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This paper proposes a method for controlling the topological structures in high-order optical vortices by employing a noncanonical phase structure. The control of the evolutions in high-order optical vortices by using a noncanonical phase structure with a nonuniform azimuthal gradient is studied numerically and experimentally. Results show that the propagation of high-order optical vortices along with a noncanonical phase structure becomes a decayed optical distribution with multiple one-charged singularities along a line. In addition, the control from the noncanonical phase structure can suppress random evolutions of topological structures resulted from the phase noise. These conclusions may indicate a new method to control the decay of high-order optical vortices, and promising potential applications in many fields, such as optical vortices-based optical communications and optical tweezers.
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Keywords:
- optical vortex /
- noncanonical phase /
- topological structure /
- phase noise
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[25] Cui Q, Li M, Yu Z 2014 Opt. Commun. 329 10
[26] Dennis M R, O'Holleran K, Padgett M J 2009 Progress in Opt. 53 293
[27] Molina-Terriza G, Wright E M, Torner L 2001 Opt. Lett. 26 163
[28] Kim G H, Lee H J, Kim J U 2003 JOSA B 20 351
[29] Basistiy I V, Soskin M S, Vasnetsov M V 1995 Opt. Commun. 119 604
[30] Sacks Z S, Rozas D, Swartzlander G A 1998 JOSA B 15 2226
[31] Ostrovsky A S, Rickenstorff-Parrao C, Arrizon V 2013 Opt. Lett. 38 534
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[34] Cui Q, Li M, Yu Z 2014 Opt. Commun. 329 10
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[1] Cullet P, Gil L, Rocca F 1989 Opt. Commun. 73 403
[2] Kivshar Y S, Ostrovskaya E A 2001 Opt. Photon. News 12 24
[3] Nye J F, Berry M V 1974 Phys. Engin. Sci. 336 165
[4] Ding P F, Pu J X 2012 Acta Phys. Sin. 61 174201 (in Chinese) [丁攀峰, 蒲继雄 2012 物理学报 61 174201]
[5] Fang G J, Sun S H, Pu J X 2012 Acta Phys. Sin. 61 064210 (in Chinese) [方桂娟, 孙顺红, 蒲继雄 2012 物理学报 61 064210]
[6] Gecevičius M, Drevinskas R, Beresna M, Kazansky P 2014 Appl. Phys. Lett. 104 231110
[7] Chen C R, Yeh C H, Shih M F 2014 Opt. Express 22 3180
[8] Dholakia K, Čžmár T 2011 Nature Photon. 5 335
[9] Fickler R, Lapkiewicz R, Plick W N, Krenn M, Schaeff C, Ramelow S, Zeilinger A 2012 Science 338 640
[10] Rodenburg B, Mirhosseini M, Malik M, Rodenburg B, Mirhosseini M, Malik M, Magaña-LoaizaO, Yanakas M, Maher L, Steinhoff N, Tyler G, Boyd R 2014 New Journal of Phys. 16 033020
[11] Lehmuskero A, Li Y, Johansson P 2014 Opt. Express 22 434
[12] Liu Y, Li H N, Hu Y, Du A 2014 Chin. Phys. B 23 087501
[13] Zhou Z H, Guo Y K, Zhu L 2014 Chin. Phys. B 23 044201
[14] Yarmchuk E J, Cordon M J V, Packard R E 1979 Phys. Rev. Lett. 43 214
[15] Gan X, Zhao J, Liu S, Fang L 2009 Chin. Opt. Lett. 7 1142
[16] Mamaev A V, Saffman M, Zozulya A 1997 Phys. Rev. Lett. 78 2108
[17] Gan X, Zhang P, Liu S, Zheng Y, Zhao J, Chen Z G 2009 Opt. Express 17 23130
[18] Vaity P, Singh R P 2012 Opt. Lett. 37 1301
[19] Denisenko V, Shvedov V, Desyatnikov A S, Neshev D, Krolikowski W, Volyar A, Soskin M, Kivshar Y S 2009 Opt. Express 17 23374
[20] Vuong L, Grow T, Ishaaya A, Gaeta A, Eliel E, Fibich G 2006 Phys. Rev. Lett. 96 133901
[21] Ouyang S G 2013 Acta Phys. Sin. 62 040504 (in Chinese) [欧阳世根 2013 物理学报 62 040504]
[22] Malik M, O'Sullivan M, Rodenburg B, Mirhosseini M, Leach J, Lavery M P, Padgett M J, Boyd R W 2012 Opt. Express 20 13195
[23] Reddy S G, Prabhakar S, Aadhi A, Banerji J, Singh R P 2014 JOSA A 31 1295
[24] Anguita J A, Rodriguez H, Quezada C 2014 Aerospace Conference IEEE 2014 p1
[25] Cui Q, Li M, Yu Z 2014 Opt. Commun. 329 10
[26] Dennis M R, O'Holleran K, Padgett M J 2009 Progress in Opt. 53 293
[27] Molina-Terriza G, Wright E M, Torner L 2001 Opt. Lett. 26 163
[28] Kim G H, Lee H J, Kim J U 2003 JOSA B 20 351
[29] Basistiy I V, Soskin M S, Vasnetsov M V 1995 Opt. Commun. 119 604
[30] Sacks Z S, Rozas D, Swartzlander G A 1998 JOSA B 15 2226
[31] Ostrovsky A S, Rickenstorff-Parrao C, Arrizon V 2013 Opt. Lett. 38 534
[32] Palacios D, Rozas D, Swartzlander Jr G A 2002 Phys. Rev. Lett. 88 103902
[33] Nye J F, Berry M V 1974 Mathematical and Physical Sciences 336 165
[34] Cui Q, Li M, Yu Z 2014 Opt. Commun. 329 10
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