Synchronously-driven Microresonator Solitons and Application in Astronomy

被引:0
|
作者
Obrzud, E. [1 ,2 ]
Rainer, M. [3 ]
Harutyunyan, A. [4 ]
Anderson, M. H. [5 ]
Liu, J. [5 ]
Geiselmann, M. [5 ,6 ]
Chazelas, B. [2 ]
Kundermann, S. [1 ]
Lecomte, S. [1 ]
Cecconi, M. [4 ]
Ghedina, A. [4 ]
Molinari, E. [4 ,7 ]
Pepe, F. [2 ]
Wildi, F. [2 ]
Bouchy, F. [2 ]
Kippenberg, T. J. [5 ]
Herr, T. [1 ]
机构
[1] Swiss Ctr Elect & Microtechnol CSEM, Time & Frequency, Rue Observ 58, CH-2002 Neuchatel, Switzerland
[2] Univ Geneva, Dept Astron, Geneva Observ PlanetS, Chemin Maillettes 51, CH-1290 Versoix, Switzerland
[3] Natl Inst Astrophys INAF, Astron Observ Brera, Via Brera 28, I-20121 Milan, Italy
[4] Fdn Galileo Galilei INAF, Rambla Jose Ana Fernandez Perez 7, Brena Baja 38712, Santa Cruz De T, Spain
[5] Swiss Fed Inst Technol EPFL, SB IPHYS LPQM1, PH D3,Stn 3, CH-1015 Lausanne, Switzerland
[6] Ligentec, EPFL Innovat Pk,Batiment C, CH-1015 Lausanne, Switzerland
[7] INAF, Osservatorio Astron Cagliari, Via Sci 5, I-09047 Selargius, CA, Italy
基金
瑞士国家科学基金会;
关键词
FREQUENCY COMB; PRECISION;
D O I
暂无
中图分类号
TP301 [理论、方法];
学科分类号
081202 ;
摘要
Synchronous-driving of nonlinear optical microresonator offers robust, deterministic and ultra-efficient generation of ultra-short temporal soliton pulses as well as high-repetition rate frequency combs. The soliton pulses are all-optically controlled and provide resolvable lines for astronomical spectrometer calibration or optical telecommunications.
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页数:3
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