We report experimental and theoretical studies of Raman-induced cross-phase modulational instabilities (XPMI) in a high-birefringence, normally dispersive optical fiber. Experimental results reveal that the Raman-Stokes wave, generated by a quasi-CW pump beam, interacts with the latter to create a novel type of XPMI sidebands. These sidebands are characterized by a narrow gain bandwidth. The sideband frequencies are well reproduced by a linear stability analysis as well as by full numerical solutions of the coupled generalized nonlinear Schrödinger equations.

Cross-phase modulational instability induced by Raman scattering in highly birefringent fiber / F., Amrani; B., Kibler; Grelu, P. h.; Wabnitz, Stefan; S., Trillo; G., Millot. - In: OPTICS LETTERS. - ISSN 0146-9592. - 38:24(2013), pp. 5327-5330. [10.1364/OL.38.005327]

Cross-phase modulational instability induced by Raman scattering in highly birefringent fiber

WABNITZ, Stefan;
2013

Abstract

We report experimental and theoretical studies of Raman-induced cross-phase modulational instabilities (XPMI) in a high-birefringence, normally dispersive optical fiber. Experimental results reveal that the Raman-Stokes wave, generated by a quasi-CW pump beam, interacts with the latter to create a novel type of XPMI sidebands. These sidebands are characterized by a narrow gain bandwidth. The sideband frequencies are well reproduced by a linear stability analysis as well as by full numerical solutions of the coupled generalized nonlinear Schrödinger equations.
2013
Cross phase modulational instability; dinger equation; full numerical solution
01 Pubblicazione su rivista::01a Articolo in rivista
Cross-phase modulational instability induced by Raman scattering in highly birefringent fiber / F., Amrani; B., Kibler; Grelu, P. h.; Wabnitz, Stefan; S., Trillo; G., Millot. - In: OPTICS LETTERS. - ISSN 0146-9592. - 38:24(2013), pp. 5327-5330. [10.1364/OL.38.005327]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11573/1214630
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