dc.contributor.author |
Apurv Chaitanya, N. |
|
dc.contributor.author |
Jabir, M. V. |
|
dc.contributor.author |
Banerji, Jagannath |
|
dc.contributor.author |
Samanta, Goutam Kumar |
|
dc.date.accessioned |
2016-07-20T12:22:20Z |
|
dc.date.available |
2016-07-20T12:22:20Z |
|
dc.date.issued |
2016-06 |
|
dc.identifier.citation |
Apurv Chaitanya, N.; Jabir, M. V.; Banerji, J. and Samanta, G. K., “Hollow Gaussian beam generation through nonlinear interaction of photons with orbital-angular-momemtum”, arXiv, Cornell University Library, DOI: arXiv:1606.09005, Jun. 2016. |
en_US |
dc.identifier.uri |
https://repository.iitgn.ac.in/handle/123456789/2381 |
|
dc.identifier.uri |
http://arxiv.org/abs/1606.09005 |
|
dc.description.abstract |
Hollow Gaussian beams (HGB) are a special class of doughnut shaped beams that do not carry orbital angular momentum (OAM). Such beams have a wide range of applications in many fields including atomic optics, bio-photonics, atmospheric science, and plasma physics. Till date, these beams have been generated using linear optical elements. Here, we show a new way of generating HGBs by three-wave mixing in a nonlinear crystal. Based on nonlinear interaction of photons having OAM and conservation of OAM in nonlinear processes, we experimentally generated ultrafast HGBs of order as high as 6 and power >180 mW at 355 nm. This generic concept can be extended to any wavelength, timescales (continuous-wave and ultrafast) and any orders. We show that the removal of azimuthal phase of vortices does not produce Gaussian beam. We also propose a new and only method to characterize the order of the HGBs. |
en_US |
dc.description.statementofresponsibility |
by N. Apurv Chaitanya, M. V. Jabir, J. Banerji, G. K. Samanta |
|
dc.language.iso |
en_US |
en_US |
dc.publisher |
Cornell University Library |
en_US |
dc.title |
Hollow Gaussian beam generation through nonlinear interaction of photons with orbital-angular-momentum |
en_US |
dc.type |
Preprint |
en_US |