Ciencias,UNAM

Standard and embedded solitons in nematic optical fibers

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dc.contributor.author Reyes, JA
dc.contributor.author Espinosa-Ceron, A
dc.contributor.author Fujioka, J
dc.contributor.author Malomed, BA
dc.contributor.author Rodríguez, RF
dc.date.accessioned 2011-01-22T10:26:44Z
dc.date.available 2011-01-22T10:26:44Z
dc.date.issued 2003
dc.identifier.issn 1063-651X
dc.identifier.uri http://hdl.handle.net/11154/1681
dc.description.abstract A model for a non-Kerr cylindrical nematic fiber is presented. We use the multiple scales method to show the possibility of constructing different kinds of wave packets of transverse magnetic modes propagating through the fiber. This procedure allows us to generate different hierarchies of nonlinear partial differential equations which describe the propagation of optical pulses along the fiber. We go beyond the usual weakly nonlinear limit of a Kerr medium and derive a complex modified Korteweg-de Vries equation (CM KdV) which governs the dynamics for the amplitude of the wave packet. In this derivation the dispersion, self-focussing, and diffraction in the nematic fiber are taken into account. It is shown that this CM KdV equation has two-parameter families of bright and dark complex solitons. We show analytically that under certain conditions, the bright solitons are actually double-embedded solitons. We explain why these solitons do not radiate at all, even though their wave numbers are contained in the linear spectrum of the system. We study (numerically and analytically) the stability of these solitons. Our results show that these embedded solitons are stable solutions, which is an interesting property since in most systems the embedded solitons are weakly unstable solutions. Finally, we close the paper by making comments on the advantages as well as the limitations of our approach, and on further generalizations of the model and method presented. en_US
dc.language.iso en en_US
dc.title Standard and embedded solitons in nematic optical fibers en_US
dc.type Article en_US
dc.identifier.idprometeo 1939
dc.identifier.doi 10.1103/PhysRevE.68.036606
dc.source.novolpages 68(3)
dc.subject.wos Physics, Fluids & Plasmas
dc.subject.wos Physics, Mathematical
dc.description.index WoS: SCI, SSCI o AHCI
dc.relation.journal Physical Review E

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