Soliton-induced relativistic-scattering and amplification

被引:43
作者
Rubino, E. [2 ]
Lotti, A. [2 ,3 ]
Belgiorno, F. [4 ]
Cacciatori, S. L. [2 ]
Couairon, A. [3 ]
Leonhardt, U. [5 ]
Faccio, D. [1 ]
机构
[1] Heriot Watt Univ, SUPA, Sch Engn & Phys Sci, Edinburgh EH14 4AS, Midlothian, Scotland
[2] Univ Insubria, Dipartimento Sci & Alta Tecnol, IT-22100 Como, Italy
[3] Ecole Polytech, Ctr Phys Theor CNRS, F-91128 Palaiseau, France
[4] Politecn Milan, Dipartimento Matemat, I-20133 Milan, Italy
[5] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland
基金
英国工程与自然科学研究理事会;
关键词
RADIATION; ANALOG; GENERATION; LIGHT;
D O I
10.1038/srep00932
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Solitons are of fundamental importance in photonics due to applications in optical data transmission and also as a tool for investigating novel phenomena ranging from light generation at new frequencies and wave-trapping to rogue waves. Solitons are also moving scatterers: they generate refractive index perturbations moving at the speed of light. Here we found that such perturbations scatter light in an unusual way: they amplify light by the mixing of positive and negative frequencies, as we describe using a first Born approximation and numerical simulations. The simplest scenario in which these effects may be observed is within the initial stages of optical soliton propagation: a steep shock front develops that may efficiently scatter a second, weaker probe pulse into relatively intense positive and negative frequency modes with amplification at the expense of the soliton. Our results show a novel all-optical amplification scheme that relies on soliton induced scattering.
引用
收藏
页数:4
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