a positive energy shift of the m f = ±1 sublevels δ = (E + + E − − 2E 0 )/2 ≈ B 2 A, where B is the magnetic field strength and A = (g I + g J ) 2 μ 2 B /16E HFS , where g I and g J are the gyromagnetic ratios of the electron and nucleus, μ B is the Bohr magneton, and E HFS is the hyperfine energy splitting at zero magnetic field [21,22]. Finally, the spin-dependent Hamiltonian (2) becomes…”
Section: Antiferromagnetic Spinor Condensates In One Dimensionmentioning
confidence: 99%
“…, where E HFS is the hyperfine energy splitting at zero magnetic field, α = (g I + g J )µ B B/E HFS , µ B is the Bohr magneton, g I and g J are the gyromagnetic ratios of electron and nucleus, and B is the magnetic field strength [17].…”
mentioning
confidence: 99%
“…This argument also allows to understand the absence of rotonlike instability in ferromagnetic condensates. In this case, the excited nematic and 2C states [17] are characterized by zero transverse spin, and the spin conservation does not prevent energy relaxation.…”
mentioning
confidence: 99%