Using a multipoint interferometer to measure the orbital angular momentum of light in astrophysics

被引:53
|
作者
Berkhout, G. C. G.
Beijersbergen, M. W.
机构
[1] Leiden Univ, Huygens Lab, NL-2300 RA Leiden, Netherlands
[2] Cosine Sci & Comp BV, NL-2333 CA Leiden, Netherlands
来源
JOURNAL OF OPTICS A-PURE AND APPLIED OPTICS | 2009年 / 11卷 / 09期
关键词
optical angular momentum; multipoint interferometer; detection; astrophysics; WAVE-FRONT; BEAMS; DISLOCATIONS;
D O I
10.1088/1464-4258/11/9/094021
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Recently it was shown that the orbital angular momentum of light can be measured using a multipoint interferometer, a system in which the light from several point measurements is interferometrically combined. This system has important applications in optics but could also be employed to detect astrophysical orbital angular momentum. Until now, the response of a multipoint interferometer to an on-axis, normally incident Laguerre-Gaussian beam has been studied by visual inspection. In this paper we present an algorithm to determine the orbital angular momentum of the impinging beam from the obtained interference patterns. Using this algorithm we extend our study to general optical vortices and a superposition of optical vortices.
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页数:7
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