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Matter-wave solitons with a periodic, piecewise-constant scattering length

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dc.contributor.author Rodrigues, AS en
dc.contributor.author Kevrekidis, PG en
dc.contributor.author Porter, MA en
dc.contributor.author Frantzeskakis, DJ en
dc.contributor.author Schmelcher, P en
dc.contributor.author Bishop, AR en
dc.date.accessioned 2014-03-01T01:57:27Z
dc.date.available 2014-03-01T01:57:27Z
dc.date.issued 2008 en
dc.identifier.issn 1050-2947 en
dc.identifier.uri https://dspace.lib.ntua.gr/xmlui/handle/123456789/28423
dc.subject.classification Optics en
dc.subject.classification Physics, Atomic, Molecular & Chemical en
dc.subject.other BOSE-EINSTEIN CONDENSATE en
dc.subject.other OPTICAL LATTICES en
dc.subject.other FESHBACH RESONANCES en
dc.subject.other DARK SOLITONS en
dc.subject.other HAMILTONIAN-SYSTEMS en
dc.subject.other ULTRACOLD ATOMS en
dc.subject.other SOLITARY WAVES en
dc.subject.other NEUTRAL ATOMS en
dc.subject.other POTENTIALS en
dc.subject.other TRAPS en
dc.title Matter-wave solitons with a periodic, piecewise-constant scattering length en
heal.type journalArticle en
heal.identifier.secondary 013611 en
heal.language English en
heal.publicationDate 2008 en
heal.abstract Motivated by recent proposals of "collisionally inhomogeneous" Bose-Einstein condensates (BECs), which have a spatially modulated scattering length, we study the existence and stability properties of bright and dark matter-wave solitons of a BEC characterized by a periodic, piecewise-constant scattering length. We use a "stitching" approach to analytically approximate the pertinent solutions of the underlying nonlinear Schrodinger equation by matching the wave function and its derivatives at the interfaces of the nonlinearity coefficient. To accurately quantify the stability of bright and dark solitons, we adapt general tools from the theory of perturbed Hamiltonian systems. We show that stationary solitons must be centered in one of the constant regions of the piecewise-constant nonlinearity. We find both stable and unstable configurations for bright solitons and show that all dark solitons are unstable, with different instability mechanisms that depend on the soliton location. We corroborate our analytical results with numerical computations. en
heal.publisher AMER PHYSICAL SOC en
heal.journalName PHYSICAL REVIEW A en
dc.identifier.isi ISI:000258180300167 en
dc.identifier.volume 78 en
dc.identifier.issue 1 en


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