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Proceedings Paper

Generation of optical frequency combs in fibres: an optical pulse analysis
Author(s): Marina Zajnulina; Michael Böhm; Keith Blow; José M. Chavez Boggio; Andres A. Rieznik; Roger Haynes; Martin M. Roth
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Paper Abstract

The innovation of optical frequency combs (OFCs) generated in passive mode-locked lasers has provided astronomy with unprecedented accuracy for wavelength calibration in high-resolution spectroscopy in research areas such as the discovery of exoplanets or the measurement of fundamental constants. The unique properties of OCFs, namely a highly dense spectrum of uniformly spaced emission lines of nearly equal intensity over the nominal wavelength range, is not only beneficial for high-resolution spectroscopy. Also in the low- to medium-resolution domain, the OFCs hold the promise to revolutionise the calibration techniques. Here, we present a novel method for generation of OFCs. As opposed to the mode-locked laser-based approach that can be complex, costly, and difficult to stabilise, we propose an all optical fibre-based system that is simple, compact, stable, and low-cost. Our system consists of three optical fibres where the first one is a conventional single-mode fibre, the second one is an erbium-doped fibre and the third one is a highly nonlinear low-dispersion fibre. The system is pumped by two equally intense continuous-wave (CW) lasers. To be able to control the quality and the bandwidth of the OFCs, it is crucial to understand how optical solitons arise out of the initial modulated CW field in the first fibre. Here, we numerically investigate the pulse evolution in the first fibre using the technique of the solitons radiation beat analysis. Having applied this technique, we realised that formation of higherorder solitons is supported in the low-energy region, whereas, in the high-energy region, Kuznetsov-Ma solitons appear.

Paper Details

Date Published: 18 July 2014
PDF: 7 pages
Proc. SPIE 9151, Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation, 91514V (18 July 2014); doi: 10.1117/12.2055554
Show Author Affiliations
Marina Zajnulina, Leibniz-Institut für Astrophysik Potsdam (Germany)
Michael Böhm, Univ. Potsdam (Germany)
Keith Blow, Aston Univ. (United Kingdom)
José M. Chavez Boggio, Leibniz-Institut für Astrophysik Potsdam (Germany)
Andres A. Rieznik, Instituto Tecnológico de Buenos Aires (Argentina)
Roger Haynes, Leibniz-Institut für Astrophysik Potsdam (Germany)
Martin M. Roth, Leibniz-Institut für Astrophysik Potsdam (Germany)


Published in SPIE Proceedings Vol. 9151:
Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation
Ramón Navarro; Colin R. Cunningham; Allison A. Barto, Editor(s)

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