diffuse media
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2021 ◽  
Vol 11 (1) ◽  
Author(s):  
Netanel Biton ◽  
Judy Kupferman ◽  
Shlomi Arnon

AbstractA major challenge in use of the optical spectrum for communication and imaging applications is the scattering of light as it passes through diffuse media. Recent studies indicate that light beams with orbital angular momentum (OAM) can penetrate deeper through diffuse media than simple Gaussian beams. To the best knowledge of the authors, in this paper we describe for the first time an experiment examining transmission of OAM beams through biological tissue with thickness of up to a few centimeters, and for OAM modes reaching up to 20. Our results indicate that OAM beams do indeed show a higher transmittance relative to Gaussian beams, and that the greater the OAM, the higher the transmittance also up to 20, Our results extend measured results to highly multi scattering media and indicate that at 2.6 cm tissue thickness for OAM of order 20, we measure nearly 30% more power in comparison to a Gaussian beam. In addition, we develop a mathematical model describing the improved permeability. This work shows that OAM beams can be a valuable contribution to optical wireless communication (OWC) for medical implants, optical biological imaging, as well as recent innovative applications of medical diagnosis.


2020 ◽  
Vol 2 (7) ◽  
pp. 403-410 ◽  
Author(s):  
Babak Rahmani ◽  
Damien Loterie ◽  
Eirini Kakkava ◽  
Navid Borhani ◽  
Uğur Teğin ◽  
...  

Author(s):  
John L. Holdsworth ◽  
Zachary T. Groth ◽  
Jordan V. Velich ◽  
Nigel P. Walters ◽  
Galiya Sharafutdinova ◽  
...  

2017 ◽  
Author(s):  
Claas Falldorf ◽  
Thorsten Klein ◽  
Mostafa Agour ◽  
Ralf B. Bergmann

2014 ◽  
Vol 22 (4) ◽  
pp. 4180 ◽  
Author(s):  
Martin Lošt’ák ◽  
Radim Chmelík ◽  
Michala Slabá ◽  
Tomáš Slabý

Author(s):  
Vera Kollarova ◽  
Martin Lostak ◽  
Michala Slaba ◽  
Tomas Slaby ◽  
Jana Collakova ◽  
...  
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2009 ◽  
Vol 5 (H15) ◽  
pp. 427-427
Author(s):  
Elisabete M. de Gouveia Dal Pino ◽  
Alex Lazarian

Most of the baryonic matter in the Universe is permeated by magnetic fields which affect many, if not most, of astrophysical phenomena both, in compact sources and in diffuse gas.


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